371 results on '"Aryshev, A."'
Search Results
202. Feasibility of Double Diffraction Radiation Target Interferometry for Compact Linear Accelerator Micro-train Bunch Spacing Diagnostics
- Author
-
A. P. Potylitsyn, Junji Urakawa, Alexander Aryshev, and D. A. Shkitov
- Subjects
Physics ,Diffraction ,History ,business.industry ,Electron ,Radiation ,Linear particle accelerator ,Computer Science Applications ,Education ,Interferometry ,Optics ,Physics::Accelerator Physics ,business ,Energy (signal processing) - Abstract
In this paper the simulation of the interaction between micro-train electron beams with different parameters of energy, bunch length, bunch spacing which chosen for KEK LUCX accelerator facility and a double diffraction radiation target is considered. Calculation model and several accepted assumptions on the first step of our investigations are also described. Conducted researches allow us to conclude that applying the double diffraction radiation target interferometry as a tool for non-invasive micro-train bunch spacing diagnostics for compact linear accelerator is possible. more...
- Published
- 2014
- Full Text
- View/download PDF
203. Some Analytical Aspects of Business Integration
- Author
-
Ivanyuk, Tatyana, primary and Aryshev, Vasiliy, additional
- Published
- 2012
- Full Text
- View/download PDF
204. Cavity optimization for compact accelerator-based free-electron maser
- Author
-
Aryshev, A., primary, Verigin, D., additional, Araki, S., additional, Fukuda, M., additional, Karataev, P., additional, Naumenko, G., additional, Potylitsyn, A., additional, Sakaue, K., additional, Sukhikh, L., additional, Terunuma, N., additional, and Urakawa, J., additional more...
- Published
- 2012
- Full Text
- View/download PDF
205. Cavity beam position monitor system for the Accelerator Test Facility 2
- Author
-
Kim, Y. I., primary, Ainsworth, R., additional, Aryshev, A., additional, Boogert, S. T., additional, Boorman, G., additional, Frisch, J., additional, Heo, A., additional, Honda, Y., additional, Hwang, W. H., additional, Huang, J. Y., additional, Kim, E-S., additional, Kim, S. H., additional, Lyapin, A., additional, Naito, T., additional, May, J., additional, McCormick, D., additional, Mellor, R. E., additional, Molloy, S., additional, Nelson, J., additional, Park, S. J., additional, Park, Y. J., additional, Ross, M., additional, Shin, S., additional, Swinson, C., additional, Smith, T., additional, Terunuma, N., additional, Tauchi, T., additional, Urakawa, J., additional, and White, G. R., additional more...
- Published
- 2012
- Full Text
- View/download PDF
206. First Observation of the Point Spread Function of Optical Transition Radiation
- Author
-
Karataev, Pavel, primary, Aryshev, Alexander, additional, Boogert, Stewart, additional, Howell, David, additional, Terunuma, Nobuhiro, additional, and Urakawa, Junji, additional
- Published
- 2011
- Full Text
- View/download PDF
207. Micron-scale laser-wire scanner for the KEK Accelerator Test Facility extraction line
- Author
-
Boogert, Stewart T., primary, Blair, Grahame A., additional, Boorman, Gary, additional, Bosco, Alessio, additional, Deacon, Lawrence C., additional, Karataev, Pavel, additional, Aryshev, Alexander, additional, Fukuda, Masafumi, additional, Terunuma, Nobihiro, additional, Urakawa, Junji, additional, Corner, Laura, additional, Delerue, Nicolas, additional, Foster, Brian, additional, Howell, David, additional, Newman, Myriam, additional, Senanayake, Rohan, additional, Walczak, Roman, additional, and Ganaway, Fred, additional more...
- Published
- 2010
- Full Text
- View/download PDF
208. First beam waist measurements in the final focus beam line at the KEK Accelerator Test Facility
- Author
-
Bai, Sha, primary, Aryshev, Alexander, additional, Bambade, Philip, additional, Mc Cormick, Doug, additional, Bolzon, Benoit, additional, Gao, Jie, additional, Tauchi, Toshiaki, additional, and Zhou, Feng, additional more...
- Published
- 2010
- Full Text
- View/download PDF
209. A novel method for sub-micrometer transverse electron beam size measurements using optical transition radiation
- Author
-
Aryshev, A, primary, Boogert, S T, additional, Howell, D, additional, Karataev, P, additional, Terunuma, N, additional, and Urakawa, J, additional
- Published
- 2010
- Full Text
- View/download PDF
210. Development of microwave and soft X-ray sources based on coherent radiation and Thomson scattering
- Author
-
Aryshev, A, primary, Araki, A, additional, Fukuda, M, additional, Karataev, P, additional, Naumenko, G, additional, Potylitsyn, A, additional, Sakaue, K, additional, Sukhikh, L, additional, Urakawa, J, additional, and Verigin, D, additional more...
- Published
- 2010
- Full Text
- View/download PDF
211. Present status and first results of the final focus beam line at the KEK Accelerator Test Facility
- Author
-
Bambade, P., primary, Alabau Pons, M., additional, Amann, J., additional, Angal-Kalinin, D., additional, Apsimon, R., additional, Araki, S., additional, Aryshev, A., additional, Bai, S., additional, Bellomo, P., additional, Bett, D., additional, Blair, G., additional, Bolzon, B., additional, Boogert, S., additional, Boorman, G., additional, Burrows, P. N., additional, Christian, G., additional, Coe, P., additional, Constance, B., additional, Delahaye, J.-P., additional, Deacon, L., additional, Elsen, E., additional, Faus-Golfe, A., additional, Fukuda, M., additional, Gao, J., additional, Geffroy, N., additional, Gianfelice-Wendt, E., additional, Guler, H., additional, Hayano, H., additional, Heo, A.-Y., additional, Honda, Y., additional, Huang, J. Y., additional, Hwang, W. H., additional, Iwashita, Y., additional, Jeremie, A., additional, Jones, J., additional, Kamiya, Y., additional, Karataev, P., additional, Kim, E.-S., additional, Kim, H.-S., additional, Kim, S. H., additional, Komamiya, S., additional, Kubo, K., additional, Kume, T., additional, Kuroda, S., additional, Lam, B., additional, Lyapin, A., additional, Masuzawa, M., additional, McCormick, D., additional, Molloy, S., additional, Naito, T., additional, Nakamura, T., additional, Nelson, J., additional, Okamoto, D., additional, Okugi, T., additional, Oroku, M., additional, Park, Y. J., additional, Parker, B., additional, Paterson, E., additional, Perry, C., additional, Pivi, M., additional, Raubenheimer, T., additional, Renier, Y., additional, Resta-Lopez, J., additional, Rimbault, C., additional, Ross, M., additional, Sanuki, T., additional, Scarfe, A., additional, Schulte, D., additional, Seryi, A., additional, Spencer, C., additional, Suehara, T., additional, Sugahara, R., additional, Swinson, C., additional, Takahashi, T., additional, Tauchi, T., additional, Terunuma, N., additional, Tomas, R., additional, Urakawa, J., additional, Urner, D., additional, Verderi, M., additional, Wang, M.-H., additional, Warden, M., additional, Wendt, M., additional, White, G., additional, Wittmer, W., additional, Wolski, A., additional, Woodley, M., additional, Yamaguchi, Y., additional, Yamanaka, T., additional, Yan, Y., additional, Yoda, H., additional, Yokoya, K., additional, Zhou, F., additional, and Zimmermann, F., additional more...
- Published
- 2010
- Full Text
- View/download PDF
212. Observation of focusing effect in optical transition and diffraction radiation generated from a spherical target
- Author
-
Sukhikh, L. G., primary, Aryshev, A. S., additional, Karataev, P. V., additional, Naumenko, G. A., additional, Potylitsyn, A. P., additional, Terunuma, N., additional, and Urakawa, J., additional
- Published
- 2009
- Full Text
- View/download PDF
213. A novel method for sub-micrometer transverse electron beam size measurements using optical transition radiation
- Author
-
Stewart Boogert, Nobuhiro Terunuma, Alexander Aryshev, David Howell, J. Urakawa, and Pavel Karataev
- Subjects
Point spread function ,History ,Chemistry ,business.industry ,Resolution (electron density) ,Boundary (topology) ,Nanotechnology ,Dielectric ,Radiation ,Charged particle ,Computer Science Applications ,Education ,Transverse plane ,Optics ,Cathode ray ,business - Abstract
Optical Transition Radiation (OTR) appearing when a charged particle crosses a boundary between two media with different dielectric properties has widely been used as a tool for transverse profile measurements of charged particle beams in various facilities worldwide. The resolution of the monitor is defined by so-called Point Spread Function (PSF), source distribution generated by a single electron and projected by an optical system onto a screen. In this paper we represent the development of a novel sub-micrometre electron beam profile monitor based on the measurements of the PSF structure. The first experimental results are presented and future plans on the optimization of the monitor are discussed © 2010 IOP Publishing Ltd. more...
- Published
- 2010
- Full Text
- View/download PDF
214. Development of microwave and soft X-ray sources based on coherent radiation and Thomson scattering
- Author
-
D. Verigin, G. A. Naumenko, Kazuyuki Sakaue, Pavel Karataev, Alexander Aryshev, A. P. Potylitsyn, J. Urakawa, Leonid Sukhikh, Masafumi Fukuda, and A. Araki
- Subjects
Diffraction ,Physics ,History ,Thomson scattering ,Scattering ,business.industry ,Astrophysics::High Energy Astrophysical Phenomena ,Particle accelerator ,Radiation ,Undulator ,Laser ,Computer Science Applications ,Education ,law.invention ,Optics ,law ,Physics::Accelerator Physics ,business ,Microwave - Abstract
Compact, high-brightness and reliable sources in the VUV and the soft X-ray region may be used for numerous applications in medicine and biochemistry. We propose a new approach to produce the intense beams of X-rays in the range of ≤ 500 eV based on compact electron accelerator. We present our first experimental results obtained in the Laser Undulator Compact X-ray facility (LUCX) at KEK: High Energy Accelerator Research Organization devoted to the development of a compact microwave and soft X-ray source based on coherent diffraction radiation and Thompson scattering processes. more...
- Published
- 2010
- Full Text
- View/download PDF
215. Experimental observation and investigation of the prewave zone effect in optical diffraction radiation
- Author
-
Karataev, P., primary, Araki, S., additional, Aryshev, A., additional, Naumenko, G., additional, Potylitsyn, A., additional, Terunuma, N., additional, and Urakawa, J., additional
- Published
- 2008
- Full Text
- View/download PDF
216. Coherent transition and diffraction radiation from a bunched 6.1MeV electron beam
- Author
-
Naumenko, G.A., primary, Aleinik, A.N., additional, Aryshev, A.S., additional, Kalinin, B.N., additional, Potylitsyn, A.P., additional, Saruev, G.A., additional, and Sharafutdinov, A.F., additional
- Published
- 2005
- Full Text
- View/download PDF
217. Stimulated Smith–Purcell Radiation.
- Author
-
Ale&icaron;nik, A. N., Aryshev, A. S., Bogomazova, E. A., Kalinin, B. N., Naumenko, G. A., Potylitsyn, A. P., Saruev, G. A., and Sharafutdinov, A. F.
- Subjects
- *
FREE electron lasers , *SMITH-Purcell effect , *SUBMILLIMETER waves , *ELECTROMAGNETIC waves , *LASERS , *PHYSICS - Abstract
The design of free-electron lasers (FELs) based on submillimeter-range undulators involves difficulties associated with the fabrication of undulators with a very small period. To do this also requires accelerators with high-energy electron beams (>50 MeV). It should also be taken into account that these facilities use precision and expensive magnetic systems. In some works, an alternative FEL mechanism based on the use of the SmithPurcell radiation (SPR) was considered. To realize the feedback in such an FEL, one must use a basically different cavity scheme. This work reports the results of experimental study on the stimulated SPR in a ‘transverse’ cavity. [ABSTRACT FROM AUTHOR] more...
- Published
- 2004
- Full Text
- View/download PDF
218. Beam Test Proposal of an ODR Beam Size Monitor at SLAC FFTB.
- Author
-
Fukui, Y., Cline, D., Feng Zhou, Ross, M., Bolton, P., Urakawa, J., Tobiyama, M., Muto, T., Karataev, P., Aryshev, A., Hamatsu, R., Potylitsyn, A., Naumenko, G., and Sharafutdinov, A.
- Published
- 2005
- Full Text
- View/download PDF
219. The Possibility of Noninvasive Micron High Energy Electron Beam Size Measurement Using Diffraction Radiation.
- Author
-
Naumenko, G., Potylitsyn, A., Araki, S., Aryshev, A., Hayano, H., Karataev, P., Muto, T., Urakawa, J., Ross, M., Cline, D., Fukui, Y., and Hamatsu, R.
- Published
- 2005
- Full Text
- View/download PDF
220. Transient radiation of the charged particles bunch.
- Author
-
V.A. Nagorny and A.S. Aryshev
- Published
- 2003
- Full Text
- View/download PDF
221. Stability of colliding flows
- Author
-
Yu. A. Aryshev, V. A. Golovin, and Sh. A. Ershin
- Subjects
Physics::Fluid Dynamics ,Fluid Flow and Transfer Processes ,Physics ,Classical mechanics ,Flow (mathematics) ,Mechanical Engineering ,Linear system ,General Physics and Astronomy ,Perfect fluid ,Conservative vector field ,Stability (probability) - Abstract
The stability of the flow in the interaction region of colliding streams is investigated in the framework of linear theory. To simplify the analysis, the treatment is restricted to the case of an ideal fluid and an irrotational main flow. more...
- Published
- 1981
- Full Text
- View/download PDF
222. Development of a Fast Microwave Detection System and its Application to CSR Measurements
- Author
-
ARYSHEV, Alexander and Alexander , ARYSHEV
223. Stimulated emission of THz coherent diffraction radiation in an optical cavity by a multibunch electron beam.
- Author
-
Y. Honda, A. Aryshev, R. Kato, T. Miyajima, T. Obina, M. Shimada, R. Takai, T. Uchiyama, and N. Yamamoto
- Published
- 2019
- Full Text
- View/download PDF
224. Pre-bunched electron beam emittance simulation and measurement
- Author
-
Kliuchevskaia, Yulia, Aryshev, Alexander, Polozov, Sergey, Shevelev, Mikhail, Terunuma, Nobuhiro, and Urakawa, Junji
- Subjects
Physics::Accelerator Physics ,02 Photon Sources and Electron Accelerators ,Accelerator Physics - Abstract
LUCX facility at KEK is used as the high brightness pre-bunched electron beam source for radiation experiments. Emittance measurement and optimization is one of the important research activities for newly developed operation mode of the facility. Characterization of the pre-bunched beam (THz sequence of a hundred femtosecond bunches) properties opens a possibility to establish detailed simulation of the THz FEL radiation yield and continuously improve pre-bunched beam dynamics insight. Emittance has been measured by the Q-scan method. The measurement results and possible ways of emittance optimization are discussed. The measurement results are compared with beam dynamics simulation done by self-consistent BEAMDULAC-BL code., Proceedings of the 7th Int. Particle Accelerator Conf., IPAC2016, Busan, Korea more...
225. Experimental investigation of THz Smith-Purcell radiation from composite corrugated capillary
- Author
-
Lekomtsev, Konstantin, Aryshev, Alexander, Ponomarenko, Aleksandr, Shevelev, Mikhail, Terunuma, Nobuhiro, Tishchenko, Alexey, and Urakawa, Junji
- Subjects
Physics::Optics ,Physics::Accelerator Physics ,02 Photon Sources and Electron Accelerators ,Accelerator Physics - Abstract
Terahertz part of electromagnetic spectrum has a variety of potential applications ranging from fundamental to security applications. Further advances in development of a linac based, tunable, and narrow band coherent source of THz radiation are very important. Mechanisms of Cherenkov radiation and Smith-Purcell radiation (SPR) [*] may be used for generation of THz radiation via coherent emission [**, ***]. In this report we will present experimental investigations of the SPR generated from the corrugated capillary with a reflector, using the femtosecond multi-bunch electron beam of LUCX accelerator at KEK, Japan [****]. LUCX is capable to generate a train of 4 bunches each with 200 femtosecond (60 micrometer) duration and 200 micrometer transverse size. We will discuss the composite design of the capillary, measurements of the SPR angular distributions and the comparison of these measurements with PIC simulations. In addition, we will discuss SPR spectral characteristics; bunch energy modulation, introduced by the corrugated capillary; and the way in which the bunch spacing changes the spectrum and angular distributions of SPR., Proceedings of the 7th Int. Particle Accelerator Conf., IPAC2016, Busan, Korea more...
226. Generation of soft X-ray radiation using Thomson scattering of coherent diffraction radiation by a short electron bunch
- Author
-
Potylitsyn, A. P., Kostousov, A. S., Sukhikh, L. G., Urakawa, J., Aryshev, A. S., Boogert, S., and Pavel Karataev
227. Development of Self-Resonating Enhancement Cavity Operating in Single-Longitudinal-Mode
- Author
-
Tsunehiko Omori, Yuji Hosaka, Tohru Takahashi, Shunichi Sato, Yuuki Uesugi, Masakazu Washio, Seiya Otsuka, Masafumi Fukuda, Junji Urakawa, Nobuhiro Terunuma, Alexander Aryshev, and Yuya Koshiba
- Subjects
Cavity resonance ,Physics ,Amplified spontaneous emission ,Disturbance (geology) ,High power lasers ,business.industry ,Feedback control ,02 engineering and technology ,021001 nanoscience & nanotechnology ,01 natural sciences ,010309 optics ,Longitudinal mode ,Finesse ,Optics ,0103 physical sciences ,0210 nano-technology ,business ,Laser light - Abstract
A single-longitudinal-mode operation of a self-resonating enhancement cavity with the finesse of 524 was achieved without any feedback control, demonstrating a capability to automaticaly follow the cavity resonance frequency against environmental disturbance. more...
228. A compact soft X-ray source based on thomson scattering of Coherent Diffraction Radiation
- Author
-
Aryshev, Alexander, Araki, Sakae, Fukuda, Masafumi, Karataev, Pavel, Naumenko, Gennady, Potylitsyn, Alexander, Sakaue, Kazuyuki, Sukhikh, Leonid, Urakawa, Junji, and Verigin, Dan
- Subjects
U05 Applications, Other ,08 Applications of Accelerators, Technology Transfer and Industrial Relations ,Accelerator Physics - Abstract
High-brightness and reliable sources in the VUV and the soft X-ray region may be used for numerous applications in such areas as medicine, biology, biochemistry, material science, etc. 4th generation light sources based on X-ray free electron lasers are being built in a few world’s leading laboratories. However, those installations are very expensive and the access to wider community is very limited. We propose a new approach to produce the intense beams of X-rays in the range of less than 500 eV based on compact electron accelerator. An ultimate goal of the project is to create a compact soft X-ray source based on Thomson scattering of Coherent Diffraction Radiation (CDR) using a small accelerator machine. CDR is generated when a charged particle moves in the vicinity of an obstacle. The radiation is coherent when its wavelength is comparable to or longer than the bunch length. The CDR waves will be generated in an opened resonator formed by two mirrors. In this report we represent the status of the experiment. The pilot experimental results and general hardware design will be demonstrated., Proceedings of the 1st International Particle Accelerator Conference, IPAC2010, Kyoto, Japan more...
229. Optical polarization radiation of relativistic electrons in conducting targets
- Author
-
Naumenko, G. A., Aleinik, A. F., Aryshev, A. S., Kalinin, B. N., Pavel Karataev, Potylitsyn, A. P., Saruev, G. A., Chefonov, O. V., and Sharafutdinov, A. N.
230. The Compact Linear Collider (CLIC) - 2018 Summary Report
- Author
-
CLICdp collaborations, The CLIC, Charles, T. K., Giansiracusa, P. J., Lucas, T. G., Rassool, R. P., Volpi, M., Balazs, C., Afanaciev, K., Makarenko, V., Patapenka, A., Zhuk, I., Collette, C., Boland, M. J., Hoffman, A. C. Abusleme, Diaz, M. A., Garay, F., Chi, Y., He, X., Pei, G., Pei, S., Shu, G., Wang, X., Zhang, J., Zhao, F., Zhou, Z., Chen, H., Gao, Y., Huang, W., Kuang, Y. P., Li, B., Li, Y., Meng, X., Shao, J., Shi, J., Tang, C., Wang, P., Wu, X., Zha, H., Ma, L., Han, Y., Fang, W., Gu, Q., Huang, D., Huang, X., Tan, J., Wang, Z., Zhao, Z., Uggerhøj, U. I., Wistisen, T. N., Aabloo, A., Aare, R., Kuppart, K., Vigonski, S., Zadin, V., Aicheler, M., Baibuz, E., Brücken, E., Djurabekova, F., Eerola, P., Garcia, F., Haeggström, E., Huitu, K., Jansson, V., Kassamakov, I., Kimari, J., Kyritsakis, A., Lehti, S., Meriläinen, A., Montonen, R., Nordlund, K., Österberg, K., Saressalo, A., Väinölä, J., Veske, M., Farabolini, W., Mollard, A., Peauger, F., Plouin, J., Bambade, P., Chaikovska, I., Chehab, R., Delerue, N., Davier, M., Faus-Golfe, A., Irles, A., Kaabi, W., LeDiberder, F., Pöschl, R., Zerwas, D., Aimard, B., Balik, G., J. -J. Blaising, Brunetti, L., Chefdeville, M., Dominjon, A., Drancourt, C., Geoffroy, N., Jacquemier, J., Jeremie, A., Karyotakis, Y., Nappa, J. M., Serluca, M., Vilalte, S., Vouters, G., Bernhard, A., Bründermann, E., Casalbuoni, S., Hillenbrand, S., Gethmann, J., Grau, A., Huttel, E., Müller, A.-S., Peiffer, P., Perić, I., Jauregui, D. Saez de, Emberger, L., Graf, C., Simon, F., Szalay, M., Kolk, N. van der, Brass, S., Kilian, W., Alexopoulos, T., Apostolopoulos, T., Gazis, E. N., Gazis, N., Kostopoulos, V., Kourkoulis, S., Heilig, B., Lichtenberger, J., Shrivastava, P., Dayyani, M. K., Ghasem, H., Hajari, S. S., Shaker, H., Ashkenazy, Y., Popov, I., Engelberg, E., Yashar, A., Abramowicz, H., Benhammou, Y., Borysov, O., Borysova, M., Levy, A., Levy, I., Alesini, D., Bellaveglia, M., Buonomo, B., Cardelli, A., Diomede, M., Ferrario, M., Gallo, A., Ghigo, A., Giribono, A., Piersanti, L., Stella, A., Vaccarezza, C., Blas, J. de, Franceschini, R., D’Auria, G., Mitri, S. Di, Abe, T., Aryshev, A., Fukuda, M., Furukawa, K., Hayano, H., Higashi, Y., Higo, T., Kubo, K., Kuroda, S., Matsumoto, S., Michizono, S., Naito, T., Okugi, T., Shidara, T., Tauchi, T., Terunuma, N., Urakawa, J., Yamamoto, A., Raboanary, R., Luiten, O. J., Stragier, X. F. D., Hart, R., Graaf, H. van der, Eigen, G., Adli, E., Lindstrøm, C. A., Lillestøl, R., Malina, L., Pfingstner, J., Sjobak, K. N., Ahmad, A., Hoorani, H., Khan, W. A., Bugiel, S., Bugiel, R., Firlej, M., Fiutowski, T. A., Idzik, M., Moroń, J., Świentek, K. P., Renstrom, P. Brückman de, Krupa, B., Kucharczyk, M., Lesiak, T., Pawlik, B., Sopicki, P., Turbiarz, B., Wojtoń, T., Zawiejski, L. K., Kalinowski, J., Nowak, K., Żarnecki, A. F., Firu, E., Ghenescu, V., Neagu, A. T., Preda, T., Zgura, I. S., Aloev, A., Azaryan, N., Boyko, I., Budagov, J., Chizhov, M., Filippova, M., Glagolev, V., Gongadze, A., Grigoryan, S., Gudkov, D., Karjavine, V., Lyablin, M., Nefedov, Yu, Olyunin, A., Rymbekova, A., Samochkine, A., Sapronov, A., Shelkov, G., Shirkov, G., Soldatov, V., Solodko, E., Trubnikov, G., Tyapkin, I., Uzhinsky, V., Vorozhtov, A., Zhemchugov, A., Levichev, E., Mezentsev, N., Piminov, P., Shatilov, D., Vobly, P., Zolotarev, K., Jelisavčić, I. Božović, Kačarević, G., Dumbelović, G. Milutinović, Pandurović, M., Radulović, M., Stevanović, J., Vukasinović, N., D. -H. Lee, Ayala, N., Benedetti, G., Guenzel, T., Iriso, U., Marti, Z., Perez, F., Pont, M., Trenado, J., Ruiz-Jimeno, A., Vila, I., Calero, J., Dominguez, M., Garcia-Tabares, L., Gavela, D., Lopez, D., Toral, F., Gutierrez, C. Blanch, Boronat, M., Esperante, D., Fullana, E., Fuster, J., García, I., Gimeno, B., Lopez, P. Gomis, González, D., Perelló, M., Ros, E., Villarejo, M. A., Vnuchenko, A., Vos, M., Borgmann, Ch, Brenner, R., Ekelöf, T., Jacewicz, M., Olvegård, M., Ruber, R., Ziemann, V., Aguglia, D., Gonzalvo, J. Alabau, Leon, M. Alcaide, Tehrani, N. Alipour, Anastasopoulos, M., Andersson, A., Andrianala, F., Antoniou, F., Apyan, A., Arominski, D., Artoos, K., Assly, S., Atieh, S., Baccigalupi, C., Sune, R. Ballabriga, Caballero, D. Banon, Barnes, M. J., Garcia, J. Barranco, Bartalesi, A., Bauche, J., Bayar, C., Belver-Aguilar, C., Morell, A. Benot, Bernardini, M., Bett, D. R., Bettoni, S., Bettencourt, M., Bielawski, B., Garcia, O. Blanco, Kraljevic, N. Blaskovic, Bolzon, B., Bonnin, X. A., Bozzini, D., Branger, E., Brondolin, E., Brunner, O., Buckland, M., Bursali, H., Burkhardt, H., Caiazza, D., Calatroni, S., Campbell, M., Lasheras, N. Catalan, Cassany, B., Castro, E., Soares, R. H. Cavaleiro, Bastos, M. Cerqueira, Cherif, A., Chevallay, E., Cilento, V., Corsini, R., Costa, R., Cure, B., Curt, S., Gobbo, A. Dal, Dannheim, D., Daskalaki, E., Deacon, L., Degiovanni, A., Michele, G. De, Oliveira, L. De, Romano, V. Del Pozo, Delahaye, J. P., Delikaris, D., Almeida, P. G. Dias de, Dobers, T., Doebert, S., Doytchinov, I., Draper, M., Ramos, F. Duarte, Duquenne, M., Plaja, N. Egidos, Elsener, K., Esberg, J., Esposito, M., Evans, L., Fedosseev, V., Ferracin, P., Fiergolski, A., Foraz, K., Fowler, A., Friebel, F., Fuchs, J.-F., Gaddi, A., Gamba, D., Fajardo, L. Garcia, Morales, H. Garcia, Garion, C., Gasior, M., Gatignon, L., Gayde, J.-C., Gerbershagen, A., Gerwig, H., Giambelli, G., Gilardi, A., Goldblatt, A. N., Anton, S. Gonzalez, Grefe, C., Grudiev, A., Guerin, H., Guillot-Vignot, F. G., Gutt-Mostowy, M. L., Lutz, M. Hein, Hessler, C., Holma, J. K., Holzer, E. B., Hourican, M., Hynds, D., Ikarios, E., Levinsen, Y. Inntjore, Janssens, S., Jeff, A., Jensen, E., Jonker, M., Kamugasa, S. W., Kastriotou, M., Kemppinen, J. M. K., Khan, V., Kieffer, R. B., Klempt, W., Kokkinis, N., Kossyvakis, I., Kostka, Z., Korsback, A., Platia, E. Koukovini, Kovermann, J. W., Kozsar, C.-I., Kremastiotis, I., Kröger, J., Kulis, S., Latina, A., Leaux, F., Lebrun, P., Lefevre, T., Leogrande, E., Linssen, L., Liu, X., Cudie, X. Llopart, Magnoni, S., Maidana, C., Maier, A. A., Durand, H. Mainaud, Mallows, S., Manosperti, E., Marelli, C., Lacoma, E. Marin, Marsh, S., Martin, R., Martini, I., Martyanov, M., Mazzoni, S., Mcmonagle, G., Mether, L. M., Meynier, C., Modena, M., Moilanen, A., Mondello, R., Cabral, P. B. Moniz, Irazabal, N. Mouriz, Munker, M., Muranaka, T., Nadenau, J., Navarro, J. G., Quirante, J. L. Navarro, Busto, E. Nebo Del, Nikiforou, N., Ninin, P., Nonis, M., Nisbet, D., Nuiry, F. X., Nürnberg, A., Ögren, J., Osborne, J., Ouniche, A. C., Pan, R., Papadopoulou, S., Papaphilippou, Y., Paraskaki, G., Pastushenko, A., Passarelli, A., Patecki, M., Pazdera, L., Pellegrini, D., Pepitone, K., Codina, E. Perez, Fontenla, A. Perez, Persson, T. H. B., Petrič, M., Pitman, S., Pitters, F., Pittet, S., Plassard, F., Popescu, D., Quast, T., Rajamak, R., Redford, S., Remandet, L., Renier, Y., Rey, S. F., Orozco, O. Rey, Riddone, G., Castro, E. Rodriguez, Roloff, P., Rossi, C., Rossi, F., Rude, V., Ruehl, I., Rumolo, G., Sailer, A., Sandomierski, J., Santin, E., Sanz, C., Bedolla, J. Sauza, Schnoor, U., Schmickler, H., Schulte, D., Senes, E., Serpico, C., Severino, G., Shipman, N., Sicking, E., Simoniello, R., Skowronski, P. K., Mompean, P. Sobrino, Soby, L., Sollander, P., Solodko, A., Sosin, M. P., Spannagel, S., Sroka, S., Stapnes, S., Sterbini, G., Stern, G., Ström, R., Stuart, M. J., Syratchev, I., Szypula, K., Tecker, F., Thonet, P. A., Thrane, P., Timeo, L., Tiirakari, M., Garcia, R. Tomas, Tomoiaga, C. I., Valerio, P., Vaňát, T., Vamvakas, A. L., Hoorne, J. Van, Viazlo, O., Pinto, M. Vicente Barreto, Vitoratou, N., Vlachakis, V., Weber, M. A., Wegner, R., Wendt, M., Widorski, M., Williams, O. E., Williams, M., Woolley, B., Wuensch, W., Wulzer, A., Uythoven, J., Xydou, A., Yang, R., Zelios, A., Zhao, Y., Zisopoulos, P., Benoit, M., Sultan, D. M. S., Riva, F., Bopp, M., Braun, H. H., Craievich, P., Dehler, M., Garvey, T., Pedrozzi, M., Raguin, J. Y., Rivkin, L., Zennaro, R., Guillaume, S., Rothacher, M., Aksoy, A., Nergiz, Z., Yavas, Ö., Denizli, H., Keskin, U., Oyulmaz, K. Y., Senol, A., Ciftci, A. K., Baturin, V., Karpenko, O., Kholodov, R., Lebed, O., Lebedynskyi, S., Mordyk, S., Musienko, I., Profatilova, Ia, Storizhko, V., Bosley, R. R., Price, T., Watson, M. F., Watson, N. K., Winter, A. G., Goldstein, J., Green, S., Marshall, J. S., Thomson, M. A., Xu, B., You, T., Gillespie, W. A., Spannowsky, M., Beggan, C., Martin, V., Zhang, Y., Protopopescu, D., Robson, A., Apsimon, R. J., Bailey, I., Burt, G. C., Dexter, A. C., Edwards, A. V., Hill, V., Jamison, S., Millar, W. L., Papke, K., Casse, G., Vossebeld, J., Aumeyr, T., Bergamaschi, M., Bobb, L., Bosco, A., Boogert, S., Boorman, G., Cullinan, F., Gibson, S., Karataev, P., Kruchinin, K., Lekomtsev, K., Lyapin, A., Nevay, L., Shields, W., Snuverink, J., Towler, J., Yamakawa, E., Boisvert, V., West, S., Jones, R., Joshi, N., Bett, D., Bodenstein, R. M., Bromwich, T., Burrows, P. N., Christian, G. B., Gohil, C., Korysko, P., Paszkiewicz, J., Perry, C., Ramjiawan, R., Roberts, J., Coates, T., Salvatore, F., Bainbridge, A., Clarke, J. A., Krumpa, N., Shepherd, B. J. A., Walsh, D., Chekanov, S., Demarteau, M., Gai, W., Liu, W., Metcalfe, J., Power, J., Repond, J., Weerts, H., Xia, L., Zupan, J., Wells, J. D., Zhang, Z., Adolphsen, C., Barklow, T., Dolgashev, V., Franzi, M., Graf, N., Hewett, J., Kemp, M., Kononenko, O., Markiewicz, T., Moffeit, K., Neilson, J., Nosochkov, Y., Oriunno, M., Phinney, N., Rizzo, T., Tantawi, S., Wang, J., Weatherford, B., White, G., and Woodley, M. more...
- Subjects
Technology ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,ddc:600 ,Accelerators and Storage Rings ,physics.acc-ph - Abstract
The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improv The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^−$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively, for a site length ranging from 11 km to 50 km. CLIC uses a two-beam acceleration scheme, in which normal-conducting high-gradient 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in significant progress in recent years. Moreover, this has led to an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept, which matches the physics performance requirements and the CLIC experimental conditions, has been refined using improved software tools for simulation and reconstruction. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations with overlay of beam-induced backgrounds, and through parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25–30 years. The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^-$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively. CLIC uses a two-beam acceleration scheme, in which 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept has been refined using improved software tools. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations and parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25-30 years. more...
231. Cs2Te photocathode response time measurements and femtosecond comb electron beam generation as a milestone towards pre-bunched THz FEL realization
- Author
-
Alexander Aryshev, Honda, Y., Lekomtsev, K., Shevelev, M., Terunuma, N., and Urakawa, J.
232. ILC Reference Design Report Volume 3 - Accelerator
- Author
-
Phinney, Nan, Toge, Nobukazu, Walker, Nicholas J., Aarons, Gerald, Abe, Toshinori, Abernathy, Jason, Ablikim, Medina, Abramowicz, Halina, Adey, David, Adloff, Catherine, Adolphsen, Chris, Afanaciev, Konstantin, Agapov, Ilya, Ahn, Jung-Keun, Aihara, Hiroaki, Akemoto, Mitsuo, Del Carmen Alabau, Maria, Albert, Justin, Albrecht, Hartwig, Albrecht, Michael, Alesini, David, Alexander, Gideon, Alexander, Jim, Allison, Wade, Amann, John, Amirikas, Ramila, An, Qi, Anami, Shozo, Ananthanarayan, B., Anderson, Terry, Andricek, Ladislav, Anduze, Marc, Anerella, Michael, Anfimov, Nikolai, Angal-Kalinin, Deepa, Antipov, Sergei, Antoine, Claire, Aoki, Mayumi, Aoza, Atsushi, Aplin, Steve, Appleby, Rob, Arai, Yasuo, Araki, Sakae, Arkan, Tug, Arnold, Ned, Arnold, Ray, Arnowitt, Richard, Artru, Xavier, Arya, Kunal, Aryshev, Alexander, Asakawa, Eri, Asiri, Fred, Asner, David, Atac, Muzaffer, Atoian, Grigor, Attié, David, Augustin, Jean-Eudes, Augustine, David B., Ayres, Bradley, Aziz, Tariq, Baars, Derek, Badaud, Frederique, Baddams, Nigel, Bagger, Jonathan, Bai, Sha, Bailey, David, Bailey, Ian R., Baker, David, Balalykin, Nikolai I., Balbuena, Juan Pablo, Baldy, Jean-Luc, Ball, Markus, Ball, Maurice, Ballestrero, Alessandro, Ballin, Jamie, Baltay, Charles, Bambade, Philip, Ban, Syuichi, Band, Henry, Bane, Karl, Banerjee, Bakul, Barbanotti, Serena, Barbareschi, Daniele, Barbaro-Galtieri, Angela, Barber, Desmond P., Barbi, Mauricio, Bardin, Dmitri Y., Barish, Barry, Barklow, Timothy L., Barlow, Roger, Barnes, Virgil E., Barone, Maura, Bartels, Christoph, Bartsch, Valeria, Basu, Rahul, Battaglia, Marco, Batygin, Yuri, Baudot, Jerome, Baur, Ulrich, Elwyn Baynham, D., Beard, Carl, Bebek, Chris, Bechtle, Philip, Becker, Ulrich J., Bedeschi, Franco, Bedjidian, Marc, Behera, Prafulla, Behnke, Ties, Bellantoni, Leo, Bellerive, Alain, Bellomo, Paul, Bentson, Lynn D., Benyamna, Mustapha, Bergauer, Thomas, Berger, Edmond, Bergholz, Matthias, Beri, Suman, Berndt, Martin, Bernreuther, Werner, Bertolini, Alessandro, Besancon, Marc, Besson, Auguste, Beteille, Andre, Bettoni, Simona, Beyer, Michael, Bhandari, R. K., Bharadwaj, Vinod, Bhatnagar, Vipin, Bhattacharya, Satyaki, Bhattacharyya, Gautam, Bhattacherjee, Biplob, Bhuyan, Ruchika, Bi, Xiao-Jun, Biagini, Marica, Bialowons, Wilhelm, Biebel, Otmar, Bieler, Thomas, Bierwagen, John, Birch, Alison, Bisset, Mike, Biswal, S. S., Blackmore, Victoria, Blair, Grahame, Blanchard, Guillaume, Blazey, Gerald, Blue, Andrew, Blümlein, Johannes, Boffo, Christian, Bohn, Courtlandt, Boiko, V. I., Boisvert, Veronique, Bondarchuk, Eduard N., Boni, Roberto, Bonvicini, Giovanni, Boogert, Stewart, Boonekamp, Maarten, Boorman, Gary, Borras, Kerstin, Bortoletto, Daniela, Bosco, Alessio, Bosio, Carlo, Bosland, Pierre, Bosotti, Angelo, Boudry, Vincent, Boumediene, Djamel-Eddine, Bouquet, Bernard, Bourov, Serguei, Bowden, Gordon, Bower, Gary, Boyarski, Adam, Bozovic-Jelisavcic, Ivanka, Bozzi, Concezio, Brachmann, Axel, Bradshaw, Tom W., Brandt, Andrew, Brasser, Hans Peter, Brau, Benjamin, Brau, James E., Breidenbach, Martin, Bricker, Steve, Brient, Jean-Claude, Brock, Ian, Brodsky, Stanley, Brooksby, Craig, Broome, Timothy A., Brown, David, Brownell, James H., Bruchon, Mélanie, Brueck, Heiner, Brummitt, Amanda J., Brun, Nicole, Buchholz, Peter, Budagov, Yulian A., Bulgheroni, Antonio, Bulyak, Eugene, Bungau, Adriana, Bürger, Jochen, Burke, Dan, Burkhart, Craig, Burrows, Philip, Burt, Graeme, Burton, David, Büsser, Karsten, Butler, John, Butterworth, Jonathan, Buzulutskov, Alexei, Cabruja, Enric, Caccia, Massimo, Cai, Yunhai, Calcaterra, Alessandro, Caliier, Stephane, Camporesi, Tiziano, Cao, Jun-Jie, Cao, J. S., Capatina, Ofelia, Cappellini, Chiara, Carcagno, Ruben, Carena, Marcela, Carloganu, Cristina, Carosi, Roberto, Stephen Carr, F., Carrion, Francisco, Carter, Harry F., Carter, John, Carwardine, John, Cassel, Richard, Cassell, Ronald, Cavallari, Giorgio, Cavallo, Emanuela, Cembranos, Jose A. R., Chakraborty, Dhiman, Chandez, Frederic, Charles, Matthew, Chase, Brian, Chattopadhyay, Subhasis, Chauveau, Jacques, Chefdeville, Maximilien, Chehab, Robert, Chel, Stéphane, Chelkov, Georgy, Chen, Chiping, Chen, He Sheng, Chen, Huai Bi, Chen, Jia Er, Chen, Sen Yu, Chen, Shaomin, Chen, Shenjian, Chen, Xun, Chen, Yuan Bo, Cheng, Jian, Chevallier, M., Chi, Yun Long, Chickering, William, Cho, Gi-Chol, Cho, Moo-Hyun, Choi, Jin-Hyuk, Choi, Jong Bum, Choi, Seong Youl, Choi, Young-Il, Choudhary, Brajesh, Choudhury, Debajyoti, Rai Choudhury, S., Christian, David, Christian, Glenn, Christophe, Grojean, Chung, Jin-Hyuk, Church, Mike, Ciborowski, Jacek, Cihangir, Selcuk, Ciovati, Gianluigi, Clarke, Christine, Clarke, Don G., Clarke, James A., Clements, Elizabeth, Coca, Cornelia, Coe, Paul, Cogan, John, Colas, Paul, Collard, Caroline, Colledani, Claude, Combaret, Christophe, Comerma, Albert, Compton, Chris, Constance, Ben, Conway, John, Cook, Ed, Cooke, Peter, Cooper, William, Corcoran, Sean, Cornat, Rémi, Corner, Laura, Cortina Gil, Eduardo, Clay Corvin, W., Cotta Ramusino, Angelo, Cowan, Ray, Crawford, Curtis, Cremaldi, Lucien M., Crittenden, James A., Cussans, David, Cvach, Jaroslav, Da Silva, Wilfrid, Dabiri Khah, Hamid, Dabrowski, Anne, Dabrowski, Wladyslaw, Dadoun, Olivier, Dai, Jian Ping, Dainton, John, Daly, Colin, Damerell, Chris, Danilov, Mikhail, Daniluk, Witold, Daram, Sarojini, Datta, Anindya, Dauncey, Paul, David, Jacques, Davier, Michel, Davies, Ken P., Dawson, Sally, Boer, Wim, Curtis, Stefania, Groot, Nicolo, La Taille, Christophe, Lira, Antonio, Roeck, Albert, Sangro, Riccardo, Santis, Stefano, Deacon, Laurence, Deandrea, Aldo, Dehmelt, Klaus, Delagnes, Eric, Delahaye, Jean-Pierre, Delebecque, Pierre, Delerue, Nicholas, Delferriere, Olivier, Demarteau, Marcel, Deng, Zhi, Denisov, Yu N., Densham, Christopher J., Desch, Klaus, Deshpande, Nilendra, Devanz, Guillaume, Devetak, Erik, Dexter, Amos, Di Benedetto, Vito, Diéguez, Angel, Diener, Ralf, Dinh, Nguyen Dinh, Dixit, Madhu, Dixit, Sudhir, Djouadi, Abdelhak, Dolezal, Zdenek, Dollan, Ralph, Dong, Dong, Dong, Hai Yi, Dorfan, Jonathan, Dorokhov, Andrei, Doucas, George, Downing, Robert, Doyle, Eric, Doziere, Guy, Drago, Alessandro, Dragt, Alex, Drake, Gary, Drásal, Zbynek, Dreiner, Herbert, Drell, Persis, Driouichi, Chafik, Drozhdin, Alexandr, Drugakov, Vladimir, Du, Shuxian, Dugan, Gerald, Duginov, Viktor, Dulinski, Wojciech, Dulucq, Frederic, Dutta, Sukanta, Dwivedi, Jishnu, Dychkant, Alexandre, Dzahini, Daniel, Eckerlin, Guenter, Edwards, Helen, Ehrenfeld, Wolfgang, Ehrlichman, Michael, Ehrlichmann, Heiko, Eigen, Gerald, Elagin, Andrey, Elementi, Luciano, Eliasson, Peder, Ellis, John, Ellwood, George, Elsen, Eckhard, Emery, Louis, Enami, Kazuhiro, Endo, Kuninori, Enomoto, Atsushi, Eozénou, Fabien, Erbacher, Robin, Erickson, Roger, Oleg Eyser, K., Fadeyev, Vitaliy, Fang, Shou Xian, Fant, Karen, Fasso, Alberto, Faucci Giannelli, Michele, Fehlberg, John, Feld, Lutz, Feng, Jonathan L., Ferguson, John, Fernandez-Garcia, Marcos, Luis Fernandez-Hernando, J., Fiala, Pavel, Fieguth, Ted, Finch, Alexander, Finocchiaro, Giuseppe, Fischer, Peter, Fisher, Peter, Eugene Fisk, H., Fitton, Mike D., Fleck, Ivor, Fleischer, Manfred, Fleury, Julien, Flood, Kevin, Foley, Mike, Ford, Richard, Fortin, Dominique, Foster, Brian, Fourches, Nicolas, Francis, Kurt, Frey, Ariane, Frey, Raymond, Friedsam, Horst, Frisch, Josef, Frishman, Anatoli, Fuerst, Joel, Fujii, Keisuke, Fujimoto, Junpei, Fukuda, Masafumi, Fukuda, Shigeki, Funahashi, Yoshisato, Funk, Warren, Furletova, Julia, Furukawa, Kazuro, Furuta, Fumio, Fusayasu, Takahiro, Fuster, Juan, Gadow, Karsten, Gaede, Frank, Gaglione, Renaud, Gai, Wei, Gajewski, Jan, Galik, Richard, Galkin, Alexei, Galkin, Valery, Gallin-Martel, Laurent, Gannaway, Fred, Gao, Jian She, Gao, Jie, Gao, Yuanning, Garbincius, Peter, Garcia-Tabares, Luis, Garren, Lynn, Garrido, Luís, Garutti, Erika, Garvey, Terry, Garwin, Edward, Gascón, David, Gastal, Martin, Gatto, Corrado, Gatto, Raoul, Gay, Pascal, Ge, Lixin, Ge, Ming Qi, Ge, Rui, Geiser, Achim, Gellrich, Andreas, Genat, Jean-Francois, Geng, Zhe Qiao, Gentile, Simonetta, Gerbick, Scot, Gerig, Rod, Ghosh, Dilip Kumar, Ghosh, Kirtiman, Gibbons, Lawrence, Giganon, Arnaud, Gillespie, Allan, Gillman, Tony, Ginzburg, Ilya, Giomataris, Ioannis, Giunta, Michele, Gladkikh, Peter, Gluza, Janusz, Godbole, Rohini, Godfrey, Stephen, Goldhaber, Gerson, Goldstein, Joel, Gollin, George D., Gonzalez-Sanchez, Francisco Javier, Goodrick, Maurice, Gornushkin, Yuri, Gostkin, Mikhail, Gottschalk, Erik, Goudket, Philippe, Gough Eschrich, Ivo, Gournaris, Filimon, Graciani, Ricardo, Graf, Norman, Grah, Christian, Grancagnolo, Francesco, Grandjean, Damien, Grannis, Paul, Grassellino, Anna, Eugeni Graugés, Gray, Stephen, Green, Michael, Greenhalgh, Justin, Greenshaw, Timothy, Grefe, Christian, Gregor, Ingrid-Maria, Grenier, Gerald, Grimes, Mark, Grimm, Terry, Gris, Philippe, Grivaz, Jean-Francois, Groll, Marius, Gronberg, Jeffrey, Grondin, Denis, Groom, Donald, Gross, Eilam, Grunewald, Martin, Grupen, Claus, Grzelak, Grzegorz, Gu, Jun, Gu, Yun-Ting, Guchait, Monoranjan, Guiducci, Susanna, Guler, Ali Murat, Guler, Hayg, Gulmez, Erhan, Gunion, John, Guo, Zhi Yu, Gurtu, Atul, Ha, Huy Bang, Haas, Tobias, Haase, Andy, Haba, Naoyuki, Haber, Howard, Haensel, Stephan, Hagge, Lars, Hagura, Hiroyuki, Hajdu, Csaba, Haller, Gunther, Haller, Johannes, Hallermann, Lea, Halyo, Valerie, Hamaguchi, Koichi, Hammond, Larry, Han, Liang, Han, Tao, Hand, Louis, Handu, Virender K., Hano, Hitoshi, Hansen, Christian, Hansen, Jørn Dines, Hansen, Jorgen Beck, Hara, Kazufumi, Harder, Kristian, Hartin, Anthony, Hartung, Walter, Hast, Carsten, Hauptman, John, Hauschild, Michael, Hauviller, Claude, Havranek, Miroslav, Hawkes, Chris, Hawkings, Richard, Hayano, Hitoshi, Hazumi, Masashi, He, An, He, Hong Jian, Hearty, Christopher, Heath, Helen, Hebbeker, Thomas, Hedberg, Vincent, Hedin, David, Heifets, Samuel, Heinemeyer, Sven, Heini, Sebastien, Helebrant, Christian, Helms, Richard, Heltsley, Brian, Henrot-Versille, Sophie, Henschel, Hans, Hensel, Carsten, Hermel, Richard, Herms, Atilà, Herten, Gregor, Hesselbach, Stefan, Heuer, Rolf-Dieter, Heusch, Clemens A., Hewett, Joanne, Higashi, Norio, Higashi, Takatoshi, Higashi, Yasuo, Higo, Toshiyasu, Hildreth, Michael D., Hiller, Karlheinz, Hillert, Sonja, Hillier, Stephen James, Himel, Thomas, Himmi, Abdelkader, Hinchliffe, Ian, Hioki, Zenro, Hirano, Koichiro, Hirose, Tachishige, Hisamatsu, Hiromi, Hisano, Junji, Hlaing, Chit Thu, Hock, Kai Meng, Hoeferkamp, Martin, Hohlfeld, Mark, Honda, Yousuke, Hong, Juho, Hong, Tae Min, Honma, Hiroyuki, Horii, Yasuyuki, Horvath, Dezso, Hosoyama, Kenji, Hostachy, Jean-Yves, Hou, Mi, Hou, Wei-Shu, Howell, David, Hronek, Maxine, Hsiung, Yee B., Hu, Bo, Hu, Tao, Huang, Jung-Yun, Huang, Tong Ming, Huang, Wen Hui, Huedem, Emil, Huggard, Peter, Hugonie, Cyril, Hu-Guo, Christine, Huitu, Katri, Hwang, Youngseok, Idzik, Marek, Ignatenko, Alexandr, Ignatov, Fedor, Ikeda, Hirokazu, Ikematsu, Katsumasa, Ilicheva, Tatiana, Imbault, Didier, Imhof, Andreas, Incagli, Marco, Ingbir, Ronen, Inoue, Hitoshi, Inoue, Youichi, Introzzi, Gianluca, Ioakeimidi, Katerina, Ishihara, Satoshi, Ishikawa, Akimasa, Ishikawa, Tadashi, Issakov, Vladimir, Ito, Kazutoshi, Ivanov, V. V., Ivanov, Valentin, Ivanyushenkov, Yury, Iwasaki, Masako, Iwashita, Yoshihisa, Jackson, David, Jackson, Frank, Jacobsen, Bob, Jaganathan, Ramaswamy, Jamison, Steven, Janssen, Matthias Enno, Jaramillo-Echeverria, Richard, Jaros, John, Jauffret, Clement, Jawale, Suresh B., Jeans, Daniel, Jedziniak, Ron, Jeffery, Ben, Jehanno, Didier, Jenner, Leo J., Jensen, Chris, Jensen, David R., Jiang, Hairong, Jiang, Xiao Ming, Jimbo, Masato, Jin, Shan, Keith Jobe, R., Johnson, Anthony, Johnson, Erik, Johnson, Matt, Johnston, Michael, Joireman, Paul, Jokic, Stevan, Jones, James, Jones, Roger M., Jongewaard, Erik, Jönsson, Leif, Joshi, Gopal, Joshi, Satish C., Jung, Jin-Young, Junk, Thomas, Juste, Aurelio, Kado, Marumi, Kadyk, John, Käfer, Daniela, Kako, Eiji, Kalavase, Puneeth, Kalinin, Alexander, Kalinowski, Jan, Kamitani, Takuya, Kamiya, Yoshio, Kamiya, Yukihide, Kamoshita, Jun-Ichi, Kananov, Sergey, Kanaya, Kazuyuki, Kanazawa, Ken-Ichi, Kanemura, Shinya, Kang, Heung-Sik, Kang, Wen, Kanjial, D., Kapusta, Frédéric, Karataev, Pavel, Karchin, Paul E., Karlen, Dean, Karyotakis, Yannis, Kashikhin, Vladimir, Kashiwagi, Shigeru, Kasley, Paul, Katagiri, Hiroaki, Kato, Takashi, Kato, Yukihiro, Katzy, Judith, Kaukher, Alexander, Kaur, Manjit, Kawagoe, Kiyotomo, Kawamura, Hiroyuki, Kazakov, Sergei, Kekelidze, V. D., Keller, Lewis, Kelley, Michael, Kelly, Marc, Kelly, Michael, Kennedy, Kurt, Kephart, Robert, Keung, Justin, Khainovski, Oleg, Khan, Sameen Ahmed, Khare, Prashant, Khovansky, Nikolai, Kiesling, Christian, Kikuchi, Mitsuo, Kilian, Wolfgang, Killenberg, Martin, Kim, Donghee, Kim, Eun San, Kim, Eun-Joo, Kim, Guinyun, Kim, Hongjoo, Kim, Hyoungsuk, Kim, Hyun-Chui, Kim, Jonghoon, Kim, Kwang-Je, Kim, Kyung Sook, Kim, Peter, Kim, Seunghwan, Kim, Shin-Hong, Kim, Sun Kee, Kim, Tae Jeong, Kim, Youngim, Kim, Young-Kee, Kimmitt, Maurice, Kirby, Robert, Kircher, François, Kisielewska, Danuta, Kittel, Olaf, Klanner, Robert, Klebaner, Arkadiy L., Kleinwort, Claus, Klimkovich, Tatsiana, Klinkby, Esben, Kluth, Stefan, Knecht, Marc, Kneisel, Peter, Ko, In Soo, Ko, Kwok, Kobayashi, Makoto, Kobayashi, Nobuko, Kobel, Michael, Koch, Manuel, Kodys, Peter, Koetz, Uli, Kohrs, Robert, Kojima, Yuuji, Kolanoski, Hermann, Kolodziej, Karol, Kolomensky, Yury G., Komamiya, Sachio, Kong, Xiang Cheng, Konigsberg, Jacobo, Korbel, Volker, Koscielniak, Shane, Kostromin, Sergey, Kowalewski, Robert, Kraml, Sabine, Krammer, Manfred, Krasnykh, Anatoly, Krautscheid, Thorsten, Krawczyk, Maria, James Krebs, H., Krempetz, Kurt, Kribs, Graham, Krishnagopal, Srinivas, Kriske, Richard, Kronfeld, Andreas, Kroseberg, Jürgen, Kruchonak, Uladzimir, Kruecker, Dirk, Krüger, Hans, Krumpa, Nicholas A., Krumshtein, Zinovii, Kuang, Yu Ping, Kubo, Kiyoshi, Kuchler, Vic, Kudoh, Noboru, Kulis, Szymon, Kumada, Masayuki, Kumar, Abhay, Kume, Tatsuya, Kundu, Anirban, Kurevlev, German, Kurihara, Yoshimasa, Kuriki, Masao, Kuroda, Shigeru, Kuroiwa, Hirotoshi, Kurokawa, Shin-Ichi, Kusano, Tomonori, Kush, Pradeep K., Kutschke, Robert, Kuznetsova, Ekaterina, Kvasnicka, Peter, Kwon, Youngjoon, Labarga, Luis, Lacasta, Carlos, Lackey, Sharon, Lackowski, Thomas W., Lafaye, Remi, Lafferty, George, Lagorio, Eric, Laktineh, Imad, Lal, Shankar, Laloum, Maurice, Lam, Briant, Lancaster, Mark, Lander, Richard, Lange, Wolfgang, Langenfeld, Ulrich, Langeveld, Willem, Larbalestier, David, Larsen, Ray, Lastovicka, Tomas, Lastovicka-Medin, Gordana, Latina, Andrea, Latour, Emmanuel, Laurent, Lisa, Le, Ba Nam, Le, Duc Ninh, Le Diberder, Francois, Dû, Patrick Le, Lebbolo, Hervé, Lebrun, Paul, Lecoq, Jacques, Lee, Sung-Won, Lehner, Frank, Leibfritz, Jerry, Lenkszus, Frank, Lesiak, Tadeusz, Levy, Aharon, Lewandowski, Jim, Leyh, Greg, Li, Cheng, Li, Chong Sheng, Li, Chun Hua, Li, Da Zhang, Li, Gang, Li, Jin, Li, Shao Peng, Li, Wei Ming, Li, Weiguo, Li, Xiao Ping, Li, Xue-Qian, Li, Yuanjing, Li, Yulan, Li, Zenghai, Li, Zhong Quan, Liang, Jian Tao, Liao, Yi, Lilje, Lutz, Guilherme Lima, J., Lintern, Andrew J., Lipton, Ronald, List, Benno, List, Jenny, Liu, Chun, Liu, Jian Fei, Liu, Ke Xin, Liu, Li Qiang, Liu, Shao Zhen, Liu, Sheng Guang, Liu, Shubin, Liu, Wanming, Liu, Wei Bin, Liu, Ya Ping, Liu, Yu Dong, Lockyer, Nigel, Logan, Heather E., Logatchev, Pavel V., Lohmann, Wolfgang, Lohse, Thomas, Lola, Smaragda, Lopez-Virto, Amparo, Loveridge, Peter, Lozano, Manuel, Lu, Cai-Dian, Lu, Changguo, Lu, Gong-Lu, Lu, Wen Hui, Lubatti, Henry, Lucotte, Arnaud, Lundberg, Björn, Lundin, Tracy, Luo, Mingxing, Luong, Michel, Luth, Vera, Lutz, Benjamin, Lutz, Pierre, Lux, Thorsten, Luzniak, Pawel, Lyapin, Alexey, Lykken, Joseph, Lynch, Clare, Ma, Li, Ma, Lili, Ma, Qiang, Ma, Wen-Gan, Macfarlane, David, Maciel, Arthur, Macleod, Allan, Macnair, David, Mader, Wolfgang, Magill, Stephen, Magnan, Anne-Marie, Maiheu, Bino, Maity, Manas, Majchrzak, Millicent, Majumder, Gobinda, Makarov, Roman, Makowski, Dariusz, Malaescu, Bogdan, Mallik, C., Mallik, Usha, Malton, Stephen, Malyshev, Oleg B., Malysheva, Larisa I., Mammosser, John, Mamta, Mamuzic, Judita, Manen, Samuel, Manghisoni, Massimo, Manly, Steven, Marcellini, Fabio, Marcisovsky, Michal, Markiewicz, Thomas W., Marks, Steve, Marone, Andrew, Marti, Felix, Martin, Jean-Pierre, Martin, Victoria, Martin-Chassard, Gisèle, Martinez, Manel, Martinez-Rivero, Celso, Martsch, Dennis, Martyn, Hans-Ulrich, Maruyama, Takashi, Masuzawa, Mika, Mathez, Hervé, Matsuda, Takeshi, Matsumoto, Hiroshi, Matsumoto, Shuji, Matsumoto, Toshihiro, Matsunaga, Hiroyuki, Mättig, Peter, Mattison, Thomas, Mavromanolakis, Georgios, Mawatari, Kentarou, Mazzacane, Anna, Mcbride, Patricia, Mccormick, Douglas, Mccormick, Jeremy, Mcdonald, Kirk T., Mcgee, Mike, Mcintosh, Peter, Mckee, Bobby, Mcpherson, Robert A., Meidlinger, Mandi, Meier, Karlheinz, Mele, Barbara, Meller, Bob, Melzer-Pellmann, Isabell-Alissandra, Mendez, Hector, Mercer, Adam, Merkin, Mikhail, Meshkov, I. N., Messner, Robert, Metcalfe, Jessica, Meyer, Chris, Meyer, Hendrik, Meyer, Joachim, Meyer, Niels, Meyners, Norbert, Michelato, Paolo, Michizono, Shinichiro, Mihalcea, Daniel, Mihara, Satoshi, Mihara, Takanori, Mikami, Yoshinari, Mikhailichenko, Alexander A., Milardi, Catia, Miller, David J., Miller, Owen, Miller, Roger J., Milstene, Caroline, Mimashi, Toshihiro, Minashvili, Irakli, Miquel, Ramon, Mishra, Shekhar, Mitaroff, Winfried, Mitchell, Chad, Miura, Takako, Miyamoto, Akiya, Miyata, Hitoshi, Mjörnmark, Ulf, Mnich, Joachim, Moenig, Klaus, Moffeit, Kenneth, Mokhov, Nikolai, Molloy, Stephen, Monaco, Laura, Monasterio, Paul R., Montanari, Alessandro, Moon, Sung Ik, Moortgat-Pick, Gudrid A., Mora Freitas, Paulo, Morel, Federic, Moretti, Stefano, Morgunov, Vasily, Mori, Toshinori, Morin, Laurent, Morisseau, François, Morita, Yoshiyuki, Morita, Youhei, Morita, Yuichi, Morozov, Nikolai, Morozumi, Yuichi, Morse, William, Moser, Hans-Guenther, Moultaka, Gilbert, Mtingwa, Sekazi, Mudrinic, Mihajlo, Mueller, Alex, Mueller, Wolfgang, Muennich, Astrid, Muhlleitner, Milada Margarete, Mukherjee, Bhaskar, Mukhopadhyaya, Biswarup, Müller, Thomas, Munro, Morrison, Murayama, Hitoshi, Muto, Toshiya, Myneni, Ganapati Rao, Nabhiraj, P. Y., Nagaitsev, Sergei, Nagamine, Tadashi, Nagano, Ai, Naito, Takashi, Nakai, Hirotaka, Nakajima, Hiromitsu, Nakamura, Isamu, Nakamura, Tomoya, Nakanishi, Tsutomu, Nakao, Katsumi, Nakao, Noriaki, Nakayoshi, Kazuo, Nam, Sang, Namito, Yoshihito, Namkung, Won, Nantista, Chris, Napoly, Olivier, Narain, Meenakshi, Naroska, Beate, Nauenberg, Uriel, Nayyar, Ruchika, Neal, Homer, Nelson, Charles, Nelson, Janice, Nelson, Timothy, Nemecek, Stanislav, Neubauer, Michael, Neuffer, David, Newman, Myriam Q., Nezhevenko, Oleg, Ng, Cho-Kuen, Nguyen, Anh Ky, Nguyen, Minh, Nguyen Thi, Hong, Niebuhr, Carsten, Niehoff, Jim, Niezurawski, Piotr, Nishitani, Tomohiro, Nitoh, Osamu, Noguchi, Shuichi, Nomerotski, Andrei, Noonan, John, Norbeck, Edward, Nosochkov, Yuri, Notz, Dieter, Nowak, Grazyna, Nowak, Hannelies, Noy, Matthew, Nozaki, Mitsuaki, Nyffeler, Andreas, Nygren, David, Oddone, Piermaria, O, Joseph, Oh, Jong-Seok, Oh, Sun Kun, Ohkuma, Kazumasa, Ohlerich, Martin, Ohmi, Kazuhito, Ohnishi, Yukiyoshi, Ohsawa, Satoshi, Ohuchi, Norihito, Oide, Katsunobu, Okada, Nobuchika, Okada, Yasuhiro, Okamura, Takahiro, Okugi, Toshiyuki, Okumi, Shoji, Okumura, Ken-Ichi, Olchevski, Alexander, Oliver, William, Olivier, Bob, Olsen, James, Olsen, Jeff, Olsen, Stephen, Olshevsky, A. G., Olsson, Jan, Omori, Tsunehiko, Onel, Yasar, Onengut, Gulsen, Ono, Hiroaki, Onoprienko, Dmitry, Oreglia, Mark, Oren, Will, Orimoto, Toyoko J., Oriunno, Marco, Orlandea, Marius Ciprian, Oroku, Masahiro, Orr, Lynne H., Orr, Robert S., Oshea, Val, Oskarsson, Anders, Osland, Per, Ossetski, Dmitri, Österman, Lennart, Ostiguy, Francois, Otono, Hidetoshi, Ottewell, Brian, Ouyang, Qun, Padamsee, Hasan, Padilla, Cristobal, Pagani, Carlo, Palmer, Mark A., Pam, Wei Min, Pande, Manjiri, Pande, Rajni, Pandit, V. S., Pandita, P. N., Pandurovic, Mila, Pankov, Alexander, Panzeri, Nicola, Papandreou, Zisis, Paparella, Rocco, Para, Adam, Park, Hwanbae, Parker, Brett, Parkes, Chris, Parma, Vittorio, Parsa, Zohreh, Parsons, Justin, Partridge, Richard, Pasquinelli, Ralph, Pásztor, Gabriella, Paterson, Ewan, Patrick, Jim, Patteri, Piero, Ritchie Patterson, J., Pauletta, Giovanni, Paver, Nello, Pavlicek, Vince, Pawlik, Bogdan, Payet, Jacques, Pchalek, Norbert, Pedersen, John, Pei, Guo Xi, Pei, Shi Lun, Pelka, Jerzy, Pellegrini, Giulio, Pellett, David, Peng, G. X., Penn, Gregory, Penzo, Aldo, Perry, Colin, Peskin, Michael, Peters, Franz, Petersen, Troels Christian, Peterson, Daniel, Peterson, Thomas, Petterson, Maureen, Pfeffer, Howard, Pfund, Phil, Phelps, Alan, Phi, Quang, Phillips, Jonathan, Piccolo, Marcello, Piemontese, Livio, Pierini, Paolo, Thomas Piggott, W., Pike, Gary, Pillet, Nicolas, Jayawardena, Talini Pinto, Piot, Phillippe, Pitts, Kevin, Pivi, Mauro, Plate, Dave, Pleier, Marc-Andre, Poblaguev, Andrei, Poehler, Michael, Poelker, Matthew, Poffenberger, Paul, Pogorelsky, Igor, Poirier, Freddy, Poling, Ronald, Poole, Mike, Popescu, Sorina, Popielarski, John, Pöschl, Roman, Postranecky, Martin, Potukochi, Prakash N., Prast, Julie, Prat, Serge, Preger, Miro, Prepost, Richard, Price, Michael, Proch, Dieter, Puntambekar, Avinash, Qin, Qing, Qu, Hua Min, Quadt, Arnulf, Quesnel, Jean-Pierre, Radeka, Veljko, Rahmat, Rahmat, Rai, Santosh Kumar, Raimondi, Pantaleo, Ramberg, Erik, Ranjan, Kirti, Rao, Sista V. L. S., Raspereza, Alexei, Ratti, Alessandro, Ratti, Lodovico, Raubenheimer, Tor, Raux, Ludovic, Ravindran, V., Raychaudhuri, Sreerup, Re, Valerio, Rease, Bill, Reece, Charles E., Regler, Meinhard, Rehlich, Kay, Reichel, Ina, Reichold, Armin, Reid, John, Reid, Ron, Reidy, James, Reinhard, Marcel, Renz, Uwe, Repond, Jose, Resta-Lopez, Javier, Reuen, Lars, Ribnik, Jacob, Rice, Tyler, Richard, François, Riemann, Sabine, Riemann, Tord, Riles, Keith, Riley, Daniel, Rimbault, Cécile, Rindani, Saurabh, Rinolfi, Louis, Risigo, Fabio, Riu, Imma, Rizhikov, Dmitri, Rizzo, Thomas, Rochford, James H., Rodriguez, Ponciano, Roeben, Martin, Rolandi, Gigi, Roodman, Aaron, Rosenberg, Eli, Roser, Robert, Ross, Marc, Rossel, François, Rossmanith, Robert, Roth, Stefan, Rougé, André, Rowe, Allan, Roy, Amit, Roy, Sendhunil B., Roy, Sourov, Royer, Laurent, Royole-Degieux, Perrine, Royon, Christophe, Ruan, Manqi, Rubin, David, Ruehl, Ingo, Jimeno, Alberto Ruiz, Ruland, Robert, Rusnak, Brian, Ryu, Sun-Young, Sabbi, Gian Luca, Sadeh, Iftach, Sadygov, Ziraddin Y., Saeki, Takayuki, Sagan, David, Sahni, Vinod C., Saini, Arun, Saito, Kenji, Saito, Kiwamu, Sajot, Gerard, Sakanaka, Shogo, Sakaue, Kazuyuki, Salata, Zen, Salih, Sabah, Salvatore, Fabrizio, Samson, Joergen, Sanami, Toshiya, Levi Sanchez, Allister, Sands, William, Santic, John, Sanuki, Tomoyuki, Sapronov, Andrey, Sarkar, Utpal, Sasao, Noboru, Satoh, Kotaro, Sauli, Fabio, Saunders, Claude, Saveliev, Valeri, Savoy-Navarro, Aurore, Sawyer, Lee, Saxton, Laura, Schäfer, Oliver, Schälicke, Andreas, Schade, Peter, Schaetzel, Sebastien, Scheitrum, Glenn, Schibler, Emilie, Schindler, Rafe, Schlösser, Markus, Schlueter, Ross D., Schmid, Peter, Schmidt, Ringo Sebastian, Schneekloth, Uwe, Schreiber, Heinz Juergen, Schreiber, Siegfried, Schroeder, Henning, Peter Schüler, K., Schulte, Daniel, Schultz-Coulon, Hans-Christian, Schumacher, Markus, Schumann, Steffen, Schumm, Bruce A., Schwienhorst, Reinhard, Schwierz, Rainer, Scott, Duncan J., Scuri, Fabrizio, Sefkow, Felix, Sefri, Rachid, Seguin-Moreau, Nathalie, Seidel, Sally, Seidman, David, Sekmen, Sezen, Seletskiy, Sergei, Senaha, Eibun, Senanayake, Rohan, Sendai, Hiroshi, Sertore, Daniele, Seryi, Andrei, Settles, Ronald, Sever, Ramazan, Shales, Nicholas, Shao, Ming, Shelkov, G. A., Shepard, Ken, Shepherd-Themistocleous, Claire, Sheppard, John C., Shi, Cai Tu, Shidara, Tetsuo, Shim, Yeo-Jeong, Shimizu, Hirotaka, Shimizu, Yasuhiro, Shimizu, Yuuki, Shimogawa, Tetsushi, Shin, Seunghwan, Shioden, Masaomi, Shipsey, Ian, Shirkov, Grigori, Shishido, Toshio, Shivpuri, Ram K., Shrivastava, Purushottam, Shulga, Sergey, Shumeiko, Nikolai, Shuvalov, Sergey, Si, Zongguo, Siddiqui, Azher Majid, Siegrist, James, Simon, Claire, Simrock, Stefan, Sinev, Nikolai, Singh, Bhartendu K., Singh, Jasbir, Singh, Pitamber, Singh, R. K., Singh, S. K., Singini, Monito, Sinha, Anil K., Sinha, Nita, Sinha, Rahul, Sinram, Klaus, Sissakian, A. N., Skachkov, N. B., Skrinsky, Alexander, Slater, Mark, Slominski, Wojciech, Smiljanic, Ivan, Smith, A. J. Stewart, Smith, Alex, Smith, Brian J., Smith, Jeff, Smith, Jonathan, Smith, Steve, Smith, Susan, Smith, Tonee, Neville Snodgrass, W., Sobloher, Blanka, Sohn, Young-Uk, Solidum, Ruelson, Solyak, Nikolai, Son, Dongchul, Sonmez, Nasuf, Sopczak, Andre, Soskov, V., Spencer, Cherrill M., Spentzouris, Panagiotis, Speziali, Valeria, Spira, Michael, Sprehn, Daryl, Sridhar, K., Srivastava, Asutosh, St Lorant, Steve, Stahl, Achim, Stanek, Richard P., Stanitzki, Marcel, Stanley, Jacob, Stefanov, Konstantin, Stein, Werner, Steiner, Herbert, Stenlund, Evert, Stern, Amir, Sternberg, Matt, Stockinger, Dominik, Stockton, Mark, Stoeck, Holger, Strachan, John, Strakhovenko, V., Strauss, Michael, Striganov, Sergei I., Strologas, John, Strom, David, Strube, Jan, Stupakov, Gennady, Su, Dong, Sudo, Yuji, Suehara, Taikan, Suehiro, Toru, Suetsugu, Yusuke, Sugahara, Ryuhei, Sugimoto, Yasuhiro, Sugiyama, Akira, Suh, Jun Suhk, Sukovic, Goran, Sun, Hong, Sun, Stephen, Sun, Werner, Sun, Yi, Sun, Yipeng, Suszycki, Leszek, Sutcliffe, Peter, Suthar, Rameshwar L., Suwada, Tsuyoshi, Suzuki, Atsuto, Suzuki, Chihiro, Suzuki, Shiro, Suzuki, Takashi, Swent, Richard, Swientek, Krzysztof, Swinson, Christina, Syresin, Evgeny, Szleper, Michal, Tadday, Alexander, Takahashi, Rika, Takahashi, Tohru, Takano, Mikio, Takasaki, Fumihiko, Takeda, Seishi, Takenaka, Tateru, Takeshita, Tohru, Takubo, Yosuke, Tanaka, Masami, Tang, Chuan Xiang, Taniguchi, Takashi, Tantawi, Sami, Tapprogge, Stefan, Tartaglia, Michael A., Tassielli, Giovanni Francesco, Tauchi, Toshiaki, Tavian, Laurent, Tawara, Hiroko, Taylor, Geoffrey, Telnov, Alexandre V., Telnov, Valery, Tenenbaum, Peter, Teodorescu, Eliza, Terashima, Akio, Terracciano, Giuseppina, Terunuma, Nobuhiro, Teubner, Thomas, Teuscher, Richard, Theilacker, Jay, Thomson, Mark, Tice, Jeff, Tigner, Maury, Timmermans, Jan, Titov, Maxim, Tokareva, N. A., Tollefson, Kirsten, Tomasek, Lukas, Tomovic, Savo, Tompkins, John, Tonutti, Manfred, Topkar, Anita, Toprek, Dragan, Toral, Fernando, Torrence, Eric, Traversi, Gianluca, Trimpl, Marcel, Mani Tripathi, S., Trischuk, William, Trodden, Mark, Trubnikov, G. V., Tschirhart, Robert, Tskhadadze, Edisher, Tsuchiya, Kiyosumi, Tsukamoto, Toshifumi, Tsunemi, Akira, Tucker, Robin, Turchetta, Renato, Tyndel, Mike, Uekusa, Nobuhiro, Ueno, Kenji, Umemori, Kensei, Ummenhofer, Martin, Underwood, David, Uozumi, Satoru, Urakawa, Junji, Urban, Jeremy, Uriot, Didier, Urner, David, Ushakov, Andrei, Usher, Tracy, Uzunyan, Sergey, Vachon, Brigitte, Valerio, Linda, Valin, Isabelle, Valishev, Alex, Vamra, Raghava, Graaf, Harry, Kooten, Rick, Zandbergen, Gary, Vanel, Jean-Charles, Variola, Alessandro, Varner, Gary, Velasco, Mayda, Velte, Ulrich, Velthuis, Jaap, Vempati, Sundir K., Venturini, Marco, Vescovi, Christophe, Videau, Henri, Vila, Ivan, Vincent, Pascal, Virey, Jean-Marc, Visentin, Bernard, Viti, Michele, Vo, Thanh Cuong, Vogel, Adrian, Vogt, Harald, Toerne, Eckhard, Vorozhtsov, S. B., Vos, Marcel, Votava, Margaret, Vrba, Vaclav, Wackeroth, Doreen, Wagner, Albrecht, Wagner, Carlos E. M., Wagner, Stephen, Wake, Masayoshi, Walczak, Roman, Walkowiak, Wolfgang, Wallon, Samuel, Walsh, Roberval, Walston, Sean, Waltenberger, Wolfgang, Walz, Dieter, Wang, Chao En, Wang, Chun Hong, Wang, Dou, Wang, Faya, Wang, Guang Wei, Wang, Haitao, Wang, Jiang, Wang, Jiu Qing, Wang, Juwen, Wang, Lanfa, Wang, Lei, Wang, Min-Zu, Wang, Qing, Wang, Shu Hong, Wang, Xiaolian, Wang, Xue-Lei, Wang, Yi Fang, Wang, Zheng, Wanzenberg, Rainer, Ward, Bennie, Ward, David, Warmbein, Barbara, Warner, David W., Warren, Matthew, Washio, Masakazu, Watanabe, Isamu, Watanabe, Ken, Watanabe, Takashi, Watanabe, Yuichi, Watson, Nigel, Wattimena, Nanda, Wayne, Mitchell, Weber, Marc, Weerts, Harry, Weiglein, Georg, Weiland, Thomas, Weinzierl, Stefan, Weise, Hans, Weisend, John, Wendt, Manfred, Wendt, Oliver, Wenzel, Hans, Wenzel, William A., Wermes, Norbert, Werthenbach, Ulrich, Wesseln, Steve, Wester, William, White, Andy, White, Glen R., Wichmann, Katarzyna, Wienemann, Peter, Wierba, Wojciech, Wilksen, Tim, Willis, William, Wilson, Graham W., Wilson, John A., Wilson, Robert, Wing, Matthew, Winter, Marc, Wirth, Brian D., Wolbers, Stephen A., Wolff, Dan, Wolski, Andrzej, Woodley, Mark D., Woods, Michael, Woodward, Michael L., Woolliscroft, Timothy, Worm, Steven, Wormser, Guy, Wright, Dennis, Wright, Douglas, Wu, Andy, Wu, Tao, Wu, Yue Liang, Xella, Stefania, Xia, Guoxing, Xia, Lei, Xiao, Aimin, Xiao, Liling, Xie, Jia Lin, Xing, Zhi-Zhong, Xiong, Lian You, Xu, Gang, Xu, Qing Jing, Yajnik, Urjit A., Yakimenko, Vitaly, Yamada, Ryuji, Yamaguchi, Hiroshi, Yamamoto, Akira, Yamamoto, Hitoshi, Yamamoto, Masahiro, Yamamoto, Naoto, Yamamoto, Richard, Yamamoto, Yasuchika, Yamanaka, Takashi, Yamaoka, Hiroshi, Yamashita, Satoru, Yamazaki, Hideki, Yan, Wenbiao, Yang, Hai-Jun, Yang, Jin Min, Yang, Jongmann, Yang, Zhenwei, Yano, Yoshiharu, Yazgan, Efe, Yeh, G. P., Yilmaz, Hakan, Yock, Philip, Yoda, Hakutaro, Yoh, John, Yokoya, Kaoru, Yokoyama, Hirokazu, York, Richard C., Yoshida, Mitsuhiro, Yoshida, Takuo, Yoshioka, Tamaki, Young, Andrew, Yu, Cheng Hui, Yu, Jaehoon, Yu, Xian Ming, Yuan, Changzheng, Yue, Chong-Xing, Yue, Jun Hui, Zacek, Josef, Zagorodnov, Igor, Zalesak, Jaroslav, Zalikhanov, Boris, Zarnecki, Aleksander Filip, Zawiejski, Leszek, Zeitnitz, Christian, Zeller, Michael, Zerwas, Dirk, Zerwas, Peter, Zeyrek, Mehmet, Zhai, Ji Yuan, Zhang, Bao Cheng, Zhang, Bin, Zhang, Chuang, Zhang, He, Zhang, Jiawen, Zhang, Jing, Zhang, Jing Ru, Zhang, Jinlong, Zhang, Liang, Zhang, X., Zhang, Yuan, Zhang, Zhige, Zhang, Zhiqing, Zhang, Ziping, Zhao, Haiwen, Zhao, Ji Jiu, Zhao, Jing Xia, Zhao, Ming Hua, Zhao, Sheng Chu, Zhao, Tianchi, Zhao, Tong Xian, Zhao, Zhen Tang, Zhao, Zhengguo, Zhou, Min, Zhou, Feng, Zhou, Shun, Zhu, Shou Hua, Zhu, Xiong Wei, Zhukov, Valery, Zimmermann, Frank, Ziolkowski, Michael, Zisman, Michael S., Zomer, Fabian, Zong, Zhang Guo, Zorba, Osman, and Zutshi, Vishnu more...
- Subjects
Physics::Accelerator Physics ,Accelerators and Storage Rings - Abstract
The International Linear Collider (ILC) is a 200-500 GeV center-of-mass high-luminosity linear electron-positron collider, based on 1.3 GHz superconducting radio-frequency (SCRF) accelerating cavities. The ILC has a total footprint of about 31 km and is designed for a peak luminosity of 2x10^34 cm^-2 s^-1. The complex includes a polarized electron source, an undulator-based positron source, two 6.7 km circumference damping rings, two-stage bunch compressors, two 11 km long main linacs and a 4.5 km long beam delivery system. This report is Volume III (Accelerator) of the four volume Reference Design Report, which describes the design and cost of the ILC. The International Linear Collider (ILC) is a 200-500 GeV center-of-mass high-luminosity linear electron-positron collider, based on 1.3 GHz superconducting radio-frequency (SCRF) accelerating cavities. The ILC has a total footprint of about 31 km and is designed for a peak luminosity of 2x10^34 cm^-2 s^-1. The complex includes a polarized electron source, an undulator-based positron source, two 6.7 km circumference damping rings, two-stage bunch compressors, two 11 km long main linacs and a 4.5 km long beam delivery system. This report is Volume III (Accelerator) of the four volume Reference Design Report, which describes the design and cost of the ILC. more...
233. The International Linear Collider: Report to Snowmass 2021
- Author
-
Aryshev, Alexander, Behnke, Ties, Berggren, Mikael, Brau, James, Craig, Nathaniel, Freitas, Ayres, Gaede, Frank, Gessner, Spencer, Gori, Stefania, Grojean, Christophe, Heinemeyer, Sven, Jeans, Daniel, Kruger, Katja, List, Benno, List, Jenny, Liu, Zhen, Michizono, Shinichiro, Miller, David W., Moult, Ian, Murayama, Hitoshi, Nakada, Tatsuya, Nanni, Emilio, Nojiri, Mihoko, Padamsee, Hasan, Perelstein, Maxim, Peskin, Michael E., Poeschl, Roman, Posen, Sam, Robson, Aidan, Strube, Jan, Suehara, Taikan, Tian, Junping, Titov, Maxim, Vos, Marcel, White, Andrew, Wilson, Graham, Yokoya, Kaoru, Zarnecki, Aleksander Filip, Adachi, Ichiro, Agashe, Kaustubh, Jovin, Tatjana Agatonovic, Aihara, Hiroaki, Altmannshofer, Wolfgang, Alves, Daniele, Anguiano, Justin, Aoki, Ken-Ichi, Aoki, Masato, Aoki, Toshihiro, Aoki, Yumi, Arai, Yasuo, Araki, Hayato, Asada, Haruka, Asai, Kento, Asai, Shoji, Attie, David, Baer, Howard, Bagger, Jonathan, Bai, Yang, Bailey, Ian, Barrue, Ricardo, Bartoldus, Rainer, Barzi, Emanuela, Basso, Matthew, Bauerdick, Lothar, Baum, Sebastian, Bellerive, Alain, Belomestnykh, Sergey, Antequera, Jorge Berenguer, Beyer, Jakob, Bhat, Pushpalatha, Bilki, Burak, Black, Kevin, Bloom, Kenneth, Bodwin, Geoffrey, Boisvert, Veronique, Boran, Fatma, Boudry, Vincent, Boughezal, Radja, Boveia, Antonio, Bozovic-Jelisavcic, Ivanka, Brient, Jean-Claude, Brodsky, Stanley, Brunetti, Laurent, Buesser, Karsten, Bulyak, Eugene, Burrows, Philip N., Burt, Graeme C., Cai, Yunhai, Cairo, Valentina, Canepa, Anadi, Celiberto, Francesco Giovanni, Cenni, Enrico, Chacko, Zackaria, Chaikovska, Iryna, Checchin, Mattia, Chen, Lisong, Chen, Thomas Y., Cheng, Hsin Chia, Cho, Gi-Chol, Choudhary, Brajesh, Clarke, Jim, Cline, James, Co, Raymond, Cohen, Timothy, Colas, Paul, Damerell, Chris, Das, Arindam, Dasu, Sridhara, Dawson, Sally, de Blas, Jorge, de Lima, Carlos Henrique, Deandrea, Aldo, Dehmelt, Klaus, Delayen, Jean, Demarteau, Marcel, Denisov, Dmitri, Dermisek, Radovan, Dieguez, Angel, Dohmae, Takeshi, Dopke, Jens, Dort, Katharina, Du, Yong, Dudar, Bohdan, Dutta, Bhaskar, Dutta, Juhi, Einhaus, Ulrich, Elsen, Eckhard, Endo, Motoi, Eremeev, Grigory, Eren, Engin, Erler, Jens, Esarey, Eric, Everett, Lisa, Golfe, Angeles Faus, Garcia, Marcos Fernandez, Foster, Brian, Fourches, Nicolas, Fouz, Mary-Cruz, Fujii, Keisuke, Fujimoto, Junpei, Torregrosa, Esteban Fullan, Furukawa, Kazuro, Fusayasu, Takahiro, Fuster, Juan, Ganjour, Serguei, Gao, Yuanning, Gaur, Naveen, Geng, Rongli, Georgi, Howard, Gherghetta, Tony, Goldstein, Joel, Goncalves, Dorival, Gonski, Julia, Gonzalo, Tomas, Goto, Takeyoshi, Goto, Toru, Graf, Norman, Grames, Joseph, Grannis, Paul, Gray, Lindsey, Grohsjean, Alexander, Gu, Jiayin, Guler, Yalcin, Gutierrez, Phillip, Haba, Junji, Haber, Howard, Hallford, John, Hamaguchi, Koichi, Han, Tao, Hara, Kazuhiko, Harada, Daisuke, Hashimoto, Koji, Hashino, Katsuya, Hayashi, Masahito, Heinrich, Gudrun, Hidaka, Keisho, Higuchi, Takeo, Hinode, Fujio, Hioki, Zenro, Hirose, Minoru, Hiroshima, Nagisa, Hisano, Junji, Hollik, Wolfgang, Homiller, Samuel, Hong, Sungwoo, Hook, Anson, Horii, Yasuyuki, Hoshina, Hiroki, Hristova, Ivana, Huitu, Katri, Hyakutake, Yoshifumi, Iijima, Toru, Ikematsu, Katsumasa, Ilderton, Anton, Inami, Kenji, Irles, Adrian, Ishikawa, Akimasa, Ishiwata, Koji, Ito, Hayato, Ivanov, Igor, Iwamoto, Sho, Iwamoto, Toshiyuki, Iwasaki, Masako, Iwashita, Yoshihisa, Jia, Haoyi, Morales, Fabricio Jimenez, Joshi, Prakash, Jung, Sunghoon, Kacarevic, Goran, Kagan, Michael, Kakizaki, Mitsuru, Kalinowski, Jan, Kaminski, Jochen, Kanaya, Kazuyuki, Kanemura, Shinya, Kanno, Hayato, Kano, Yuya, Kashiwagi, Shigeru, Kato, Yukihiro, Kawada, Nanami, Kawada, Shin-ichi, Kawagoe, Kiyotomo, Khoze, Valery, Kichimi, Hiromichi, Kim, Doojin, Kitahara, Teppei, Kitano, Ryuichiro, Klamka, Jan, Komamiya, Sachio, Kong, K. C., Konomi, Taro, Kotera, Katsushige, Kou, Emi, Kravchenko, Ilya, Kubo, Kiyoshi, Kubo, Takayuki, Kumaoka, Takuya, Kumar, Ashish, Kumar, Nilanjana, Kunath, Jonas, Kundu, Saumyen, Kunitomo, Hiroshi, Kurata, Masakazu, Kuriki, Masao, Kusenko, Alexander, Lagouri, Theodota, Lankford, Andrew J., Lastovicka-Medin, Gordana, Diberder, Francois Le, Lee, Claire, Liepe, Matthias, Linacre, Jacob, Liptak, Zachary, Lomte, Shivani, Low, Ian, Ma, Yang, Maalouf, Hani, MacFarlane, David, Madison, Brendon, Madlener, Thomas, Maeda, Tomohito, Malek, Paul, Mandal, Sanjoy, Markiewicz, Thomas, Marshall, John, Martens, Aurelien, Martin, Victoria, Martinello, Martina, Rivero, Celso Martinez, Maru, Nobuhito, Matheson, John, Matsumoto, Shigeki, Matsunaga, Hiroyuki, Matsuo, Yutaka, Mawatari, Kentarou, Mbagwu, Johnpaul, McIntosh, Peter, McKeown, Peter, Meade, Patrick, Mekala, Krzysztof, Merkel, Petra, Mihara, Satoshi, Miralles, Víctor, Lopez, Marcos Miralles, Mishima, Go, Mishima, Satoshi, Mistlberger, Bernhard, Mitov, Alexander, Miyabayashi, Kenkichi, Miyamoto, Akiya, Mohanty, Gagan, Monaco, Laura, Mondragon, Myriam, Montgomery, Hugh E., Moortgat-Pick, Gudrid, Morange, Nicolas, Llacer, María Moreno, Moretti, Stefano, Mori, Toshinori, Morii, Toshiyuki, Moroi, Takeo, Morrissey, David, Nachman, Benjamin, Nagano, Kunihiro, Nakajima, Jurina, Nakamura, Eiji, Narita, Shinya, Nath, Pran, Nelson, Timothy, Newbold, David, Niki, Atsuya, Nishimura, Yasuhiro, Nishiyama, Eisaku, Nomura, Yasunori, Nowak, Kacper, Nozaki, Mitsuaki, de Vera, María Teresa Nunez Pardo, Ochoa, Ines, Ogata, Masahito, Ohashi, Satoru, Ohta, Hikaru, Ohta, Shigemi, Ohuchi, Norihito, Oide, Hideyuki, Okada, Nobuchika, Okada, Yasuhiro, Okawa, Shohei, Okayasu, Yuichi, Okugawa, Yuichi, Okugi, Toshiyuki, Okui, Takemichi, Okuyama, Yoshitaka, Omet, Mathieu, Omori, Tsunehiko, Ono, Hiroaki, Onoe, Tomoki, Ootani, Wataru, Otono, Hidetoshi, Ozawa, Shuhei, Griso, Simone Pagan, Papa, Alessandro, Paparella, Rocco, Park, Eun-Kyung, Perez, Gilad, Perez-Lorenzana, Abdel, Peters, Yvonne, Petriello, Frank, Piedra, Jonatan, Porod, Werner, Potter, Christopher, Price, Alan, Radkhorrami, Yasser, Reina, Laura, Reuter, Juergen, Richard, Francois, Riemann, Sabine, Rimmer, Robert, Rizzo, Thomas, Robens, Tania, Ruber, Roger, Jimeno, Alberto Ruiz, Saeki, Takayuki, Saha, Ipsita, Saito, Tomoyuki, Sakaguchi, Makoto, Sakai, Tadakatsu, Sakaki, Yasuhito, Sakurai, Kodai, Salvatico, Riccardo, Salvatore, Fabrizio, San, Yik Chuen, Sandick, Pearl, Sanuki, Tomoyuki, Sasikumar, Kollassery Swathi, Schaefer, Oliver, Schaefer, Ruth, Schneekloth, Uwe, Schoerner-Sadenius, Thomas, Schroeder, Carl, Schuster, Philip, Schwartzman, Ariel, Schwienhorst, Reinhard, Sefkow, Felix, Seiya, Yoshihiro, Sekiguchi, Motoo, Sekizawa, Kazuyuki, Senyo, Katsumi, Sert, Hale, Sertore, Danielev, Settles, Ronald, Shafi, Qaisar, Shahdara, Tetsuo, Haghi, Barmak Shams Es, Sharma, Ashish, Shelton, Jessie, Shepherd-Themistocleous, Claire, Shibuya, Hiroto, Shidara, Tetsuo, Shimomura, Takashi, Shindou, Tetsuo, Shoji, Yutaro, Shu, Jing, Sievers, Ian, Simon, Frank, Singh, Rajeev, Soreq, Yotam, Stanitzki, Marcel, Stapnes, Steinar, Steinhebel, Amanda, Stupak, John, Su, Shufang, Suekane, Fumihiko, Sugamoto, Akio, Sugawara, Yuji, Sugimoto, Satoru, Sugimoto, Yasuhiro, Sugiyama, Hiroaki, Sumino, Yukinari, Sundrum, Raman, Suzuki, Atsuto, Suzuki, Shin, Swiatlowski, Maximilian, Tait, Tim M. P., Takahashi, Shota, Takahashi, Tohru, Takeshita, Tohru, Takeuchi, Michihisa, Takubo, Yosuke, Tanabe, Tomohiko, Tanedo, Philip, Tanimoto, Morimitsu, Tao, Shuichiro, Tata, Xerxes, Tauchi, Toshiaki, Taylor, Geoffrey, Terada, Takahiro, Terunuma, Nobuhiro, Thaler, Jesse, Thea, Alessandro, Tillinger, Finn, Timmermans, Jan, Tobioka, Kohsaku, Toda, Kouichi, Tokiyasu, Atsushi, Toma, Takashi, Torndal, Julie, Tosun, Mehmet, Tsai, Yu-Dai, Tseng, Shih-Yen, Tsumura, Koji, Tuckler, Douglas, Uchida, Yoshiki, Uchiyama, Yusuke, Ueda, Daiki, Ukegawa, Fumihiko, Umemori, Kensei, Urakawa, Junji, Vallee, Claude, Vega, Roberto, Velasco, Liliana, Verdu-Andres, Silvia, Vernieri, Caterina, Vila, Anna, Alvarez, Ivan Vila, Vossebeld, Joost, Vsrms, Raghava, Vukasinovic, Natasa, Wackeroth, Doreen, Wakida, Moe, Wang, Liantao, Washio, Masakazu, Watanabe, Takashi, Watson, Nigel, Watts, Gordon, Weiglein, Georg, Wells, James D., Wenskat, Marc, Westhoff, Susanne, White, Glen, Williams, Ciaran, Willocq, Stephane, Wing, Matthew, Winter, Alasdair, Winter, Marc, Wu, Yongcheng, Xie, Keping, Xu, Tao, Yakovlev, Vyacheslav, Yamada, Shuei, Yamamoto, Akira, Yamamoto, Hitoshi, Yamamoto, Kei, Yamamoto, Yasuchika, Yamanaka, Masato, Yamashita, Satoru, Yamatani, Masahiro, Yamatsu, Naoki, Yasui, Shigehiro, Yoda, Takuya, Yonamine, Ryo, Yoshihara, Keisuke, Yoshioka, Masakazu, Yoshioka, Tamaki, Yuasa, Fukuko, Yumino, Keita, Zerwas, Dirk, Zheng, Ya-Juan, Zhou, Jia, Zhu, Hua Xing, Zobov, Mikhail, Zomer, Fabian, HEP, INSPIRE, Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), École polytechnique (X), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and ILC International Development Team more...
- Subjects
Accelerator Physics (physics.acc-ph) ,[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex] ,hep-ex ,[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph] ,FOS: Physical sciences ,[PHYS.PHYS.PHYS-ACC-PH] Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph] ,hep-ph ,ILC Coll ,Accelerators and Storage Rings ,High Energy Physics - Experiment ,[PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph] ,High Energy Physics - Phenomenology ,High Energy Physics - Experiment (hep-ex) ,High Energy Physics - Phenomenology (hep-ph) ,[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] ,accelerator, technology ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,Physics - Accelerator Physics ,accelerator: technology ,activity report ,accelerator: design ,Particle Physics - Experiment ,Particle Physics - Phenomenology ,physics.acc-ph - Abstract
The International Linear Collider (ILC) is on the table now as a new global energy-frontier accelerator laboratory taking data in the 2030s. The ILC addresses key questions for our current understanding of particle physics. It is based on a proven accelerator technology. Its experiments will challenge the Standard Model of particle physics and will provide a new window to look beyond it. This document brings the story of the ILC up to date, emphasizing its strong physics motivation, its readiness for construction, and the opportunity it presents to the US and the global particle physics community., Comment: 356 pages, Large pdf file (40 MB) submitted to Snowmass 2021; v2 references to Snowmass contributions added, additional authors; v3 references added, some updates, additional authors more...
- Full Text
- View/download PDF
234. Feasibility of pre-bunched FEL based on Coherent Diffraction Radiation
- Author
-
Sukhikh, L. G., Naumenko, G. A., Alexander Potylitsyn, Urakawa, J., Aryshev, A. S., Boogert, S., and Karataev, P. V.
235. Focusing of optical transition and diffraction radiation by a spherical target
- Author
-
Sukhikh, L. G., Naumenko, G. A., Alexander Potylitsyn, Urakawa, J., Aryshev, A. S., Boogert, S., and Karataev, P. V.
236. Pulsed green laser wire system for effective inverse compton scattering
- Author
-
Rawankar, A., Akagi, T., Aryshev, A., Yosuke Honda, Terunuma, N., Urakawa, J., Jehanno, D., and Sakaue, K.
237. Evaluation of Beam Halo from Beam-Gas Scattering at the KEK Accelerator Test Facility
- Author
-
Yang, R., Naito, T., Bai, S., Aryshev, A., Kubo, K., Okugi, T., Terunuma, N., Zhou, D., Faus-Golfe, A., Kubytskyi, V., Liu, Shan, Wallon, S., and Bambade, P.
- Subjects
7. Clean energy ,3. Good health - Abstract
Physical review accelerators and beams 21(5), 051001 (2018). doi:10.1103/PhysRevAccelBeams.21.051001, In circular colliders, as well as in damping rings and synchrotron radiation light sources, beam halo is one of the critical issues limiting the performance as well as potentially causing component damage and activation. It is imperative to clearly understand the mechanisms that lead to halo formation and to test the available theoretical models. Elastic beam-gas scattering can drive particles to large oscillation amplitudes and be a potential source of beam halo. In this paper, numerical estimation and Monte Carlo simulations of this process at the ATF of KEK are presented. Experimental measurements of beam halo in the ATF2 beam line using a diamond sensor detector are also described, which clearly demonstrate the influence of the beam-gas scattering process on the transverse halo distribution., Published by American Physical Society, College Park, MD more...
238. Sub-micrometre resolution laserwire transverse beam size measurement system
- Author
-
Nevay, L. J., Boogert, S. T., Karataev, P., Konstantin Kruchinin, Corner, L., Walczak, R., Aryshev, A., Urakawa, J., and Terunuma, N.
- Abstract
The laserwire system at the Accelerator Test Facility 2 (ATF2) is a transverse beam profile measurement system capable of measuring a micrometre-size electron beam. We present recent results demonstrating a measured vertical size of 1.16 ± 0.06 μm and a horizontal size of 110.1 ± 3.8 μ m. Due to the high aspect ratio of the electron beam, the natural divergence of the tightly focussed laser beam across the electron beam width requires the use of the full overlap integral to deconvolve the scans. For this to be done accurately, the propagation of the 150 mJ, 167 ps long laser pulses was precisely measured at a scaled virtual interaction point. more...
239. Novel approach to the elimination of background radiation in a single-shot longitudinal beam profile monitor
- Author
-
Harrison, Hannah, Aryshev, Alexander, Doucas, George, Konoplev, Ivan, Lancaster, Andrew, Shevelev, Mikhail, Terunuma, Nobuhiro, Urakawa, Junji, and Zhang, Huibo
- Subjects
Time Resolved Diagnostics and Synchronization ,Physics::Accelerator Physics ,Accelerator Physics - Abstract
It is proposed to use the polarization of coherent Smith-Purcell radiation (cSPr) to distinguish between the cSPr signal and background radiation in a single-shot longitudinal bunch profile monitor. A preliminary measurement of the polarization has been carried out using a 1mm periodic metallic grating installed at the 8MeV electron accelerator LUCX, KEK (Japan). The measured degree of polarization at '=90° (300GHz) is 72.6 ±%. To make a thorough test of the theoretical model, measurements of the degree of polarization must be taken at more emission angles - equivalent to more frequencies., Proceedings of the 5th Int. Beam Instrumentation Conf., IBIC2016, Barcelona, Spain more...
240. A laser-wire system at the ATF extraction line
- Author
-
Boogert, S. T., Blair, G., Boorman, G., Bosco, A., Deacon, L., Driouichi, C., Pavel Karataev, Kamps, T., Delerue, N., Dixit, S., Foster, B., Gannaway, F., Howell, D. F., Qureshi, M., Reichold, A., Senanayake, R., Aryshev, A., Hayano, H., Kubo, K., Terunuma, N., Urakawa, J., Jenner, L. J., Brachmann, A., Frisch, J., and Ross, M. more...
- Subjects
Accelerators and Storage Rings - Abstract
3 pp. (2006)., A new laser-wire (LW) system has been installed at the ATF extraction line at KEK, Tsukuba. The system aims at a micron-scale laser spot size and employs a mode-locked laser system. The purpose-built interaction chamber, light delivery optics, and lens systems are described, and the first results are presented. more...
- Full Text
- View/download PDF
241. Extremely low emittance beam size diagnostics with sub-micrometer resolution using optical transition radiation
- Author
-
Konstantin Kruchinin, Boogert, S. T., Karataev, P., Nevay, L. J., Bolzon, B., Lefevre, T., Mazzoni, S., Aryshev, A., Shevelev, M., Terunuma, N., and Urakawa, J.
- Subjects
Physics::Accelerator Physics ,Accelerators and Storage Rings - Abstract
Transition radiation (TR) appearing when relativistic uniformly moving charged particle (or bunch of particles) crosses a boundary between two media with different di- electric properties is widely used as a tool for diagnostics of particle beams in modern accelerator facilities. The best resolution which can be achieved using beam profile mon- itors based on TR in optical wave range has a limitation caused by a spatial resolution of an optical system. Using a method based on analyzing a visibility of the TR Point Spread Function one can achieve a sub-micrometer reso- lution. In this report we shall represent the recent exper- imental results of a micron-scale beam size measurement at KEK-ATF2. We shall discuss the hardware status and future plans. more...
242. International Linear Collider Reference Design Report Volume 2: Physics at the ILC
- Author
-
Djouadi, Abdelhak, Lykken, Joseph, Moenig, Klaus, Okada, Yasuhiro, Oreglia, Mark, Yamashita, Satoru, Aarons, Gerald, Abe, Toshinori, Abernathy, Jason, Ablikim, Medina, Abramowicz, Halina, Adey, David, Adloff, Catherine, Adolphsen, Chris, Afanaciev, Konstantin, Agapov, Ilya, Ahn, Jung-Keun, Aihara, Hiroaki, Akemoto, Mitsuo, Del Carmen Alabau, Maria, Albert, Justin, Albrecht, Hartwig, Albrecht, Michael, Alesini, David, Alexander, Gideon, Alexander, Jim, Allison, Wade, Amann, John, Amirikas, Ramila, An, Qi, Anami, Shozo, Ananthanarayan, B., Anderson, Terry, Andricek, Ladislav, Anduze, Marc, Anerella, Michael, Anfimov, Nikolai, Angal-Kalinin, Deepa, Antipov, Sergei, Antoine, Claire, Aoki, Mayumi, Aoza, Atsushi, Aplin, Steve, Appleby, Rob, Arai, Yasuo, Araki, Sakae, Arkan, Tug, Arnold, Ned, Arnold, Ray, Arnowitt, Richard, Artru, Xavier, Arya, Kunal, Aryshev, Alexander, Asakawa, Eri, Asiri, Fred, Asner, David, Atac, Muzaffer, Atoian, Grigor, Attié, David, Augustin, Jean-Eudes, Augustine, David B., Ayres, Bradley, Aziz, Tariq, Baars, Derek, Badaud, Frederique, Baddams, Nigel, Bagger, Jonathan, Bai, Sha, Bailey, David, Bailey, Ian R., Baker, David, Balalykin, Nikolai I., Balbuena, Juan Pablo, Baldy, Jean-Luc, Ball, Markus, Ball, Maurice, Ballestrero, Alessandro, Ballin, Jamie, Baltay, Charles, Bambade, Philip, Ban, Syuichi, Band, Henry, Bane, Karl, Banerjee, Bakul, Barbanotti, Serena, Barbareschi, Daniele, Barbaro-Galtieri, Angela, Barber, Desmond P., Barbi, Mauricio, Bardin, Dmitri Y., Barish, Barry, Barklow, Timothy L., Barlow, Roger, Barnes, Virgil E., Barone, Maura, Bartels, Christoph, Bartsch, Valeria, Basu, Rahul, Battaglia, Marco, Batygin, Yuri, Baudot, Jerome, Baur, Ulrich, Elwyn Baynham, D., Beard, Carl, Bebek, Chris, Bechtle, Philip, Becker, Ulrich J., Bedeschi, Franco, Bedjidian, Marc, Behera, Prafulla, Behnke, Ties, Bellantoni, Leo, Bellerive, Alain, Bellomo, Paul, Bentson, Lynn D., Benyamna, Mustapha, Bergauer, Thomas, Berger, Edmond, Bergholz, Matthias, Beri, Suman, Berndt, Martin, Bernreuther, Werner, Bertolini, Alessandro, Besancon, Marc, Besson, Auguste, Beteille, Andre, Bettoni, Simona, Beyer, Michael, Bhandari, R. K., Bharadwaj, Vinod, Bhatnagar, Vipin, Bhattacharya, Satyaki, Bhattacharyya, Gautam, Bhattacherjee, Biplob, Bhuyan, Ruchika, Bi, Xiao-Jun, Biagini, Marica, Bialowons, Wilhelm, Biebel, Otmar, Bieler, Thomas, Bierwagen, John, Birch, Alison, Bisset, Mike, Biswal, S. S., Blackmore, Victoria, Blair, Grahame, Blanchard, Guillaume, Blazey, Gerald, Blue, Andrew, Blümlein, Johannes, Boffo, Christian, Bohn, Courtlandt, Boiko, V. I., Boisvert, Veronique, Bondarchuk, Eduard N., Boni, Roberto, Bonvicini, Giovanni, Boogert, Stewart, Boonekamp, Maarten, Boorman, Gary, Borras, Kerstin, Bortoletto, Daniela, Bosco, Alessio, Bosio, Carlo, Bosland, Pierre, Bosotti, Angelo, Boudry, Vincent, Boumediene, Djamel-Eddine, Bouquet, Bernard, Bourov, Serguei, Bowden, Gordon, Bower, Gary, Boyarski, Adam, Bozovic-Jelisavcic, Ivanka, Bozzi, Concezio, Brachmann, Axel, Bradshaw, Tom W., Brandt, Andrew, Brasser, Hans Peter, Brau, Benjamin, Brau, James E., Breidenbach, Martin, Bricker, Steve, Brient, Jean-Claude, Brock, Ian, Brodsky, Stanley, Brooksby, Craig, Broome, Timothy A., Brown, David Nathan, Brown, David Norvil, Brownell, James H., Bruchon, Mélanie, Brueck, Heiner, Brummitt, Amanda J., Brun, Nicole, Buchholz, Peter, Budagov, Yulian A., Bulgheroni, Antonio, Bulyak, Eugene, Bungau, Adriana, Bürger, Jochen, Burke, Dan, Burkhart, Craig, Burrows, Philip, Burt, Graeme, Burton, David, Büsser, Karsten, Butler, John, Butterworth, Jonathan, Buzulutskov, Alexei, Cabruja, Enric, Caccia, Massimo, Cai, Yunhai, Calcaterra, Alessandro, Caliier, Stephane, Camporesi, Tiziano, Cao, Jun-Jie, Cao, J. S., Capatina, Ofelia, Cappellini, Chiara, Carcagno, Ruben, Carena, Marcela, Carloganu, Cristina, Carosi, Roberto, Stephen Carr, F., Carrion, Francisco, Carter, Harry F., Carter, John, Carwardine, John, Cassel, Richard, Cassell, Ronald, Cavallari, Giorgio, Cavallo, Emanuela, Cembranos, Jose A. R., Chakraborty, Dhiman, Chandez, Frederic, Charles, Matthew, Chase, Brian, Chattopadhyay, Subhasis, Chauveau, Jacques, Chefdeville, Maximilien, Chehab, Robert, Chel, Stéphane, Chelkov, Georgy, Chen, Chiping, Chen, He Sheng, Chen, Huai Bi, Chen, Jia Er, Chen, Sen Yu, Chen, Shaomin, Chen, Shenjian, Chen, Xun, Chen, Yuan Bo, Cheng, Jian, Chevallier, M., Chi, Yun Long, Chickering, William, Cho, Gi-Chol, Cho, Moo-Hyun, Choi, Jin-Hyuk, Choi, Jong Bum, Choi, Seong Youl, Choi, Young-Il, Choudhary, Brajesh, Choudhury, Debajyoti, Rai Choudhury, S., Christian, David, Christian, Glenn, Christophe, Grojean, Chung, Jin-Hyuk, Church, Mike, Ciborowski, Jacek, Cihangir, Selcuk, Ciovati, Gianluigi, Clarke, Christine, Clarke, Don G., Clarke, James A., Clements, Elizabeth, Coca, Cornelia, Coe, Paul, Cogan, John, Colas, Paul, Collard, Caroline, Colledani, Claude, Combaret, Christophe, Comerma, Albert, Compton, Chris, Constance, Ben, Conway, John, Cook, Ed, Cooke, Peter, Cooper, William, Corcoran, Sean, Cornat, Rémi, Corner, Laura, Cortina Gil, Eduardo, Clay Corvin, W., Cotta Ramusino, Angelo, Cowan, Ray, Crawford, Curtis, Cremaldi, Lucien M., Crittenden, James A., Cussans, David, Cvach, Jaroslav, Da Silva, Wilfrid, Dabiri Khah, Hamid, Dabrowski, Anne, Dabrowski, Wladyslaw, Dadoun, Olivier, Dai, Jian Ping, Dainton, John, Daly, Colin, Damerell, Chris, Danilov, Mikhail, Daniluk, Witold, Daram, Sarojini, Datta, Anindya, Dauncey, Paul, David, Jacques, Davier, Michel, Davies, Ken P., Dawson, Sally, Boer, Wim, Curtis, Stefania, Groot, Nicolo, La Taille, Christophe, Lira, Antonio, Roeck, Albert, Sangro, Riccardo, Santis, Stefano, Deacon, Laurence, Deandrea, Aldo, Dehmelt, Klaus, Delagnes, Eric, Delahaye, Jean-Pierre, Delebecque, Pierre, Delerue, Nicholas, Delferriere, Olivier, Demarteau, Marcel, Deng, Zhi, Denisov, Yu N., Densham, Christopher J., Desch, Klaus, Deshpande, Nilendra, Devanz, Guillaume, Devetak, Erik, Dexter, Amos, Di Benedetto, Vito, Diéguez, Angel, Diener, Ralf, Dinh, Nguyen Dinh, Dixit, Madhu, Dixit, Sudhir, Dolezal, Zdenek, Dollan, Ralph, Dong, Dong, Dong, Hai Yi, Dorfan, Jonathan, Dorokhov, Andrei, Doucas, George, Downing, Robert, Doyle, Eric, Doziere, Guy, Drago, Alessandro, Dragt, Alex, Drake, Gary, Drásal, Zbynek, Dreiner, Herbert, Drell, Persis, Driouichi, Chafik, Drozhdin, Alexandr, Drugakov, Vladimir, Du, Shuxian, Dugan, Gerald, Duginov, Viktor, Dulinski, Wojciech, Dulucq, Frederic, Dutta, Sukanta, Dwivedi, Jishnu, Dychkant, Alexandre, Dzahini, Daniel, Eckerlin, Guenter, Edwards, Helen, Ehrenfeld, Wolfgang, Ehrlichman, Michael, Ehrlichmann, Heiko, Eigen, Gerald, Elagin, Andrey, Elementi, Luciano, Eliasson, Peder, Ellis, John, Ellwood, George, Elsen, Eckhard, Emery, Louis, Enami, Kazuhiro, Endo, Kuninori, Enomoto, Atsushi, Eozénou, Fabien, Erbacher, Robin, Erickson, Roger, Oleg Eyser, K., Fadeyev, Vitaliy, Fang, Shou Xian, Fant, Karen, Fasso, Alberto, Faucci Giannelli, Michele, Fehlberg, John, Feld, Lutz, Feng, Jonathan L., Ferguson, John, Fernandez-Garcia, Marcos, Luis Fernandez-Hernando, J., Fiala, Pavel, Fieguth, Ted, Finch, Alexander, Finocchiaro, Giuseppe, Fischer, Peter, Fisher, Peter, Eugene Fisk, H., Fitton, Mike D., Fleck, Ivor, Fleischer, Manfred, Fleury, Julien, Flood, Kevin, Foley, Mike, Ford, Richard, Fortin, Dominique, Foster, Brian, Fourches, Nicolas, Francis, Kurt, Frey, Ariane, Frey, Raymond, Friedsam, Horst, Frisch, Josef, Frishman, Anatoli, Fuerst, Joel, Fujii, Keisuke, Fujimoto, Junpei, Fukuda, Masafumi, Fukuda, Shigeki, Funahashi, Yoshisato, Funk, Warren, Furletova, Julia, Furukawa, Kazuro, Furuta, Fumio, Fusayasu, Takahiro, Fuster, Juan, Gadow, Karsten, Gaede, Frank, Gaglione, Renaud, Gai, Wei, Gajewski, Jan, Galik, Richard, Galkin, Alexei, Galkin, Valery, Gallin-Martel, Laurent, Gannaway, Fred, Gao, Jian She, Gao, Jie, Gao, Yuanning, Garbincius, Peter, Garcia-Tabares, Luis, Garren, Lynn, Garrido, Luís, Garutti, Erika, Garvey, Terry, Garwin, Edward, Gascón, David, Gastal, Martin, Gatto, Corrado, Gatto, Raoul, Gay, Pascal, Ge, Lixin, Ge, Ming Qi, Ge, Rui, Geiser, Achim, Gellrich, Andreas, Genat, Jean-Francois, Geng, Zhe Qiao, Gentile, Simonetta, Gerbick, Scot, Gerig, Rod, Ghosh, Dilip Kumar, Ghosh, Kirtiman, Gibbons, Lawrence, Giganon, Arnaud, Gillespie, Allan, Gillman, Tony, Ginzburg, Ilya, Giomataris, Ioannis, Giunta, Michele, Gladkikh, Peter, Gluza, Janusz, Godbole, Rohini, Godfrey, Stephen, Goldhaber, Gerson, Goldstein, Joel, Gollin, George D., Gonzalez-Sanchez, Francisco Javier, Goodrick, Maurice, Gornushkin, Yuri, Gostkin, Mikhail, Gottschalk, Erik, Goudket, Philippe, Gough Eschrich, Ivo, Gournaris, Filimon, Graciani, Ricardo, Graf, Norman, Grah, Christian, Grancagnolo, Francesco, Grandjean, Damien, Grannis, Paul, Grassellino, Anna, Graugés, Eugeni, Gray, Stephen, Green, Michael, Greenhalgh, Justin, Greenshaw, Timothy, Grefe, Christian, Gregor, Ingrid-Maria, Grenier, Gerald, Grimes, Mark, Grimm, Terry, Gris, Philippe, Grivaz, Jean-Francois, Groll, Marius, Gronberg, Jeffrey, Grondin, Denis, Groom, Donald, Gross, Eilam, Grunewald, Martin, Grupen, Claus, Grzelak, Grzegorz, Gu, Jun, Gu, Yun-Ting, Guchait, Monoranjan, Guiducci, Susanna, Guler, Ali Murat, Guler, Hayg, Gulmez, Erhan, Gunion, John, Guo, Zhi Yu, Gurtu, Atul, Ha, Huy Bang, Haas, Tobias, Haase, Andy, Haba, Naoyuki, Haber, Howard, Haensel, Stephan, Hagge, Lars, Hagura, Hiroyuki, Hajdu, Csaba, Haller, Gunther, Haller, Johannes, Hallermann, Lea, Halyo, Valerie, Hamaguchi, Koichi, Hammond, Larry, Han, Liang, Han, Tao, Hand, Louis, Handu, Virender K., Hano, Hitoshi, Hansen, Christian, Hansen, Jørn Dines, Hansen, Jorgen Beck, Hara, Kazufumi, Harder, Kristian, Hartin, Anthony, Hartung, Walter, Hast, Carsten, Hauptman, John, Hauschild, Michael, Hauviller, Claude, Havranek, Miroslav, Hawkes, Chris, Hawkings, Richard, Hayano, Hitoshi, Hazumi, Masashi, He, An, He, Hong Jian, Hearty, Christopher, Heath, Helen, Hebbeker, Thomas, Hedberg, Vincent, Hedin, David, Heifets, Samuel, Heinemeyer, Sven, Heini, Sebastien, Helebrant, Christian, Helms, Richard, Heltsley, Brian, Henrot-Versille, Sophie, Henschel, Hans, Hensel, Carsten, Hermel, Richard, Herms, Atilà, Herten, Gregor, Hesselbach, Stefan, Heuer, Rolf-Dieter, Heusch, Clemens A., Hewett, Joanne, Higashi, Norio, Higashi, Takatoshi, Higashi, Yasuo, Higo, Toshiyasu, Hildreth, Michael D., Hiller, Karlheinz, Hillert, Sonja, Hillier, Stephen James, Himel, Thomas, Himmi, Abdelkader, Hinchliffe, Ian, Hioki, Zenro, Hirano, Koichiro, Hirose, Tachishige, Hisamatsu, Hiromi, Hisano, Junji, Hlaing, Chit Thu, Hock, Kai Meng, Hoeferkamp, Martin, Hohlfeld, Mark, Honda, Yousuke, Hong, Juho, Hong, Tae Min, Honma, Hiroyuki, Horii, Yasuyuki, Horvath, Dezso, Hosoyama, Kenji, Hostachy, Jean-Yves, Hou, Mi, Hou, Wei-Shu, Howell, David, Hronek, Maxine, Hsiung, Yee B., Hu, Bo, Hu, Tao, Huang, Jung-Yun, Huang, Tong Ming, Huang, Wen Hui, Huedem, Emil, Huggard, Peter, Hugonie, Cyril, Hu-Guo, Christine, Huitu, Katri, Hwang, Youngseok, Idzik, Marek, Ignatenko, Alexandr, Ignatov, Fedor, Ikeda, Hirokazu, Ikematsu, Katsumasa, Ilicheva, Tatiana, Imbault, Didier, Imhof, Andreas, Incagli, Marco, Ingbir, Ronen, Inoue, Hitoshi, Inoue, Youichi, Introzzi, Gianluca, Ioakeimidi, Katerina, Ishihara, Satoshi, Ishikawa, Akimasa, Ishikawa, Tadashi, Issakov, Vladimir, Ito, Kazutoshi, Ivanov, V. V., Ivanov, Valentin, Ivanyushenkov, Yury, Iwasaki, Masako, Iwashita, Yoshihisa, Jackson, David, Jackson, Frank, Jacobsen, Bob, Jaganathan, Ramaswamy, Jamison, Steven, Janssen, Matthias Enno, Jaramillo-Echeverria, Richard, Jaros, John, Jauffret, Clement, Jawale, Suresh B., Jeans, Daniel, Jedziniak, Ron, Jeffery, Ben, Jehanno, Didier, Jenner, Leo J., Jensen, Chris, Jensen, David R., Jiang, Hairong, Jiang, Xiao Ming, Jimbo, Masato, Jin, Shan, Keith Jobe, R., Johnson, Anthony, Johnson, Erik, Johnson, Matt, Johnston, Michael, Joireman, Paul, Jokic, Stevan, Jones, James, Jones, Roger M., Jongewaard, Erik, Jönsson, Leif, Joshi, Gopal, Joshi, Satish C., Jung, Jin-Young, Junk, Thomas, Juste, Aurelio, Kado, Marumi, Kadyk, John, Käfer, Daniela, Kako, Eiji, Kalavase, Puneeth, Kalinin, Alexander, Kalinowski, Jan, Kamitani, Takuya, Kamiya, Yoshio, Kamiya, Yukihide, Kamoshita, Jun-Ichi, Kananov, Sergey, Kanaya, Kazuyuki, Kanazawa, Ken-Ichi, Kanemura, Shinya, Kang, Heung-Sik, Kang, Wen, Kanjial, D., Kapusta, Frédéric, Karataev, Pavel, Karchin, Paul E., Karlen, Dean, Karyotakis, Yannis, Kashikhin, Vladimir, Kashiwagi, Shigeru, Kasley, Paul, Katagiri, Hiroaki, Kato, Takashi, Kato, Yukihiro, Katzy, Judith, Kaukher, Alexander, Kaur, Manjit, Kawagoe, Kiyotomo, Kawamura, Hiroyuki, Kazakov, Sergei, Kekelidze, V. D., Keller, Lewis, Kelley, Michael, Kelly, Marc, Kelly, Michael, Kennedy, Kurt, Kephart, Robert, Keung, Justin, Khainovski, Oleg, Khan, Sameen Ahmed, Khare, Prashant, Khovansky, Nikolai, Kiesling, Christian, Kikuchi, Mitsuo, Kilian, Wolfgang, Killenberg, Martin, Kim, Donghee, Kim, Eun San, Kim, Eun-Joo, Kim, Guinyun, Kim, Hongjoo, Kim, Hyoungsuk, Kim, Hyun-Chui, Kim, Jonghoon, Kim, Kwang-Je, Kim, Kyung Sook, Kim, Peter, Kim, Seunghwan, Kim, Shin-Hong, Kim, Sun Kee, Kim, Tae Jeong, Kim, Youngim, Kim, Young-Kee, Kimmitt, Maurice, Kirby, Robert, Kircher, François, Kisielewska, Danuta, Kittel, Olaf, Klanner, Robert, Klebaner, Arkadiy L., Kleinwort, Claus, Klimkovich, Tatsiana, Klinkby, Esben, Kluth, Stefan, Knecht, Marc, Kneisel, Peter, Ko, In Soo, Ko, Kwok, Kobayashi, Makoto, Kobayashi, Nobuko, Kobel, Michael, Koch, Manuel, Kodys, Peter, Koetz, Uli, Kohrs, Robert, Kojima, Yuuji, Kolanoski, Hermann, Kolodziej, Karol, Kolomensky, Yury G., Komamiya, Sachio, Kong, Xiang Cheng, Konigsberg, Jacobo, Korbel, Volker, Koscielniak, Shane, Kostromin, Sergey, Kowalewski, Robert, Kraml, Sabine, Krammer, Manfred, Krasnykh, Anatoly, Krautscheid, Thorsten, Krawczyk, Maria, James Krebs, H., Krempetz, Kurt, Kribs, Graham, Krishnagopal, Srinivas, Kriske, Richard, Kronfeld, Andreas, Kroseberg, Jürgen, Kruchonak, Uladzimir, Kruecker, Dirk, Krüger, Hans, Krumpa, Nicholas A., Krumshtein, Zinovii, Kuang, Yu Ping, Kubo, Kiyoshi, Kuchler, Vic, Kudoh, Noboru, Kulis, Szymon, Kumada, Masayuki, Kumar, Abhay, Kume, Tatsuya, Kundu, Anirban, Kurevlev, German, Kurihara, Yoshimasa, Kuriki, Masao, Kuroda, Shigeru, Kuroiwa, Hirotoshi, Kurokawa, Shin-Ichi, Kusano, Tomonori, Kush, Pradeep K., Kutschke, Robert, Kuznetsova, Ekaterina, Kvasnicka, Peter, Kwon, Youngjoon, Labarga, Luis, Lacasta, Carlos, Lackey, Sharon, Lackowski, Thomas W., Lafaye, Remi, Lafferty, George, Lagorio, Eric, Laktineh, Imad, Lal, Shankar, Laloum, Maurice, Lam, Briant, Lancaster, Mark, Lander, Richard, Lange, Wolfgang, Langenfeld, Ulrich, Langeveld, Willem, Larbalestier, David, Larsen, Ray, Lastovicka, Tomas, Lastovicka-Medin, Gordana, Latina, Andrea, Latour, Emmanuel, Laurent, Lisa, Le, Ba Nam, Le, Duc Ninh, Le Diberder, Francois, Dû, Patrick Le, Lebbolo, Hervé, Lebrun, Paul, Lecoq, Jacques, Lee, Sung-Won, Lehner, Frank, Leibfritz, Jerry, Lenkszus, Frank, Lesiak, Tadeusz, Levy, Aharon, Lewandowski, Jim, Leyh, Greg, Li, Cheng, Li, Chong Sheng, Li, Chun Hua, Li, Da Zhang, Li, Gang, Li, Jin, Li, Shao Peng, Li, Wei Ming, Li, Weiguo, Li, Xiao Ping, Li, Xue-Qian, Li, Yuanjing, Li, Yulan, Li, Zenghai, Li, Zhong Quan, Liang, Jian Tao, Liao, Yi, Lilje, Lutz, Guilherme Lima, J., Lintern, Andrew J., Lipton, Ronald, List, Benno, List, Jenny, Liu, Chun, Liu, Jian Fei, Liu, Ke Xin, Liu, Li Qiang, Liu, Shao Zhen, Liu, Sheng Guang, Liu, Shubin, Liu, Wanming, Liu, Wei Bin, Liu, Ya Ping, Liu, Yu Dong, Lockyer, Nigel, Logan, Heather E., Logatchev, Pavel V., Lohmann, Wolfgang, Lohse, Thomas, Lola, Smaragda, Lopez-Virto, Amparo, Loveridge, Peter, Lozano, Manuel, Lu, Cai-Dian, Lu, Changguo, Lu, Gong-Lu, Lu, Wen Hui, Lubatti, Henry, Lucotte, Arnaud, Lundberg, Björn, Lundin, Tracy, Luo, Mingxing, Luong, Michel, Luth, Vera, Lutz, Benjamin, Lutz, Pierre, Lux, Thorsten, Luzniak, Pawel, Lyapin, Alexey, Lynch, Clare, Ma, Li, Ma, Lili, Ma, Qiang, Ma, Wen-Gan, Macfarlane, David, Maciel, Arthur, Macleod, Allan, Macnair, David, Mader, Wolfgang, Magill, Stephen, Magnan, Anne-Marie, Maiheu, Bino, Maity, Manas, Majchrzak, Millicent, Majumder, Gobinda, Makarov, Roman, Makowski, Dariusz, Malaescu, Bogdan, Mallik, C., Mallik, Usha, Malton, Stephen, Malyshev, Oleg B., Malysheva, Larisa I., Mammosser, John, Mamta, Mamuzic, Judita, Manen, Samuel, Manghisoni, Massimo, Manly, Steven, Marcellini, Fabio, Marcisovsky, Michal, Markiewicz, Thomas W., Marks, Steve, Marone, Andrew, Marti, Felix, Martin, Jean-Pierre, Martin, Victoria, Martin-Chassard, Gisèle, Martinez, Manel, Martinez-Rivero, Celso, Martsch, Dennis, Martyn, Hans-Ulrich, Maruyama, Takashi, Masuzawa, Mika, Mathez, Hervé, Matsuda, Takeshi, Matsumoto, Hiroshi, Matsumoto, Shuji, Matsumoto, Toshihiro, Matsunaga, Hiroyuki, Mättig, Peter, Mattison, Thomas, Mavromanolakis, Georgios, Mawatari, Kentarou, Mazzacane, Anna, Mcbride, Patricia, Mccormick, Douglas, Mccormick, Jeremy, Mcdonald, Kirk T., Mcgee, Mike, Mcintosh, Peter, Mckee, Bobby, Mcpherson, Robert A., Meidlinger, Mandi, Meier, Karlheinz, Mele, Barbara, Meller, Bob, Melzer-Pellmann, Isabell-Alissandra, Mendez, Hector, Mercer, Adam, Merkin, Mikhail, Meshkov, I. N., Messner, Robert, Metcalfe, Jessica, Meyer, Chris, Meyer, Hendrik, Meyer, Joachim, Meyer, Niels, Meyners, Norbert, Michelato, Paolo, Michizono, Shinichiro, Mihalcea, Daniel, Mihara, Satoshi, Mihara, Takanori, Mikami, Yoshinari, Mikhailichenko, Alexander A., Milardi, Catia, Miller, David J., Miller, Owen, Miller, Roger J., Milstene, Caroline, Mimashi, Toshihiro, Minashvili, Irakli, Miquel, Ramon, Mishra, Shekhar, Mitaroff, Winfried, Mitchell, Chad, Miura, Takako, Miyamoto, Akiya, Miyata, Hitoshi, Mjörnmark, Ulf, Mnich, Joachim, Moffeit, Kenneth, Mokhov, Nikolai, Molloy, Stephen, Monaco, Laura, Monasterio, Paul R., Montanari, Alessandro, Moon, Sung Ik, Moortgat-Pick, Gudrid A., Mora Freitas, Paulo, Morel, Federic, Moretti, Stefano, Morgunov, Vasily, Mori, Toshinori, Morin, Laurent, Morisseau, François, Morita, Yoshiyuki, Morita, Youhei, Morita, Yuichi, Morozov, Nikolai, Morozumi, Yuichi, Morse, William, Moser, Hans-Guenther, Moultaka, Gilbert, Mtingwa, Sekazi, Mudrinic, Mihajlo, Mueller, Alex, Mueller, Wolfgang, Muennich, Astrid, Muhlleitner, Milada Margarete, Mukherjee, Bhaskar, Mukhopadhyaya, Biswarup, Müller, Thomas, Munro, Morrison, Murayama, Hitoshi, Muto, Toshiya, Myneni, Ganapati Rao, Nabhiraj, P. Y., Nagaitsev, Sergei, Nagamine, Tadashi, Nagano, Ai, Naito, Takashi, Nakai, Hirotaka, Nakajima, Hiromitsu, Nakamura, Isamu, Nakamura, Tomoya, Nakanishi, Tsutomu, Nakao, Katsumi, Nakao, Noriaki, Nakayoshi, Kazuo, Nam, Sang, Namito, Yoshihito, Namkung, Won, Nantista, Chris, Napoly, Olivier, Narain, Meenakshi, Naroska, Beate, Nauenberg, Uriel, Nayyar, Ruchika, Neal, Homer, Nelson, Charles, Nelson, Janice, Nelson, Timothy, Nemecek, Stanislav, Neubauer, Michael, Neuffer, David, Newman, Myriam Q., Nezhevenko, Oleg, Ng, Cho-Kuen, Nguyen, Anh Ky, Nguyen, Minh, Nguyen Thi, Hong, Niebuhr, Carsten, Niehoff, Jim, Niezurawski, Piotr, Nishitani, Tomohiro, Nitoh, Osamu, Noguchi, Shuichi, Nomerotski, Andrei, Noonan, John, Norbeck, Edward, Nosochkov, Yuri, Notz, Dieter, Nowak, Grazyna, Nowak, Hannelies, Noy, Matthew, Nozaki, Mitsuaki, Nyffeler, Andreas, Nygren, David, Oddone, Piermaria, O, Joseph, Oh, Jong-Seok, Oh, Sun Kun, Ohkuma, Kazumasa, Ohlerich, Martin, Ohmi, Kazuhito, Ohnishi, Yukiyoshi, Ohsawa, Satoshi, Ohuchi, Norihito, Oide, Katsunobu, Okada, Nobuchika, Okamura, Takahiro, Okugi, Toshiyuki, Okumi, Shoji, Okumura, Ken-Ichi, Olchevski, Alexander, Oliver, William, Olivier, Bob, Olsen, James, Olsen, Jeff, Olsen, Stephen, Olshevsky, A. G., Olsson, Jan, Omori, Tsunehiko, Onel, Yasar, Onengut, Gulsen, Ono, Hiroaki, Onoprienko, Dmitry, Oren, Will, Orimoto, Toyoko J., Oriunno, Marco, Orlandea, Marius Ciprian, Oroku, Masahiro, Orr, Lynne H., Orr, Robert S., Oshea, Val, Oskarsson, Anders, Osland, Per, Ossetski, Dmitri, Österman, Lennart, Ostiguy, Francois, Otono, Hidetoshi, Ottewell, Brian, Ouyang, Qun, Padamsee, Hasan, Padilla, Cristobal, Pagani, Carlo, Palmer, Mark A., Pam, Wei Min, Pande, Manjiri, Pande, Rajni, Pandit, V. S., Pandita, P. N., Pandurovic, Mila, Pankov, Alexander, Panzeri, Nicola, Papandreou, Zisis, Paparella, Rocco, Para, Adam, Park, Hwanbae, Parker, Brett, Parkes, Chris, Parma, Vittorio, Parsa, Zohreh, Parsons, Justin, Partridge, Richard, Pasquinelli, Ralph, Gabriella Pásztor, Paterson, Ewan, Patrick, Jim, Patteri, Piero, Ritchie Patterson, J., Pauletta, Giovanni, Paver, Nello, Pavlicek, Vince, Pawlik, Bogdan, Payet, Jacques, Pchalek, Norbert, Pedersen, John, Pei, Guo Xi, Pei, Shi Lun, Pelka, Jerzy, Pellegrini, Giulio, Pellett, David, Peng, G. X., Penn, Gregory, Penzo, Aldo, Perry, Colin, Peskin, Michael, Peters, Franz, Petersen, Troels Christian, Peterson, Daniel, Peterson, Thomas, Petterson, Maureen, Pfeffer, Howard, Pfund, Phil, Phelps, Alan, Phi, Quang, Phillips, Jonathan, Phinney, Nan, Piccolo, Marcello, Piemontese, Livio, Pierini, Paolo, Thomas Piggott, W., Pike, Gary, Pillet, Nicolas, Jayawardena, Talini Pinto, Piot, Phillippe, Pitts, Kevin, Pivi, Mauro, Plate, Dave, Pleier, Marc-Andre, Poblaguev, Andrei, Poehler, Michael, Poelker, Matthew, Poffenberger, Paul, Pogorelsky, Igor, Poirier, Freddy, Poling, Ronald, Poole, Mike, Popescu, Sorina, Popielarski, John, Pöschl, Roman, Postranecky, Martin, Potukochi, Prakash N., Prast, Julie, Prat, Serge, Preger, Miro, Prepost, Richard, Price, Michael, Proch, Dieter, Puntambekar, Avinash, Qin, Qing, Qu, Hua Min, Quadt, Arnulf, Quesnel, Jean-Pierre, Radeka, Veljko, Rahmat, Rahmat, Rai, Santosh Kumar, Raimondi, Pantaleo, Ramberg, Erik, Ranjan, Kirti, Rao, Sista V. L. S., Raspereza, Alexei, Ratti, Alessandro, Ratti, Lodovico, Raubenheimer, Tor, Raux, Ludovic, Ravindran, V., Raychaudhuri, Sreerup, Re, Valerio, Rease, Bill, Reece, Charles E., Regler, Meinhard, Rehlich, Kay, Reichel, Ina, Reichold, Armin, Reid, John, Reid, Ron, Reidy, James, Reinhard, Marcel, Renz, Uwe, Repond, Jose, Resta-Lopez, Javier, Reuen, Lars, Ribnik, Jacob, Rice, Tyler, Richard, François, Riemann, Sabine, Riemann, Tord, Riles, Keith, Riley, Daniel, Rimbault, Cécile, Rindani, Saurabh, Rinolfi, Louis, Risigo, Fabio, Riu, Imma, Rizhikov, Dmitri, Rizzo, Thomas, Rochford, James H., Rodriguez, Ponciano, Roeben, Martin, Rolandi, Gigi, Roodman, Aaron, Rosenberg, Eli, Roser, Robert, Ross, Marc, Rossel, François, Rossmanith, Robert, Roth, Stefan, Rougé, André, Rowe, Allan, Roy, Amit, Roy, Sendhunil B., Roy, Sourov, Royer, Laurent, Royole-Degieux, Perrine, Royon, Christophe, Ruan, Manqi, Rubin, David, Ruehl, Ingo, Jimeno, Alberto Ruiz, Ruland, Robert, Rusnak, Brian, Ryu, Sun-Young, Sabbi, Gian Luca, Sadeh, Iftach, Sadygov, Ziraddin Y., Saeki, Takayuki, Sagan, David, Sahni, Vinod C., Saini, Arun, Saito, Kenji, Saito, Kiwamu, Sajot, Gerard, Sakanaka, Shogo, Sakaue, Kazuyuki, Salata, Zen, Salih, Sabah, Salvatore, Fabrizio, Samson, Joergen, Sanami, Toshiya, Levi Sanchez, Allister, Sands, William, Santic, John, Sanuki, Tomoyuki, Sapronov, Andrey, Sarkar, Utpal, Sasao, Noboru, Satoh, Kotaro, Sauli, Fabio, Saunders, Claude, Saveliev, Valeri, Savoy-Navarro, Aurore, Sawyer, Lee, Saxton, Laura, Schäfer, Oliver, Schälicke, Andreas, Schade, Peter, Schaetzel, Sebastien, Scheitrum, Glenn, Schibler, Emilie, Schindler, Rafe, Schlösser, Markus, Schlueter, Ross D., Schmid, Peter, Schmidt, Ringo Sebastian, Schneekloth, Uwe, Schreiber, Heinz Juergen, Schreiber, Siegfried, Schroeder, Henning, Peter Schüler, K., Schulte, Daniel, Schultz-Coulon, Hans-Christian, Schumacher, Markus, Schumann, Steffen, Schumm, Bruce A., Schwienhorst, Reinhard, Schwierz, Rainer, Scott, Duncan J., Scuri, Fabrizio, Sefkow, Felix, Sefri, Rachid, Seguin-Moreau, Nathalie, Seidel, Sally, Seidman, David, Sekmen, Sezen, Seletskiy, Sergei, Senaha, Eibun, Senanayake, Rohan, Sendai, Hiroshi, Sertore, Daniele, Seryi, Andrei, Settles, Ronald, Sever, Ramazan, Shales, Nicholas, Shao, Ming, Shelkov, G. A., Shepard, Ken, Shepherd-Themistocleous, Claire, Sheppard, John C., Shi, Cai Tu, Shidara, Tetsuo, Shim, Yeo-Jeong, Shimizu, Hirotaka, Shimizu, Yasuhiro, Shimizu, Yuuki, Shimogawa, Tetsushi, Shin, Seunghwan, Shioden, Masaomi, Shipsey, Ian, Shirkov, Grigori, Shishido, Toshio, Shivpuri, Ram K., Shrivastava, Purushottam, Shulga, Sergey, Shumeiko, Nikolai, Shuvalov, Sergey, Si, Zongguo, Siddiqui, Azher Majid, Siegrist, James, Simon, Claire, Simrock, Stefan, Sinev, Nikolai, Singh, Bhartendu K., Singh, Jasbir, Singh, Pitamber, Singh, R. K., Singh, S. K., Singini, Monito, Sinha, Anil K., Sinha, Nita, Sinha, Rahul, Sinram, Klaus, Sissakian, A. N., Skachkov, N. B., Skrinsky, Alexander, Slater, Mark, Slominski, Wojciech, Smiljanic, Ivan, Smith, A. J. Stewart, Smith, Alex, Smith, Brian J., Smith, Jeff, Smith, Jonathan, Smith, Steve, Smith, Susan, Smith, Tonee, Neville Snodgrass, W., Sobloher, Blanka, Sohn, Young-Uk, Solidum, Ruelson, Solyak, Nikolai, Son, Dongchul, Sonmez, Nasuf, Sopczak, Andre, Soskov, V., Spencer, Cherrill M., Spentzouris, Panagiotis, Speziali, Valeria, Spira, Michael, Sprehn, Daryl, Sridhar, K., Srivastava, Asutosh, St Lorant, Steve, Stahl, Achim, Stanek, Richard P., Stanitzki, Marcel, Stanley, Jacob, Stefanov, Konstantin, Stein, Werner, Steiner, Herbert, Stenlund, Evert, Stern, Amir, Sternberg, Matt, Stockinger, Dominik, Stockton, Mark, Stoeck, Holger, Strachan, John, Strakhovenko, V., Strauss, Michael, Striganov, Sergei I., Strologas, John, Strom, David, Strube, Jan, Stupakov, Gennady, Su, Dong, Sudo, Yuji, Suehara, Taikan, Suehiro, Toru, Suetsugu, Yusuke, Sugahara, Ryuhei, Sugimoto, Yasuhiro, Sugiyama, Akira, Suh, Jun Suhk, Sukovic, Goran, Sun, Hong, Sun, Stephen, Sun, Werner, Sun, Yi, Sun, Yipeng, Suszycki, Leszek, Sutcliffe, Peter, Suthar, Rameshwar L., Suwada, Tsuyoshi, Suzuki, Atsuto, Suzuki, Chihiro, Suzuki, Shiro, Suzuki, Takashi, Swent, Richard, Swientek, Krzysztof, Swinson, Christina, Syresin, Evgeny, Szleper, Michal, Tadday, Alexander, Takahashi, Rika, Takahashi, Tohru, Takano, Mikio, Takasaki, Fumihiko, Takeda, Seishi, Takenaka, Tateru, Takeshita, Tohru, Takubo, Yosuke, Tanaka, Masami, Tang, Chuan Xiang, Taniguchi, Takashi, Tantawi, Sami, Tapprogge, Stefan, Tartaglia, Michael A., Tassielli, Giovanni Francesco, Tauchi, Toshiaki, Tavian, Laurent, Tawara, Hiroko, Taylor, Geoffrey, Telnov, Alexandre V., Telnov, Valery, Tenenbaum, Peter, Teodorescu, Eliza, Terashima, Akio, Terracciano, Giuseppina, Terunuma, Nobuhiro, Teubner, Thomas, Teuscher, Richard, Theilacker, Jay, Thomson, Mark, Tice, Jeff, Tigner, Maury, Timmermans, Jan, Titov, Maxim, Toge, Nobukazu, Tokareva, N. A., Tollefson, Kirsten, Tomasek, Lukas, Tomovic, Savo, Tompkins, John, Tonutti, Manfred, Topkar, Anita, Toprek, Dragan, Toral, Fernando, Torrence, Eric, Traversi, Gianluca, Trimpl, Marcel, Mani Tripathi, S., Trischuk, William, Trodden, Mark, Trubnikov, G. V., Tschirhart, Robert, Tskhadadze, Edisher, Tsuchiya, Kiyosumi, Tsukamoto, Toshifumi, Tsunemi, Akira, Tucker, Robin, Turchetta, Renato, Tyndel, Mike, Uekusa, Nobuhiro, Ueno, Kenji, Umemori, Kensei, Ummenhofer, Martin, Underwood, David, Uozumi, Satoru, Urakawa, Junji, Urban, Jeremy, Uriot, Didier, Urner, David, Ushakov, Andrei, Usher, Tracy, Uzunyan, Sergey, Vachon, Brigitte, Valerio, Linda, Valin, Isabelle, Valishev, Alex, Vamra, Raghava, Graaf, Harry, Kooten, Rick, Zandbergen, Gary, Vanel, Jean-Charles, Variola, Alessandro, Varner, Gary, Velasco, Mayda, Velte, Ulrich, Velthuis, Jaap, Vempati, Sundir K., Venturini, Marco, Vescovi, Christophe, Videau, Henri, Vila, Ivan, Vincent, Pascal, Virey, Jean-Marc, Visentin, Bernard, Viti, Michele, Vo, Thanh Cuong, Vogel, Adrian, Vogt, Harald, Toerne, Eckhard, Vorozhtsov, S. B., Vos, Marcel, Votava, Margaret, Vrba, Vaclav, Wackeroth, Doreen, Wagner, Albrecht, Wagner, Carlos E. M., Wagner, Stephen, Wake, Masayoshi, Walczak, Roman, Walker, Nicholas J., Walkowiak, Wolfgang, Wallon, Samuel, Walsh, Roberval, Walston, Sean, Waltenberger, Wolfgang, Walz, Dieter, Wang, Chao En, Wang, Chun Hong, Wang, Dou, Wang, Faya, Wang, Guang Wei, Wang, Haitao, Wang, Jiang, Wang, Jiu Qing, Wang, Juwen, Wang, Lanfa, Wang, Lei, Wang, Min-Zu, Wang, Qing, Wang, Shu Hong, Wang, Xiaolian, Wang, Xue-Lei, Wang, Yi Fang, Wang, Zheng, Wanzenberg, Rainer, Ward, Bennie, Ward, David, Warmbein, Barbara, Warner, David W., Warren, Matthew, Washio, Masakazu, Watanabe, Isamu, Watanabe, Ken, Watanabe, Takashi, Watanabe, Yuichi, Watson, Nigel, Wattimena, Nanda, Wayne, Mitchell, Weber, Marc, Weerts, Harry, Weiglein, Georg, Weiland, Thomas, Weinzierl, Stefan, Weise, Hans, Weisend, John, Wendt, Manfred, Wendt, Oliver, Wenzel, Hans, Wenzel, William A., Wermes, Norbert, Werthenbach, Ulrich, Wesseln, Steve, Wester, William, White, Andy, White, Glen R., Wichmann, Katarzyna, Wienemann, Peter, Wierba, Wojciech, Wilksen, Tim, Willis, William, Wilson, Graham W., Wilson, John A., Wilson, Robert, Wing, Matthew, Winter, Marc, Wirth, Brian D., Wolbers, Stephen A., Wolff, Dan, Wolski, Andrzej, Woodley, Mark D., Woods, Michael, Woodward, Michael L., Woolliscroft, Timothy, Worm, Steven, Wormser, Guy, Wright, Dennis, Wright, Douglas, Wu, Andy, Wu, Tao, Wu, Yue Liang, Xella, Stefania, Xia, Guoxing, Xia, Lei, Xiao, Aimin, Xiao, Liling, Xie, Jia Lin, Xing, Zhi-Zhong, Xiong, Lian You, Xu, Gang, Xu, Qing Jing, Yajnik, Urjit A., Yakimenko, Vitaly, Yamada, Ryuji, Yamaguchi, Hiroshi, Yamamoto, Akira, Yamamoto, Hitoshi, Yamamoto, Masahiro, Yamamoto, Naoto, Yamamoto, Richard, Yamamoto, Yasuchika, Yamanaka, Takashi, Yamaoka, Hiroshi, Yamazaki, Hideki, Yan, Wenbiao, Yang, Hai-Jun, Yang, Jin Min, Yang, Jongmann, Yang, Zhenwei, Yano, Yoshiharu, Yazgan, Efe, Yeh, G. P., Yilmaz, Hakan, Yock, Philip, Yoda, Hakutaro, Yoh, John, Yokoya, Kaoru, Yokoyama, Hirokazu, York, Richard C., Yoshida, Mitsuhiro, Yoshida, Takuo, Yoshioka, Tamaki, Young, Andrew, Yu, Cheng Hui, Yu, Jaehoon, Yu, Xian Ming, Yuan, Changzheng, Yue, Chong-Xing, Yue, Jun Hui, Zacek, Josef, Zagorodnov, Igor, Zalesak, Jaroslav, Zalikhanov, Boris, Zarnecki, Aleksander Filip, Zawiejski, Leszek, Zeitnitz, Christian, Zeller, Michael, Zerwas, Dirk, Zerwas, Peter, Zeyrek, Mehmet, Zhai, Ji Yuan, Zhang, Bao Cheng, Zhang, Bin, Zhang, Chuang, Zhang, He, Zhang, Jiawen, Zhang, Jing, Zhang, Jing Ru, Zhang, Jinlong, Zhang, Liang, Zhang, X., Zhang, Yuan, Zhang, Zhige, Zhang, Zhiqing, Zhang, Ziping, Zhao, Haiwen, Zhao, Ji Jiu, Zhao, Jing Xia, Zhao, Ming Hua, Zhao, Sheng Chu, Zhao, Tianchi, Zhao, Tong Xian, Zhao, Zhen Tang, Zhao, Zhengguo, Zhou, Min, Zhou, Feng, Zhou, Shun, Zhu, Shou Hua, Zhu, Xiong Wei, Zhukov, Valery, Zimmermann, Frank, Ziolkowski, Michael, Zisman, Michael S., Zomer, Fabian, Zong, Zhang Guo, Zorba, Osman, and Zutshi, Vishnu more...
- Subjects
Physics::Instrumentation and Detectors ,High Energy Physics::Phenomenology ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,hep-ph - Abstract
This article reviews the physics case for the ILC. Baseline running at 500 GeV as well as possible upgrades and options are discussed. The opportunities on Standard Model physics, Higgs physics, Supersymmetry and alternative theories beyond the Standard Model are described. This article reviews the physics case for the ILC. Baseline running at 500 GeV as well as possible upgrades and options are discussed. The opportunities on Standard Model physics, Higgs physics, Supersymmetry and alternative theories beyond the Standard Model are described. more...
243. Results of the high resolution OTR measurements at KEK and comparison with simulations
- Author
-
Bolzon, B., Lefevre, T., Stefano Mazzoni, Welsch, C. P., Karataev, P., Kruchinin, K., and Aryshev, A.
- Subjects
Physics::Accelerator Physics ,Accelerators and Storage Rings - Abstract
Optical Transition Radiation (OTR) is emitted when a charged particle crosses the interface between two media with different dielectric properties. It has become a standard tool for beam imaging and transverse beam size measurements. At the KEK Accelerator Test Facility 2 (ATF2), OTR is used at the beginning of the final focus system to measure micrometre beam size using the visibility of the OTR Point Spread Function (PSF). In order to study in detail the PSF and improve the resolution of the monitor, a novel simulation tool has been developed. Based on the physical optic propagation mode of ZEMAX, the propagation of the OTR electric field can be simulated very precisely up to the image plane, taking into account aberrations and diffraction. This contribution presents the comparison between Zemax simulations and measurements performed at ATF2. more...
244. Feasibility of THz source based on coherent smith-purcell radiation generated by femtosecond electron bunches in super-radiant regime
- Author
-
Leonid Sukhikh, Potylitsyn, A. P., Artyomov, K. P., Aryshev, A. S., Urakawa, J., and Karataev, P. V.
245. First steps towards a single-shot longitudinal profile monitor: Study of the properties of coherent smith-purcell radiation using the surface current model
- Author
-
Harrison, Hannah, Aryshev, Alexander, Doucas, George, Konoplev, Ivan, Lancaster, Andrew, Lekomtsev, Konstantin, Shevelev, Mikhail, Terunuma, Nobuhiro, and Urakawa, Junji
- Subjects
Physics::Accelerator Physics ,06 Beam Instrumentation, Controls, Feedback and Operational Aspects ,Accelerator Physics - Abstract
We propose to use the polarization of coherent Smith-Purcell radiation (cSPr) to separate the signal from background radiation in a single-shot longitudinal bunch profile monitor. We compare simulation and experimental results for the degree of polarization of cSPr generated by a grating with a 1mm periodic structure at the LUCX facility, KEK (Japan). Both experiment and simulation show that the majority of the cSPr signal is polarized in the direction parallel to the grating grooves. The degree of polarization predicted by simulation is higher than the measured result, therefore further investigation is needed to resolve this discrepancy., Proceedings of the 7th Int. Particle Accelerator Conf., IPAC2016, Busan, Korea more...
246. Transient radiation of the charged particles bunch
- Author
-
Alexander Aryshev and V.A. Nagorny
- Subjects
Physics ,Transition radiation ,Charge (physics) ,Cyclotron radiation ,Radiation ,Particle radiation ,Atomic physics ,Charged particle beam ,Charged particle ,Conductor - Abstract
The charged particle in crossing the medium boundaries generates the transient radiation. At present the properties of the transient radiation of the single point charge are well studied. Investigating the properties of the transient radiation of the charged particles bunch is of interest from the point of view of the practical usage. The given paper considers the transient radiation occurring when the charged particles bunch crosses the boundaries of the mediums vacuum-ideal conductor more...
247. The straightness monitor system at ATF2
- Author
-
Hildreth, Michael, Aryshev, Alexander, Boogert, Stewart, Honda, Yosuke, Tauchi, Toshiaki, Terunuma, Nobuhiro, and White, Glen
- Subjects
06 Beam Instrumentation and Feedback ,T03 Beam Diagnostics and Instrumentation ,Physics::Accelerator Physics ,Accelerator Physics - Abstract
The demonstration of the stability of the position of the focused beam is a primary goal of the ATF2 project. We have installed a laser interferometer system that will eventually correct the measurement of high-precision Beam Position Monitors used in the ATF2 Final Focus Steering Feedback for mechanical motion or vibrations. Here, we describe the installed system and present preliminary data on the short- and long-term mechanical stability of the BPM system., Proceedings of the 1st International Particle Accelerator Conference, IPAC2010, Kyoto, Japan more...
248. Design of an optical diffraction radiation beam size monitor at SLAC FFTB
- Author
-
G. A. Naumenko, Marc Ross, F. Zhou, J. Urakawa, Pavel Karataev, P. Bolton, T. Muto, M. Tobiyama, David B. Cline, A. P. Potylitsyn, Alexander Aryshev, Yasuo Fukui, and R. Hamatsu
- Subjects
Physics ,Beam diameter ,Ion beam ,business.industry ,Beam parameter product ,Optics ,Beamline ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,Beam expander ,Laser beam quality ,Particle beam ,business ,Beam (structure) - Abstract
We design a single bunch transverse beam size monitor which will be tested to measure the 28.5 GeV electron/positron beam at the SLAC FFTB beam line. The beam size monitor uses the CCD images of the interference pattern of the optical diffraction radiation from two slit edges which are placed close to the beam path. In this method, destruction of the accelerated electron/positron beam bunches due to the beam size monitoring is negligible, which is vital to the operation of the Linear Collider project. more...
249. Q-factor of an open resonator for a compact soft x-ray source based on thomson scattering of stimulated coherent diffraction radiation
- Author
-
Aryshev, A., Araki, S., Fukuda, M., Urakawa, J., Karataev, P., Naumenko, G., Potylitsyn, A., Leonid Sukhikh, Verigin, D., and Sakaue, K.
250. Diffraction radiation for non-invasive, high-resolution beam size measurements in future linear colliders
- Author
-
Bergamaschi, Michele, Aryshev, Alexander, Karataev, Pavel, Kieffer, Robert, Kruchinin, Konstantin, Lefèvre, Thibaut, Mazzoni, Stefano, and Terunuma, Nobuhiro
- Subjects
Physics::Instrumentation and Detectors ,06 Beam Instrumentation, Controls, Feedback and Operational Aspects ,Physics::Accelerator Physics ,Accelerators and Storage Rings ,Accelerator Physics - Abstract
Next generation linear colliders such as the Compact Linear Collider (CLIC) or the International Linear Collider (ILC) will accelerate particle beams with extremely small emittance. The high current and small size of the beam (micron-scale) due to such small emittance require non-invasive, high-resolution techniques for beam diagnostics. Diffraction Radiation (DR), a polarization radiation that appears when a charged particle moves in the vicinity of a medium, is an ideal candidate being non-invasive and allowing beams as small as a few tens of microns to be measured. Since DR is sensitive to beam parameters other than the transverse profile (e.g. its divergence and position), preparatory simulations have been performed with realistic beam parameters. A new dedicated instrument was installed in the KEK-ATF2 beam line in February 2016. At present DR is observed in the visible wavelength range, with an upgrade to the ultraviolet (200nm) planned for spring 2017 to optimize sensitivity to smaller beam sizes. Presented here are the latest results of these DR beam size measurements and simulations., Proceedings of the 8th Int. Particle Accelerator Conf., IPAC2017, Copenhagen, Denmark more...
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.