6,641 results on '"*NEUTRINO mass"'
Search Results
152. The minimal seesaw and leptogenesis models.
- Author
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Xing ZZ and Zhao ZH
- Abstract
Given its briefness and predictability, the minimal seesaw-a simplified version of the canonical seesaw mechanism with only two right-handed neutrino fields-has been studied in depth and from many perspectives, and now it is being pushed close to a position of directly facing experimental tests. This article is intended to provide an up-to-date review of various phenomenological aspects of the minimal seesaw and its associated leptogenesis mechanism in neutrino physics and cosmology. Our focus is on possible flavor structures of such benchmark seesaw and leptogenesis scenarios and confronting their predictions with current neutrino oscillation data and cosmological observations. In this connection particular attention will be paid to the topics of lepton number violation, lepton flavor violation, discrete flavor symmetries, CP violation and antimatter of the Universe., (© 2021 IOP Publishing Ltd.)
- Published
- 2021
- Full Text
- View/download PDF
153. The effective neutrino mass of neutrinoless double-beta decays: how possible to fall into a well
- Author
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Zhen-hua Zhao and Zhi-zhong Xing
- Subjects
Particle physics ,Physics and Astronomy (miscellaneous) ,High Energy Physics::Lattice ,FOS: Physical sciences ,lcsh:Astrophysics ,Threshold point ,01 natural sciences ,Neutrino Mass Matrix ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,Mathematics::Group Theory ,Effective mass (solid-state physics) ,High Energy Physics - Phenomenology (hep-ph) ,0103 physical sciences ,lcsh:QB460-466 ,Majorana Fermion ,lcsh:Nuclear and particle physics. Atomic energy. Radioactivity ,010306 general physics ,Neutrino oscillation ,Engineering (miscellaneous) ,Physics ,Mathematics::Functional Analysis ,010308 nuclear & particles physics ,High Energy Physics::Phenomenology ,Mathematics::History and Overview ,Threshold Point ,Graph ,Nonlinear Sciences::Chaotic Dynamics ,MAJORANA ,High Energy Physics - Phenomenology ,Decay Experiment ,lcsh:QC770-798 ,High Energy Physics::Experiment ,Neutrino ,Neutrino Mass - Abstract
If massive neutrinos are the Majorana particles and have a normal mass ordering, the effective mass term $\langle m\rangle^{}_{ee}$ of a neutrinoless double-beta ($0\nu 2\beta$) decay may suffer significant cancellations among its three components and thus sink into a decline, resulting in a "well" in the three-dimensional graph of $|\langle m\rangle^{}_{ee}|$ against the smallest neutrino mass $m^{}_1$ and the relevant Majorana phase $\rho$. We present a new and complete analytical understanding of the fine issues inside such a well, and discover a novel threshold of $|\langle m\rangle^{}_{ee}|$ in terms of the neutrino masses and flavor mixing angles: $|\langle m\rangle^{}_{ee}|^{}_* = m^{}_3 \sin^2\theta^{}_{13}$ in connection with $\tan\theta^{}_{12} = \sqrt{m^{}_1/m^{}_2}$ and $\rho =\pi$. This threshold point, which links the {\it local} minimum and maximum of $|\langle m\rangle^{}_{ee}|$, can be used to signify observability or sensitivity of the future $0\nu 2\beta$-decay experiments. Given current neutrino oscillation data, the possibility of $|\langle m\rangle^{}_{ee}| < |\langle m\rangle^{}_{ee}|^{}_*$ is found to be very small., Comment: 9 pages, 3 figures, version to appear in Eur. Phys. J. C
- Published
- 2017
154. Deconvolution of the energy loss function of the KATRIN experiment
- Author
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Volker Hannen, Ch. Weinheimer, Kathrin Valerius, I. Heese, and A. Sejersen Riis
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Work (thermodynamics) ,Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,FOS: Physical sciences ,Electron ,Deconvolution ,Inelastic scattering ,01 natural sciences ,Neutrino mass ,0103 physical sciences ,Electron scattering ,Nuclear Experiment (nucl-ex) ,010306 general physics ,Adiabatic process ,Nuclear Experiment ,KEV ELECTRONS ,Physics ,010308 nuclear & particles physics ,Astronomy and Astrophysics ,Instrumentation and Detectors (physics.ins-det) ,T-2 ,Atomic physics ,Neutrino ,KATRIN - Abstract
The KATRIN experiment aims at a direct and model independent determination of the neutrino mass with 0.2 eV/c^2 sensitivity (at 90% C.L.) via a measurement of the endpoint region of the tritium beta-decay spectrum. The main components of the experiment are a windowless gaseous tritium source (WGTS), differential and cryogenic pumping sections and a tandem of a pre- and a main-spectrometer, applying the concept of magnetic adiabatic collimation with an electrostatic retardation potential to analyze the energy of beta decay electrons and to guide electrons passing the filter onto a segmented silicon PIN detector. One of the important systematic uncertainties of such an experiment are due to energy losses of beta-decay electrons by elastic and inelastic scattering off tritium molecules within the source volume which alter the shape of the measured spectrum. To correct for these effects an independent measurement of the corresponding energy loss function is required. In this work we describe a deconvolution method to extract the energy loss function from measurements of the response function of the experiment at different column densities of the WGTS using a monoenergetic electron source., Comment: 18 pages, 8 figures, accepted for publication in Astroparticle Physics
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- 2017
155. Electroweak baryogenesis from a dark sector
- Author
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Kimmo Kainulainen, David Tucker-Smith, James M. Cline, and Helsinki Institute of Physics
- Subjects
Astrophysics and Astronomy ,Particle physics ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,standard model of particle physics ,Physics beyond the Standard Model ,STANDARD MODEL ,FOS: Physical sciences ,01 natural sciences ,7. Clean energy ,114 Physical sciences ,dark matter ,Higgs sector ,Standard Model ,pimeä aine ,High Energy Physics - Phenomenology (hep-ph) ,Baryon asymmetry ,0103 physical sciences ,SINGLET ,010306 general physics ,Particle Physics - Phenomenology ,Physics ,ta114 ,010308 nuclear & particles physics ,Electroweak interaction ,High Energy Physics::Phenomenology ,hiukkasfysiikan standardimalli ,RADIATIVE NEUTRINO MASS ,hep-ph ,Sphaleron ,Baryogenesis ,High Energy Physics - Phenomenology ,astro-ph.CO ,Higgs boson ,PHASE-TRANSITION ,High Energy Physics::Experiment ,MATTER ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Adding an extra singlet scalar $S$ to the Higgs sector can provide a barrier at tree level between a false vacuum with restored electroweak symmetry and the true one. This has been demonstrated to readily give a strong phase transition as required for electroweak baryogenesis. We show that with the addition of a fermionic dark matter particle $\chi$ coupling to $S$, a simple UV-complete model can realize successful electroweak baryogenesis. The dark matter gets a CP asymmetry that is transferred to the standard model through a $CP\ portal\ interaction$, which we take to be a coupling of $\chi$ to $\tau$ leptons and an inert Higgs doublet. The CP asymmetry induced in left-handed $\tau$ leptons biases sphalerons to produce the baryon asymmetry. The model has promising discovery potential at the LHC, while robustly providing a large enough baryon asymmetry and correct dark matter relic density with reasonable values of the couplings., Comment: 16 pages, 15 figures; v2: added references; v3: corrected eq.7, improved treatment of nucleation and wall velocity, added section on indirect detection; published version
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- 2017
156. Monitorování energetické stupnice v neutrinovém experimentu KATRIN
- Author
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Slezák, Martin, Vénos, Drahoslav, Štekl, Ivan, and Vorobel, Vít
- Subjects
krypton ,KATRIN ,hmotnost neutrin ,beta decay ,beta rozpad ,nuclear spectroscopy ,jaderná spektroskopie ,neutrino mass ,Physics::Instrumentation and Detectors ,Particle Physics - Experiment - Abstract
The question of the absolute mass scale of neutrinos is of particular interest for particle physics, astrophysics, and cosmology. The KATRIN experiment (KArlsruhe TRItium Neutrino experiment) aims to address the effective electron antineutrino mass from the shape of the tritium $\beta$-spectrum with an unprecedented sensitivity of 0.2 eV/c$^2$. One of the major systematic effects concerns the experimental energy scale, which has to be stable at the level of only a few parts in a million. For its calibration and monitoring the monoenergetic electrons emitted in the internal conversion of $\gamma$-transition of the metastable isotope $^{83\mathrm{m}}$Kr will be extensively applied. The aim of this thesis is to address the problem of KATRIN energy scale distortions and its monitoring in detail. The source of electrons based on $^{83\mathrm{m}}$Kr embedded in a solid as well as the source based on gaseous $^{83\mathrm{m}}$Kr are studied. Based on the experimental results an approach for the continuous stability monitoring is proposed.
- Published
- 2017
157. Electroweak breaking and neutrino mass
- Author
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Bonilla Díaz, César Manuel, Furtado Valle, José Wagner, Departament de Fisica Teòrica, and Valle, J.W.F.
- Subjects
Neutrino mass ,neutrino nature ,Higgs properties ,dark matter ,Flavour symmetries - Abstract
En este trabajo de tesis hemos analizado algunas de las posibles conexiones entre la generación de la masa de los neutrinos y la nueva física. Para ello, como preámbulo, en el primer capítulo hemos hecho un repaso del Modelo Estándar (SM) de la física de partículas, siendo ésta la descripción más precisa que tenemos de las las interacciones fuertes, débiles y electromagnéticas. Sin embargo, existen algunas interrogantes a las que el SM no ofrece respuesta, por ejemplo, ¿Por qué hay tres familias de quarks y leptones?, ¿Cuál es la explicación a la jerarquía de las masas de los fermiones y a sus ángulos de mezcla?, ¿Cómo explicar la jerarquía entre la escala electrodébil y la escala de Planck?, etc. Sin embargo, los problemas más importantes a los que el SM no ofrece una explicación son, 1) la masa de los neutrinos, 2) la materia oscura (DM), 3) la asimetría entre la materia bariónica y anti-bariónica en el universo (BAU). Dicho esto, resulta evidente la necesidad de ir más allá de la descripción estándar de la naturaleza, es decir, más allá del Modelo Estándar. Por lo tanto, esta tesis toma la física de neutrinos como el camino para resolver algunos de los problemas que, por construcción, el SM no ofrece una explicación. Por esta razón se han estudiado algunos de los mecanismos de generación de masa de los neutrinos y sus implicaciones. La física de neutrinos se ha transformado en un campo muy activo, tanto desde el punto de vista experimental como del teórico, desde la confirmación experimental de que los neutrinos cambian de sabor a lo largo de su viaje. Es decir, que los neutrinos oscilan y por lo tanto son partículas masivas. Además, experimentos como LEP han establecido que solamente hay tres especies de neutrinos activos. Por otro lado, de los ajustes globales de los parámetros de oscilación, los ángulos de mezcla y las diferencias cuadradas de las masas entre los neutrinos están muy bien determinados. Sin embargo, aun con toda la información que se tiene acerca de los los neutrinos y sus propiedades, existen algunos desafíos experimentales y teóricos. Por ejemplo, todavía no se ha podido determinar: i) el valor absoluto de la masa de los neutrinos; ii)¿cuál es la naturaleza de los neutrinos (si son partículas de Majorana o de Dirac)?; iii) la jerarquía de la masa de los neutrinos; iv) el valor de la fase de violación CP en el sector leptónico. Uno de los experimentos que podrían proporcionar alguna pista de algunas de estas incógnitas es el experimento KATRIN, el cual espera examinar hasta la escala absoluta de la masa de los neutrinos ~0.2 eV mediante el estudio del decaimiento β del tritium. Otros experimentos están dedicados a medir el decaimiento doble beta sin neutrinos 0νββ. La importancia de este tipos de experimentos está en que, en el caso de observar 0νββ, confirmaría que los neutrinos son partículas de Majorana y a su vez proporcionaría algún indicio sobre la jerarquía de las masas. El año pasado el experimento the KamLAND-Zen anunció sus resultados sobre 0νββ, pero ninguna señal ha sido observada. Lo único que obtuvimos de dicho experimentos es el límite más estricto para el decaimiento doble beta sin neutrinos, cuyas cotas están cerca de alcanzar la región característica donde la jerarquía de las masas es invertida. Del mismo modo, la colaboración de Planck (a partir de observaciones cosmológicas) ha puesto límites en la escala de la masa de los neutrinos y sus resultados desfavorecen fuertemente la posibilidad de que los neutrinos tengan un espectro de masa degenerado. Respecto a la fase de violación CP en el sector leptónico, el experimento T2K ha reportado un valor de la fase de Dirac cercana al valor 3π/2. Dicho resultado proviene de cierta tensión que hay entre los experimentos de reactor y los de aceleradores. Por lo tanto, el principal objetivo de otros experimentos como DUNE es el de medir la fase de violación de CP. Estos experimentos ponen de manifiesto el gran interés de la comunidad experimental en determinar algunas de las propiedades de los neutrinos. Desde el punto de vista teórico, el problema más interesante y que representa uno de los misterios más grandes de la física de partículas es el que respecta al origen de la masa de los neutrinos, el cual experimentalmente también resulta ser un gran reto. Por lo tanto, en el trabajo de tesis hemos descrito en qué consiste y cuáles son los ingredientes necesarios para generar la masa de los neutrinos por medio de los mecanismos de seesaw. Una vez que sabemos cómo generar la masa de los neutrinos, inmediatamente, nos damos cuenta de que el hecho de que los neutrinos sean partículas con una masa tan pequeña, del orden de 0.1 eV, es necesario la existencia de nueva física. En particular, se requiere que existan nuevos grados de libertad o partículas, las cuales actúan como mediadores entre la escala de la nueva física y la escala electrodébil, 246 GeV. El hecho que la masa de los neutrinos sea tan pequeña, comparada con el resto de las partículas de Modelo Estándar, puede deberse a que las nuevas partículas sean muy masivas. Si es el caso, la masa de los mediadores puede ser tan grande como la escala de gran unificación, por lo cual, probar su existencia resulta imposible para los experimentos actuales. La otra posibilidad de explicar la pequeñez de la masa de los neutrinos es que los parámetros de interacción necesarios para generar su masa sean extremadamente pequeños. De esta manera resulta que la masa de los mediadores podría estar a una escala cercana a la escala del rompimiento de la simetría electrodébil. Sin embargo, en el caso que los parámetros pequeños sean aquellos de las interacciones de Yukawa, los posibles procesos donde se podría observar el impacto de dichos mediadores tienden a ser muy pequeños. Esta situación ocurre, por ejemplo, con los procesos de violación de sabor leptónico que involucran a los leptones cargados como μ→eγ. Por lo tanto, la posibilidad más interesante, la cual hemos estudiado, reside en los escenarios donde el parámetro ``naturalmente'' pequeño se encuentra en el sector escalar. A dichos mecanismos los conocemos como mecanismos seesaw de energía baja. Los cuales se caracterizan no sólo de tener una predicción para los procesos de violación de sabor leptónico sino también en que experimentos tales como el LHC podrían producir las nuevas partículas (ligeras) involucradas en la generación de la masa de los neutrinos. Las características que hemos mencionado nos ayudan a hacer distinción entre la variedad de mecanismos de seesaw que existen. A nivel árbol existen solo tres tipos de seesaw: - Seesaw tipo I, en este caso el SM se extiende añadiendo neutrinos derechos (RH), los cuales son singletes bajo la simetría SU(2); - Seesaw tipo II, aquí el mediador es un escalar Δ que transforma como triplete bajo la simetría SU(2) y tiene número leptónico; - Seesaw tipo III, en este escenario se requiere la presencia de triplete fermiónico Σ. Esta clasificación es válida en el caso que los neutrinos sean partículas de Majorana. Sin embargo, no existe evidencia experimental que prohiba que los neutrinos sean partículas de Dirac. En este caso no sólo es necesario la introducción de nuevas partículas al SM si no también la existencia de una simetría G que no permita la aparición de términos de Majorana a ningún orden. La predicción más relevante de los neutrinos de Dirac es la ausencia del decaimiento doble beta sin neutrinos. Sin embargo otro tipo te conexiones y predicciones son posibles. Por ejemplo, la simetría G podría estar relacionada a un grupo de simetría de sabor, de tal modo que es posible explicar porqué existen tres generaciones de leptones y de quarks,sus masas y los valores de los parámetros de mezcla en ambos sectores.
- Published
- 2017
158. Why PeV scale left-right symmetry is a good thing
- Author
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Urjit A. Yajnik
- Subjects
FOS: Physical sciences ,General Physics and Astronomy ,Parameter space ,01 natural sciences ,Number Violation ,Theoretical physics ,High Energy Physics - Phenomenology (hep-ph) ,0103 physical sciences ,Electroweak Baryogenesis ,Spontaneous Violation ,Gauge theory ,010306 general physics ,Non-Conservation ,Boson ,Physics ,Conservation law ,Baryon Asymmetry ,Left-Right Symmetry ,010308 nuclear & particles physics ,High Energy Physics::Phenomenology ,Left-Right Model ,Lepton Number ,R-Parity ,Supersymmetry ,Domain Walls ,High Energy Physics - Phenomenology ,Metastable Vacua ,Leptogenesis ,Higgs boson ,Neutrino ,Neutrino Mass - Abstract
Left-right symmetric gauge theory presents a minimal paradigm to accommodate massive neutrinos with all known conserved symmetries duly gauged. The work presented here is based on the argument that the see-saw mechanism does not force the new right handed symmetry scale to be very high, and as such some of the species from the spectrum of the new gauge and Higgs bosons can have masses within a few orders of magnitude of the TeV scale. The scale of the left-right parity breaking in turn can be sequestered from the Planck scale by supersymmetry. We have studied several formulations of such Just Beyond Standard Model (JBSM) theories for their consistency with cosmology. Specifically the need to eliminate phenomenologically undesirable domain walls gives many useful clues. The possibility that the exact left-right symmetry breaks in conjunction with supersymmetry has been explored in the context of gauge mediation, placing restrictions on the available parameter space. Finally we have also studied a left-right symmetric model in the context of metastable supersymmetric vacua and obtained constraints on the mass scale of Right handed symmetry. In all the cases studied, The mass scale of right handed neutrino $M_R$ remains bounded from above, and in some of the cases the scale $10^9$ GeV favourable for supersymmetric thermal leptogenesis is disallowed. On the other hand PeV scale remains a viable option, and the results warrant a more detailed study of such models for their observability in collider and astroparticle experiments., Comment: 18 pages. Presented at \textsl{Pheno1} First Workshop on Beyond Standard Model Physics, IISER Mohali April 2016 and at the program Exploring the Energy Ladder of the Universe at Mainz Institute for Theoretical Physics June 2016. To appear in proceedings. arXiv admin note: substantial text overlap with arXiv:1401.8063
- Published
- 2017
159. Majorana neutrinos in an effective lagrangian approach
- Author
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Duarte, Lucía, Sampayo, Oscar Alfredo, and González Sprinberg, Gabriel
- Subjects
NEUTRINOS ,ELEMENTARY PARTICLES ,GAUGE FIELD THEORY ,NEUTRINO MASS - Published
- 2017
160. Search for Evidence of the Type-III Seesaw Mechanism in Multilepton Final States in Proton-Proton Collisions at s =13 TeV
- Author
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CMS Collaboration, Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Erö, J., Flechl, M., Friedl, M., Frühwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., König, A., Krammer, N., Krätschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rabady, D., Rad, N., Rohringer, H., Schieck, J., Schöfbeck, R., Spanring, M., Spitzbart, D., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Suarez Gonzalez, J., De Wolf, E. A., Di Croce, D., Janssen, X., Lauwers, J., Van Haevermaet, H., Van Mechelen, P., Van Remortel, N., Abu Zeid, S., Blekman, F., D’Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Van Doninck, W., Van Mulders, P., Van Parijs, I., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Karapostoli, G., Lenzi, T., Luetic, J., Maerschalk, T., Marinov, A., Randle-conde, A., Seva, T., Vander Velde, C., Vanlaer, P., Vannerom, D., Yonamine, R., Zenoni, F., Zhang, F., Cimmino, A., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Salva, S., Tytgat, M., Verbeke, W., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caudron, A., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Jafari, A., Komm, M., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Vidal Marono, M., Wertz, S., Beliy, N., Aldá Júnior, W. L., Alves, F. L., Alves, G. A., Brito, L., Correa Martins Junior, M., Hensel, C., Moraes, A., Pol, M. E., Rebello Teles, P., Belchior Batista Das Chagas, E., Carvalho, W., Chinellato, J., Custódio, A., Da Costa, E. M., Da Silveira, G. G., De Jesus Damiao, D., Fonseca De Souza, S., Huertas Guativa, L. M., Malbouisson, H., Melo De Almeida, M., Mora Herrera, C., Mundim, L., Nogima, H., Santoro, A., Sznajder, A., Tonelli Manganote, E. J., Torres Da Silva De Araujo, F., Vilela Pereira, A., Ahuja, S., Bernardes, C. A., Tomei, T. R. Fernandez Perez, Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Romero Abad, D., Ruiz Vargas, J. C., Aleksandrov, A., Hadjiiska, R., Iaydjiev, P., Misheva, M., Rodozov, M., Shopova, M., Stoykova, S., Sultanov, G., Dimitrov, A., Glushkov, I., Litov, L., Pavlov, B., Petkov, P., Fang, W., Gao, X., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhao, J., Ban, Y., Chen, G., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Avila, C., Cabrera, A., Chaparro Sierra, L. F., Florez, C., González Hernández, C. F., Ruiz Alvarez, J. D., Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Ribeiro Cipriano, P. M., Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Finger, M., Carrera Jarrin, E., El-khateeb, E., Elgammal, S., Ellithi Kamel, A., Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Tiko, A., Veelken, C., Eerola, P., Pekkanen, J., Voutilainen, M., Härkönen, J., Järvinen, T., Karimäki, V., Kinnunen, R., Lampén, T., Lassila-Perini, K., Lehti, S., Lindén, T., Luukka, P., Tuominen, E., Tuominiemi, J., Tuovinen, E., Talvitie, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Ghosh, S., Givernaud, A., Gras, P., Hamel de Monchenault, G., Jarry, P., Kucher, I., Locci, E., Machet, M., Malcles, J., Negro, G., Rander, J., Rosowsky, A., Sahin, M. Ö., Titov, M., Abdulsalam, A., Antropov, I., Baffioni, S., Beaudette, F., Busson, P., Cadamuro, L., Charlot, C., Granier de Cassagnac, R., Jo, M., Lisniak, S., Lobanov, A., Martin Blanco, J., Nguyen, M., Ochando, C., Ortona, G., Paganini, P., Pigard, P., Regnard, S., Salerno, R., Sauvan, J. B., Sirois, Y., Stahl Leiton, A. G., Strebler, T., Yilmaz, Y., Zabi, A., Zghiche, A., Agram, J.-L., Andrea, J., Bloch, D., Brom, J.-M., Buttignol, M., Chabert, E. C., Chanon, N., Collard, C., Conte, E., Coubez, X., Fontaine, J.-C., Gelé, D., Goerlach, U., Jansová, M., Le Bihan, A.-C., Tonon, N., Van Hove, P., Gadrat, S., Beauceron, S., Bernet, C., Boudoul, G., Chierici, R., Contardo, D., Depasse, P., El Mamouni, H., Fay, J., Finco, L., Gascon, S., Gouzevitch, M., Grenier, G., Ille, B., Lagarde, F., Laktineh, I. B., Lethuillier, M., Mirabito, L., Pequegnot, A. L., Perries, S., Popov, A., Sordini, V., Vander Donckt, M., Viret, S., Toriashvili, T., Lomidze, D., Autermann, C., Beranek, S., Feld, L., Kiesel, M. K., Klein, K., Lipinski, M., Preuten, M., Schomakers, C., Schulz, J., Verlage, T., Albert, A., Dietz-Laursonn, E., Duchardt, D., Endres, M., Erdmann, M., Erdweg, S., Esch, T., Fischer, R., Güth, A., Hamer, M., Hebbeker, T., Heidemann, C., Hoepfner, K., Knutzen, S., Merschmeyer, M., Meyer, A., Millet, P., Mukherjee, S., Olschewski, M., Padeken, K., Pook, T., Radziej, M., Reithler, H., Rieger, M., Scheuch, F., Teyssier, D., Thüer, S., Flügge, G., Kargoll, B., Kress, T., Künsken, A., Lingemann, J., Müller, T., Nehrkorn, A., Nowack, A., Pistone, C., Pooth, O., Stahl, A., Aldaya Martin, M., Arndt, T., Asawatangtrakuldee, C., Beernaert, K., Behnke, O., Behrens, U., Bermúdez Martínez, A., Bin Anuar, A. A., Borras, K., Botta, V., Campbell, A., Connor, P., Contreras-Campana, C., Costanza, F., Diez Pardos, C., Eckerlin, G., Eckstein, D., Eichhorn, T., Eren, E., Gallo, E., Garay Garcia, J., Geiser, A., Gizhko, A., Grados Luyando, J. 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M., Evans, A., Hansen, P., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Gonzalez Suarez, R., Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Alyari, M., Dolen, J., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Hortiangtham, A., Massironi, A., Morse, D. M., Nash, D., Orimoto, T., Teixeira De Lima, R., Trocino, D., Wood, D., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Pollack, B., Schmitt, M. H., Sung, K., Trovato, M., Velasco, M., Dev, N., Hildreth, M., Hurtado Anampa, K., Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Smith, G., Taroni, S., Wayne, M., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Liu, B., Luo, W., Puigh, D., Winer, B. L., Wulsin, H. W., Benaglia, A., Cooperstein, S., Driga, O., Elmer, P., Hardenbrook, J., Hebda, P., Higginbotham, S., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Pirouã©, P., Stickland, D., Tully, C., Norberg, S., Barker, A., Barnes, V. E., Das, S., Folgueras, S., Gutay, L., Jha, M. K., Jones, M., Jung, A. W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Schulte, J. F., Sun, J., Wang, F., Xie, W., Cheng, T., Parashar, N., Stupak, J., Adair, A., Akgun, B., Chen, Z., Ecklund, K. M., Geurts, F. J. M., Guilbaud, M., Li, W., Michlin, B., Northup, M., Padley, B. P., Roberts, J., Rorie, J., Tu, Z., Zabel, J., Bodek, A., De Barbaro, P., Demina, R., Duh, Y. T., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, P., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Christos, M., Feigelis, K., Gershtein, Y., Gómez Espinosa, T. A., Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Kunnawalkam Elayavalli, R., Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Zhou, B., Delannoy, A. G., Foerster, M., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Castaneda Hernandez, A., Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Perniã, L., Rathjens, D., Safonov, A., Tatarinov, A., Ulmer, K. A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Libeiro, T., Peltola, T., Undleeb, S., Volobouev, I., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Sheldon, P., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, P., Cox, B., Hirosky, R., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Sun, X., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Sturdy, J., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Hervã©, A., Hussain, U., Klabbers, P., Lanaro, A., Levine, A., Long, K., Loveless, R., Pierro, G. A., Polese, G., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Taylor, D., Woods, N., Yerevan Physics Institute, Institut für Hochenergiephysik, Institute for Nuclear Problems, Universiteit Antwerpen, Vrije Universiteit Brussel, Université Libre de Bruxelles, Ghent University, Université Catholique de Louvain, Université de Mons, Centro Brasileiro de Pesquisas Fisicas, Universidade do Estado do Rio de Janeiro (UERJ), Universidade Estadual Paulista (UNESP), Universidade Federal do ABC (UFABC), Bulgaria Academy of Sciences, University of Sofia, Beihang University, Institute of High Energy Physics, Peking University, Universidad de Los Andes, Mechanical Engineering and Naval Architecture, Faculty of Science, Institute Rudjer Boskovic, University of Cyprus, Charles University, Universidad San Francisco de Quito, Egyptian Network of High Energy Physics, National Institute of Chemical Physics and Biophysics, University of Helsinki, Helsinki Institute of Physics, Lappeenranta University of Technology, Université Paris-Saclay, IPHC UMR 7178, CNRS/IN2P3, Institut de Physique Nucléaire de Lyon, Georgian Technical University, Tbilisi State University, I. Physikalisches Institut, III. Physikalisches Institut A, III. Physikalisches Institut B, Deutsches Elektronen-Synchrotron, University of Hamburg, Institut für Experimentelle Kernphysik, NCSR Demokritos, National and Kapodistrian University of Athens, University of Ioánnina, Eötvös Loránd University, Wigner Research Centre for Physics, Institute of Nuclear Research ATOMKI, University of Debrecen, Indian Institute of Science (IISc), National Institute of Science Education and Research, Panjab University, University of Delhi, HBNI, Indian Institute of Technology Madras, Bhabha Atomic Research Centre, Tata Institute of Fundamental Research-A, Tata Institute of Fundamental Research-B, Indian Institute of Science Education and Research (IISER), Institute for Research in Fundamental Sciences (IPM), University College Dublin, Politecnico di Bari, INFN Sezione di Bari, Università di Bari, Università di Bologna, INFN Sezione di Bologna, Università di Catania, INFN Sezione di Catania, Università di Firenze, INFN Sezione di Firenze, INFN Laboratori Nazionali di Frascati, Università di Genova, INFN Sezione di Genova, INFN Sezione di Milano-Bicocca, Università di Milano-Bicocca, Università di Napoli 'Federico II', INFN Sezione di Napoli, Università della Basilicata, Università G. Marconi, Università di Padova, INFN Sezione di Padova, Università di Trento, Università di Pavia, INFN Sezione di Pavia, Università di Perugia, INFN Sezione di Perugia, Scuola Normale Superiore di Pisa, INFN Sezione di Pisa, Università di Pisa, INFN Sezione di Roma, Sapienza Università di Roma, Università di Torino, INFN Sezione di Torino, Università Del Piemonte Orientale, Università di Trieste, INFN Sezione di Trieste, Kyungpook National University, Chonbuk National University, Institute for Universe and Elementary Particles, Hanyang University, Korea University, Seoul National University, University of Seoul, Sungkyunkwan University, Vilnius University, Universiti Malaya, Centro de Investigacion y de Estudios Avanzados Del IPN, Universidad Iberoamericana, Benemerita Universidad Autonoma de Puebla, Universidad Autónoma de San Luis Potosí, University of Auckland, University of Canterbury, Quaid-I-Azam University, National Centre for Nuclear Research, University of Warsaw, Laboratório de Instrumentação e Física Experimental de Partículas, Joint Institute for Nuclear Research, Petersburg Nuclear Physics Institute, Institute for Nuclear Research, Institute for Theoretical and Experimental Physics, Moscow Institute of Physics and Technology, Moscow Engineering Physics Institute (MEPhI), P.N. Lebedev Physical Institute, Lomonosov Moscow State University, Novosibirsk State University (NSU), Institute for High Energy Physics, Vinca Institute of Nuclear Sciences, Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Universidad Autónoma de Madrid, Universidad de Oviedo, CSIC-Universidad de Cantabria, European Organization for Nuclear Research, Paul Scherrer Institut, ETH Zurich, Universität Zürich, National Central University, National Taiwan University (NTU), Science and Art Faculty, Physics Department, Bogazici University, Istanbul Technical University, National Academy of Science of Ukraine, Kharkov Institute of Physics and Technology, University of Bristol, Rutherford Appleton Laboratory, Imperial College, Brunel University, Baylor University, Catholic University of America, University of Alabama, Boston University, Brown University, Davis, University of California, Riverside, San Diego, Santa Barbara, California Institute of Technology, Carnegie Mellon University, University of Colorado Boulder, Cornell University, Fermi National Accelerator Laboratory, University of Florida, Florida International University, Florida State University, Florida Institute of Technology, University of Illinois at Chicago (UIC), University of Iowa, Johns Hopkins University, University of Kansas, Kansas State University, Lawrence Livermore National Laboratory, University of Maryland, Massachusetts Institute of Technology, University of Minnesota, University of Mississippi, University of Nebraska-Lincoln, State University of New York at Buffalo, Northeastern University, Northwestern University, University of Notre Dame, Ohio State University, Princeton University, University of Puerto Rico, Purdue University, Purdue University Northwest, Rice University, University of Rochester, Rockefeller University, State University of New Jersey, University of Tennessee, Texas A and M University, Texas Tech University, Vanderbilt University, University of Virginia, Wayne State University, University of Wisconsin - Madison, Texas A and M University at Qatar, Vienna University of Technology, Universidade Estadual de Campinas (UNICAMP), Universidade Federal de Pelotas, Ain Shams University, British University in Egypt, Cairo University, Université de Haute Alsace, Brandenburg University of Technology, IIT Bhubaneswar, Institute of Physics, University of Visva-Bharati, University of Ruhuna, Isfahan University of Technology, Yazd University, Islamic Azad University, Università degli Studi di Siena, International Islamic University of Malaysia, MOSTI, Consejo Nacional de Ciencia y Tecnología, Institute of Electronic Systems, Czech Technical University, St. Petersburg State Polytechnical University, Budker Institute of Nuclear Physics, University of Belgrade, Scuola Normale e Sezione dell'Infn, Riga Technical University, Stefan Meyer Institute for Subatomic Physics, Adiyaman University, Istanbul Aydin University, Mersin University, Cag University, Piri Reis University, Izmir Institute of Technology, Necmettin Erbakan University, Marmara University, Kafkas University, Istanbul Bilgi University, University of Southampton, Instituto de Astrofísica de Canarias, Utah Valley University, Beykent University, Bingol University, Erzincan University, Sinop University, and Istanbul
- Subjects
NEUTRINO MASS ,VIOLATION ,SIGNALS ,NUMBER ,MODELS ,LHC ,CMS ,hep-ex ,Physics ,Settore FIS/01 - Fisica Sperimentale ,High Energy Physics::Phenomenology ,FOS: Physical sciences ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,Physics and Astronomy (all) ,Physics and Astronomy ,Multilepton ,ddc:530 ,High Energy Physics::Experiment ,Particle Physics - Experiment - Abstract
A search for a signal consistent with the type-III seesaw mechanism in events with three or more electrons or muons is presented. The data sample consists of proton-proton collisions at sqrt(s) = 13 TeV collected by the CMS experiment at the LHC in 2016 and corresponds to an integrated luminosity of 35.9 inverse femtobarns. Selection criteria based on the number of leptons and the invariant mass of opposite-sign lepton pairs are used to distinguish the signal from the standard model background. The observations are consistent with the expectations from standard model processes. The results are used to place limits on the production of heavy fermions of the type-III seesaw model as a function of the branching ratio to each lepton flavor. In the scenario of equal branching fractions to each lepton flavor, heavy fermions with masses below 840 GeV are excluded. This is the most sensitive probe to date of the type-III seesaw mechanism., Replaced with the published version. All the figures and tables, including additional supplementary figures and tables, can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/EXO-17-006 (CMS Public Pages)
- Published
- 2017
- Full Text
- View/download PDF
161. Development of Liquid Scintillator containing a Zirconium Complex for Neutrinoless Double Beta Decay Experiment
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Fukuda, Yoshiyuki, Narengerile, OBATA, Akira, MORIYAMA, Shigetaka, and OGAWA, Izumi
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ニュートリノ質量 ,ニュートリノを放出しない2重ベータ崩壊 ,液体シンチレータ ,ジルコニウム ,Metal Complex ,Zirconium ,Neutrino Mass ,Neutrinoless Double Beta Decay ,金属錯体 ,Liquid Scintillator - Abstract
An organic liquid scintillator containing a zirconium complex has been developed for a new neutrinoless double beta decay experiment. In order to produce a detector that has good energy resolution (4% at 2.5 MeV) and low background (0.1 counts/(tonne・year) and that can monitor tonnes of target isotope, we chose a zirconium β-diketone complex having high solubility (over 10 wt.%) in anisole. However, the absorption peak of the diketone ligand overlaps with the luminescence of anisole. Therefore, the light yield of the liquid scintillator decreases in proportion to the concentration of the complex. To avoid this problem, we synthesized a β-keto ester complex introducing -OC3H7 or -OC2H5 substituent groups in the β-diketone ligand, and a diethyl malonate complex. Those shifted the absorption peak to around 245nm and 210nm, respectively, which are shorter than the emission peak of anisole (275nm). However, the shift of the absorption peak depends on the the scintillation solvent. Therefore we have to choose an adequate solvent for the liquid scintillator. The best performance will be obtained by pure anisole scintillator containing a tetrakis diethyl malonate zirconium. We also synthesized a Zr-ODZ complex, which has a high quantum yield (30%) and good emission wavelength (425nm) with a solubility 5 wt.% in benzonitrile. However, the absorption peak of the Zr-ODZ complex was around 240 nm. Therefore, it is better to use the scintillation solvent which has shorter luminescence wavelength than that of benzonitrile.
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- 2014
162. Double-β decay studies with JYFLTRAP
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Kolhinen, V. S., Rahaman, S., and Suhonen, J.
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- 2014
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163. Theory of neutrinoless double beta decay—A brief review
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Šimkovic, Fedor
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- 2013
- Full Text
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164. The extended Baryon Oscillation Spectroscopic Survey: a cosmological forecast
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Gong-Bo Zhao, Sarah Shandera, Donald P. Schneider, Francisco Prada, Jean-Paul Kneib, Yuting Wang, Timothée Delubac, Christophe Yèche, Xu Zhou, Kyle S. Dawson, H. Y. Zhang, Andres Meza, Dandan Wang, Nathalie Palanque-Delabrouille, Graziano Rossi, Ashley J. Ross, Alireza Hojjati, Hee-Jong Seo, Yuecheng Zhang, Levon Pogosian, Cameron K. McBride, Hu Zou, Adam D. Myers, Johan Comparat, Kazuya Koyama, Pengyuan Gao, Will J. Percival, Charling Tao, Jeffrey A. Newman, Fangzhou Zhu, Joel R. Brownstein, Key Laboratory for Liquid-Solid Structural Evolution and Processing of Materials, Shandong University, Department of Electrical and Computer Engineering [Minneapolis] (ECE), University of Minnesota [Twin Cities] (UMN), University of Minnesota System-University of Minnesota System, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Departamento de FisicaTeorica e IFT-UAM/CSIC, Universidad Autónoma de Madrid (UAM), EPFL Laboratoire d’astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), Institute of Cosmology & Gravitation, Dennis Sciama Building, University of Portsmouth, Department of Physics and Astronomy [Pittsburgh], University of Pittsburgh (PITT), Pennsylvania Commonwealth System of Higher Education (PCSHE)-Pennsylvania Commonwealth System of Higher Education (PCSHE), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, 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), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), and Universidad Autonoma de Madrid (UAM)
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Cosmology and Gravitation ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,FOS: Physical sciences ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,NEUTRINO MASS ,01 natural sciences ,ACOUSTIC-OSCILLATIONS ,symbols.namesake ,ST/K00090/1 ,0103 physical sciences ,Planck ,dark energy ,010303 astronomy & astrophysics ,Weak gravitational lensing ,STFC ,Astrophysics::Galaxy Astrophysics ,Physics ,010308 nuclear & particles physics ,Oscillation ,RCUK ,CONSTRAINTS ,Astronomy and Astrophysics ,Quasar ,FOREST ,Galaxy ,Baryon ,large scale structure of Universe ,GALAXIES ,QUASARS ,DATA SETS ,Space and Planetary Science ,SDSS-III ,NON-GAUSSIANITY ,symbols ,Dark energy ,astro-ph.CO ,DIGITAL SKY SURVEY ,DARK ENERGY ,large-scale structure of Universe ,Neutrino ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a science forecast for the eBOSS survey, part of the SDSS-IV project, which is a spectroscopic survey using multiple tracers of large-scale structure, including luminous red galaxies (LRGs), emission line galaxies (ELGs) and quasars (both as a direct probe of structure and through the Ly-$\alpha$ forest). Focusing on discrete tracers, we forecast the expected accuracy of the baryonic acoustic oscillation (BAO), the redshift-space distortion (RSD) measurements, the $f_{\rm NL}$ parameter quantifying the primordial non-Gaussianity, the dark energy and modified gravity parameters. We also use the line-of-sight clustering in the Ly-$\alpha$ forest to constrain the total neutrino mass. We find that eBOSS LRGs ($0.60.6$), ELGs ($0.6, Comment: 15 pages, 9 figures, 6 tables; matches the published version on MNRAS
- Published
- 2016
165. Transition-Edge Sensor Arrays of Microcalorimeters with163Ho for Direct Neutrino Mass Measurements with HOLMES
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Orlando, A., Biasotti, M., Ceriale, V., De Gerone, M., Gatti, F., Hays-Wehle, J., Pizzigoni, G., Schmidt, D., Swetz, D., and Ullom, J.
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Arrays ,Microcalorimeters ,Neutrino mass ,TES ,Atomic and Molecular Physics, and Optics ,Materials Science (all) ,Condensed Matter Physics ,Atomic and Molecular Physics ,and Optics - Published
- 2016
166. Neutrinoless ββ decays to excited 0+ states and the Majorana-neutrino mass
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Hyvärinen, Juhani and Suhonen, Jouni
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Nuclear Theory ,Majorana-neutrino mass ,nuclear matrix elements ,fysiikka ,Nuclear Experiment - Abstract
The nuclear matrix elements (NMEs) corresponding to the neutrinoless double-β (0νββ) decays to excited 0+ states of major experimental interest are calculated. All these decay transitions are electron emitting (0νβ−β− decays) and take place in the mass A = 76,82,96,100,110,116,124,130,136 nuclei. This work is an extension of our previous work [Phys. Rev. C 91, 024613 (2015)], where 0νββ decays to the ground states of the same nuclei were treated. We calculate the NMEs for transitions mediated by both the light (l-NMEs) and the heavy (h-NMEs) Majorana neutrinos. A higher-QRPA (quasiparticle random-phase approximation) framework, the multiple-commutator model, is adopted for the calculations, including a previously omitted contribution to the transitions to two-phonon states. A Bonn G-matrix-based effective nucleon-nucleon interaction is generated by exploiting the recently proposed isoscalar-isovector decomposition of the particle-particle proton-neutron interaction parameter, gpp. All the appropriate short-range correlations, nucleon form factors, and higher-order nucleonic weak currents are included to benchmark our calculations. The relevant nuclear spectroscopy was checked to validate the nuclear models used. The computed l-NMEs and h-NMEs are compared with the available other calculations and the relevance of the new included two-phonon term is discussed. The results are summarized by easy-to-use half-life-Majorana-mass interrelations. peerReviewed
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- 2016
167. Status of the HOLMES detector development
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Michele Biasotti, C. Brofferio, Joseph W. Fowler, Gene C. Hilton, Rugard Dressler, U. Koester, M. De Gerone, G. Pizzigoni, Peter Day, Emanuele Ferri, R. Nizzolo, Daniel Schmidt, D. Corsini, L. Parodi, Elisa Fumagalli, M. Lusignoli, V. Ceriale, John A. B. Mates, Stefano Nisi, Monica Sisti, M. Ribeiro-Gomes, James P. Hays-Wehle, Carl D. Reintsema, A. Nucciotti, Daniel S. Swetz, M. Faverzani, Leila R. Vale, S. Ragazzi, G. Pessina, Joel N. Ullom, Angelo Orlando, F. Siccardi, D. A. Bennett, Johnathon D. Gard, Flavio Gatti, Dorothea Schumann, G. Ceruti, A. Puiu, Andrea Giachero, Daniel T. Becker, M. Maino, F. Terranova, S. Heinitz, Bradley K. Alpert, Nucciotti, A, Alpert, B, Becker, D, Bennett, D, Biasotti, M, Brofferio, C, Ceriale, V, Ceruti, G, Corsini, D, Day, P, De Gerone, M, Dressler, R, Faverzani, M, Ferri, E, Fowler, J, Fumagalli, E, Gard, J, Gatti, F, Giachero, A, Hays Wehle, J, Heinitz, S, Hilton, G, Koester, U, Lusignoli, M, Maino, M, Mates, J, Nisi, S, Nizzolo, R, Orlando, A, Parodi, L, Pessina, G, Pizzigoni, G, Puiu, P, Ragazzi, S, Reintsema, C, Ribeiro Gomes, M, Schmidt, D, Schumann, D, Siccardi, F, Sisti, M, Swetz, D, Terranova, F, Ullom, J, and Vale, L
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010302 applied physics ,Physics ,Nuclear and High Energy Physics ,Electron capture ,Instrumentation ,Detector ,Resolution (electron density) ,Ho-163 ,Low temperature detectors ,Neutrino mass ,02 engineering and technology ,021001 nanoscience & nanotechnology ,01 natural sciences ,Nuclear physics ,Full width at half maximum ,Low temperature detector ,0103 physical sciences ,Neutrino ,0210 nano-technology ,Neutrino ma ,Sensitivity (electronics) ,Energy (signal processing) - Abstract
HOLMES is a new experiment to directly measure the neutrino mass with a sensitivity as low as 0.4 eV. HOLMES will perform a calorimetric measurement of the energy released in the electron capture decay of 163 Ho. HOLMES will deploy a large array of low temperature microcalorimeters with implanted 163 Ho nuclei. HOLMES baseline detector is an array of 1000 microcalorimeters each with an implanted 163 Ho activity of about 300 Bq, an energy resolution FWHM of about 1 eV at the spectrum end-point ( Q ≈ 2.5 keV), and a time resolution of about 1 μs. Matching these performances requires a careful optimization of all components, from the microcalorimeters to the signal processing algorithms. We outline here the project technical challenges and the present status of the development.
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- 2016
168. Radiative neutrino models in light of diphoton signals
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Antipin, Oleg, Culjak, Petar, Krešimir Kumerički, and Picek, Ivica
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750 GeV resonance ,neutrino mass ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,High Energy Physics::Phenomenology ,FOS: Physical sciences ,High Energy Physics::Experiment - Abstract
Viable explanations of a hinted 750 GeV scalar resonance may be sought within the extensions of the SM Higgs sector aimed at generating neutrino masses at the loop level. We confront a compatibility with the 750 GeV diphoton excess for two recent models which do not need to impose ad hoc symmetry to forbid the tree-level masses: a one-loop mass model providing the H(750) candidate within its real triplet scalar representation and a three-loop mass model providing it within its two Higgs doublets. Besides accounting for the 750 GeV resonance, we demonstrate that these complementary neutrino-mass scenarios have different testable predictions for the LHC which should show up soon as more data is accumulated during the ongoing 13 TeV run., 23 pages, 5 figures, new section and refs added; to stay unpublished since diphoton signal disappeared
- Published
- 2016
169. Neutrinoless ββ decays to excited 0+ states and the Majorana-neutrino mass
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ta114 ,Majorana-neutrino mass ,nuclear matrix elements ,physics - Published
- 2016
170. Cosmological constraints: anisotropic dark energy, the Hubble constant, and the neutrino mass
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Cardona Castro, Wilmar and Kunz, Martin
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Forecasts ,Galaxy surveys ,Statistical methods ,Bayesian methods ,Non-Gaussianity ,Relativistic effects ,Cosmological constraints ,ddc:500.2 ,CMB ,Cepheid stars ,Neutrino mass ,Supernovae ,Hubble parameter ,Dark energy ,Number counts ,Statistical isotropy - Abstract
Nous avons tout d'abord étudié les causes fondamentales de l'accélération de l'expansion de l'univers. Nous nous sommes interrogés sur les effets de la présence d'un stress méchanique anisotrope dans les perturbations de matière et d'énergie sombres, de même que dans les propriétés statistiques du fond cosmique des micro-ondes. Deuxièmement, nous avons estimé l'importance toute particulière de l'effet de lentille gravitationnelle lorsque l'on analyse les données d'un catalogue de galaxies tel que EUCLID. On a montré que négliger cet effet dans les contraintes cosmologiques de la masse de neutrinos fausserait les mesures de leur masse, empêchant ainsi une des résultats essentiels des futurs catalogues de galaxies. Troisièmement, nous avons développé une méthode statistique qui emploie des hyperparamètres Bayesiens afin de mesurer le paramètre Hubble avec les données disponibles. Cette approche permet un traitement compréhensif des ensembles de données disponibles sans l'utilisation d'algorithmes arbitraires pour le traitement de données aberrantes.
- Published
- 2016
171. Light sterile neutrinos
- Author
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Stefano Gariazzo, E. M. Zavanin, Carlo Giunti, Marco Laveder, and Yufeng Li
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Accelerator Physics (physics.acc-ph) ,Particle physics ,Sterile neutrino ,Nuclear and High Energy Physics ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Physics::Instrumentation and Detectors ,Physics beyond the Standard Model ,FOS: Physical sciences ,01 natural sciences ,neutrino mass ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,High Energy Physics - Phenomenology (hep-ph) ,sterile neutrinos ,0103 physical sciences ,Mass scale ,Statistical analysis ,010306 general physics ,Neutrino oscillation ,Physics ,Liquid Scintillator Neutrino Detector ,neutrino oscillations ,010308 nuclear & particles physics ,High Energy Physics::Phenomenology ,High Energy Physics - Phenomenology ,Physics - Accelerator Physics ,High Energy Physics::Experiment ,Phenomenology (particle physics) ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The theory and phenomenology of light sterile neutrinos at the eV mass scale is reviewed. The reactor, Gallium and LSND anomalies are briefly described and interpreted as indications of the existence of short-baseline oscillations which require the existence of light sterile neutrinos. The global fits of short-baseline oscillation data in 3+1 and 3+2 schemes are discussed, together with the implications for beta-decay and neutrinoless double-beta decay. The cosmological effects of light sterile neutrinos are briefly reviewed and the implications of existing cosmological data are discussed. The review concludes with a summary of future perspectives., Comment: 41 pages; final version to be published as a Topical Review in Journal of Physics G
- Published
- 2016
172. Status of the CUORE and results from the CUORE-0 neutrinoless double beta decay experiments
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M. M. Deninno, S. Di Domizio, C. Zarra, Lucia Canonica, B. K. Fujikawa, Stefano Pozzi, Stefano Dell'Oro, F. Bellini, X. Liu, Massimiliano Nastasi, L. Gironi, F. T. Avignone, A. Giuliani, T. I. Banks, N. Casali, S. Pirro, M. Vignati, A. Bersani, F. Orio, Massimiliano Clemenza, Carlo Cosmelli, C. Rosenfeld, M. Balata, G. Bari, Vladimir Datskov, L. Pattavina, G. Ventura, S. Trentalange, S. Copello, N. Moggi, C. Nones, Yu-Gang Ma, B. S. Wang, R. J. Creswick, P. Gorla, Samuele Sangiorgio, Stefano Nisi, O. Azzolini, Y. L. Li, Oliviero Cremonesi, Marisa Pedretti, A. Nucciotti, C. Brofferio, H. Z. Huang, F. Ferroni, C. Tomei, M. Tenconi, Emanuele Ferri, Ettore Fiorini, H. A. Farach, Andrea Giachero, M. Faverzani, Eugene E. Haller, G. Fernandes, L. Taffarello, Marco Pallavicini, Jeremy S. Cushman, W. D. Tian, Alan R. Smith, N. Chott, G. Pessina, M. L. Di Vacri, Davide Chiesa, K. E. Lim, Nicholas Scielzo, A. Camacho, S. Zucchelli, L. Carbone, C. Bucci, T. D. Gutierrez, Guimin Zhang, Jeffrey W. Beeman, John Wilson, A. Dally, Claudio Gotti, M. Maino, C. Pira, Yu. G. Kolomensky, Luigi Cappelli, Simone Capelli, H. W. Wang, R. W. Kadel, G. Keppel, D. R. Artusa, Larissa M. Ejzak, B. X. Zhu, T. O'Donnell, Monica Sisti, Lorenzo Cassina, V. Pettinacci, L. Cardani, C. Maiano, Lindley Winslow, X. Z. Cai, L. Wielgus, Carlo Ligi, C. Rusconi, G. Piperno, S. Morganti, M. I. Martínez, Ioan Dafinei, L. Zanotti, M. Pavan, A. Drobizhev, D. Orlandi, Kevin Hickerson, M. A. Franceschi, D. Q. Fang, C. Pagliarone, T. Wise, V. Palmieri, A. Caminata, Elena Sala, Ezio Previtali, Y. Mei, Eric B. Norman, T. Napolitano, R. Hennings-Yeomans, Xi-Guang Cao, K. M. Heeger, M. Biassoni, Ke Han, Reina H. Maruyama, Stuart J. Freedman, J. L. Ouellet, A. Woodcraft, F. Terranova, Sisti, M, Artusa, D, Avignone, F, Azzolini, O, Balata, M, Banks, T, Bari, G, Beeman, J, Bellini, F, Bersani, A, Biassoni, M, Brofferio, C, Bucci, C, Cai, X, Camacho, A, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Carbone, L, Cardani, L, Casali, N, Cassina, L, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, Dafinei, I, Dally, A, Datskov, V, Dell'Oro, S, Deninno, M, Di Domizio, S, di Vacri, M, Drobizhev, A, Ejzak, L, Fang, D, Farach, H, Faverzani, M, Fernandes, G, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Haller, E, Han, K, Heeger, K, Hennings Yeomans, R, Hickerson, K, Huang, H, Kadel, R, Keppel, G, Kolomensky, Y, Li, Y, Ligi, C, Lim, K, Liu, X, Ma, Y, Maiano, C, Maino, M, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nisi, S, Nones, C, Norman, E, Nucciotti, A, O'Donnell, T, Orio, F, Orlandi, D, Ouellet, J, Pagliarone, C, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pedretti, M, Pessina, G, Pettinacci, V, Piperno, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Rosenfeld, C, Rusconi, C, Sala, E, Sangiorgio, S, Scielzo, N, Smith, A, Taffarello, L, Tenconi, M, Terranova, F, Tian, W, Tomei, C, Trentalange, S, Ventura, G, Vignati, M, Wang, B, Wang, H, Wielgus, L, Wilson, J, Winslow, L, Wise, T, Woodcraft, A, Zanotti, L, Zarra, C, Zhang, G, Zhu, B, Zucchelli, S, Sisti, M., Artusa, D.R., Avignone, F.T., Azzolini, O., Balata, M., Banks, T.I., Bari, G., Beeman, J., Bellini, F., Bersani, A., Biassoni, M., Brofferio, C., Bucci, C., Cai, X.Z., Camacho, A., Caminata, A., Canonica, L., Cao, X.G., Capelli, S., Cappelli, L., Carbone, L., Cardani, L., Casali, N., Cassina, L., Chiesa, D., Chott, N., Clemenza, M., Copello, S., Cosmelli, C., Cremonesi, O., Creswick, R.J., Cushman, J.S., Dafinei, I., Dally, A., Datskov, V., Dell'Oro, S., Deninno, M.M., Di Domizio, S., di Vacri, M.L., Drobizhev, A., Ejzak, L., Fang, D.Q., Farach, H.A., Faverzani, M., Fernandes, G., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M.A., Freedman, S.J., Fujikawa, B.K., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Gotti, C., Gutierrez, T.D., Haller, E.E., Han, K., Heeger, K.M., Hennings-Yeomans, R., Hickerson, K.P., Huang, H.Z., Kadel, R., Keppel, G., Kolomensky, Yu.G., Li, Y.L., Ligi, C., Lim, K.E., Liu, X., Ma, Y.G., Maiano, C., Maino, M., Martinez, M., Maruyama, R.H., Mei, Y., Moggi, N., Morganti, S., Napolitano, T., Nastasi, M., Nisi, S., Nones, C., Norman, E.B., Nucciotti, A., O'Donnell, T., Orio, F., Orlandi, D., Ouellet, J.L., Pagliarone, C.E., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pedretti, M., Pessina, G., Pettinacci, V., Piperno, G., Pira, C., Pirro, S., Pozzi, Stefano, Previtali, E., Rosenfeld, C., Rusconi, C., Sala, E., Sangiorgio, S., Scielzo, N.D., Smith, A.R., Taffarello, L., Tenconi, M., Terranova, F., Tian, W.D., Tomei, C., Trentalange, S., Ventura, G., Vignati, M., Wang, B.S., Wang, H.W., Wielgus, L., Wilson, J., Winslow, L.A., Wise, T., Woodcraft, A., Zanotti, L., Zarra, C., Zhang, G.Q., Zhu, B.X., and Zucchelli, S.
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Physics ,Particle physics ,Nuclear and High Energy Physics ,010308 nuclear & particles physics ,Bolometer ,Bolometers ,01 natural sciences ,Beta decay ,Double beta decay ,Particle detector ,Massless particle ,Nuclear physics ,CUORE ,Neutrino mass ,0103 physical sciences ,Neutrino ,010306 general physics ,Neutrino ma ,Radioactive decay ,Lepton - Abstract
CUORE is a 741kg array of TeO 2 bolometers for the search of neutrinoless double beta decay of 130 Te. The detectoris being constructed at the Laboratori Nazionali del Gran Sasso, Italy, where it will start taking data in 2015. If thetarget background of 0.01counts/(keVkgy) will be reached, in five years of data taking CUORE will have a 1˙halflife sensitivity of 10 26 y. CUORE-0 is a smaller experiment constructed to test and demonstrate the performancesexpected for CUORE. The detector is a single tower of 52 CUORE-like bolometers that started taking data in spring2013. The status and perspectives of CUORE will be discussed, and the first CUORE-0 data will be presented.Keywords: Double beta decay, Neutrino mass, Bolometers1. IntroductionNeutrinos are massive particles. A beautiful proof ofthis important property was obtained by neutrino oscil-lation experiments more than a decade ago. Since then,the key role of neutrinoless double beta decay searcheshas been established, as attested by the growing numberof experimental proposals in the last years.Neutrinoless double beta decay ( 0 ) is a proposedvery rare nuclear process in which a nucleus transformsinto its (A,Z+2) isobar with the emission of two elec-trons. While the two neutrino channel ( 2 ) – wheretwo neutrinos are contemporary emitted in the decay – isallowed by the Standard Model of Particle Physics andhas been observed experimentally in a dozen of isotopeswith half-lives of the order 10
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- 2016
173. Inside HOLMES experiment: 163Ho metallic target production for the micro-calorimeter absorber
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Daniel S. Swetz, C. Boragno, M. De Gerone, A. Puiu, Michele Biasotti, Rugard Dressler, Emanuele Ferri, U. Koster, Peter Day, Andrea Giachero, Carl D. Reintsema, Stefano Nisi, F. Terranova, S. Heinitz, M. Lusignoli, A. Nucciotti, G. Pessina, C. Brofferio, S. Ragazzi, Joel N. Ullom, M. Faverazani, J. Folwer, Bradley K. Alpert, John A. B. Mates, D. Shmidt, M. Sisti, M. Maino, G. Pizzigoni, M. Ribeiro Gomes, D. A. Bennett, Dorothea Schumann, R. Nizzolo, M. Balata, G. Hilton, Flavio Gatti, Pizzigoni, G, Alpert, B, Balata, M, Bennett, D, Biasotti, M, Boragno, C, Brofferio, C, De Gerone, M, Dressler, R, Faverzani, M, Ferri, E, Folwer, J, Gatti, F, Giachero, A, Heinitz, S, Hilton, G, Köster, U, Lusignoli, M, Maino, M, Mates, J, Nisi, S, Nizzolo, R, Nucciotti, A, Pessina, G, Puiu, P, Ragazzi, S, Reintsema, C, Ribeiro Gomes, M, Shmidt, D, Schumann, D, Sisti, M, Swetz, D, Terranova, F, Ullom, J, and Day, P
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Nuclear and High Energy Physics ,Analytical chemistry ,Oxide ,chemistry.chemical_element ,01 natural sciences ,Metal ,Nuclear physics ,chemistry.chemical_compound ,Neutrino mass ,0103 physical sciences ,Irradiation ,Reduction and distillation process ,010306 general physics ,Instrumentation ,Holmes experiment ,Physics ,Reduction and distillation proce ,Isotope ,010308 nuclear & particles physics ,Neutron temperature ,Calorimeter ,Chemical state ,chemistry ,visual_art ,visual_art.visual_art_medium ,Holmium ,Neutrino ma - Abstract
The main goal in the HOLMES experiment is the neutrino mass measurement using an array of 1000 micro-calorimeters with standard metallic absorber. A good isotope for such measurement is the 163 Ho, those isotopes embedded in the metallic absorber will be 10 11 –10 13 . Since 163 Ho is not available in nature, a dedicated process must be set up to produce the amount needed for this neutrino mass experiment. The process with the highest born-up cross-section is the neutron irradiation of Er 2 O 3 enriched in 162 Er: 162 Er(n,γ) 163 Er → 163 Ho+ν e , where the decay is an EC with half-life of about 75 min and the (n,γ) is about 20 barns for thermal neutron. After the neutron irradiation in the oxide powder there are several radioactive isotopes which are potentially disturbing because of the background that they cause below 5 keV. The chemical separation of holmium from the irradiation enriched Er 2 O 3 powder is therefore mandatory and will be performed by means of ion exchange chromatography. On the end of those processes the oxide powder enriched in 162 Er will have the 163 Ho isotope number required. The holmium chemical state influences the end point of the EC spectrum, in order to avoid such effect it is necessary to embed in the absorber only the metallic isotope. Reduction and distillation technique allowed us to obtain a pure metallic holmium, starting from natural oxide holmium. This technique will be applied on the irradiated oxide powder to obtain the metallic 163 Ho, ready to be embedded in the micro-calorimeter absorber.
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- 2016
174. LUMINEU: a search for neutrinoless double beta decay based on ZnMoO$_4$ scintillating bolometers
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Armengaud, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Boiko, S., Bergmann, T., Blümer, J., Broniatowski, A., Brudanin, V., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., Chernyak, D. M., Coron, N., Coulter, P., Danevich, F. A., De Boissiére, T., Decourt, R., De Jesus, M., Devoyon, L., Drillien, A. A., Dumoulin, L., Eitel, K., Enss, C., Filosofov, D., Fleischmann, A., Foerster, N., Fourches, N., Gascon, J., Gastaldo, L., Gerbier, G., Giuliani, ANDREA ERNESTO GUIDO, Gray, D., Gros, M., Hehn, L., Henry, S., Hervé, S., Heuermann, G., Humbert, V., Ivanov, I. M., Juillard, A., Kéfélian, C., Kleifges, M., Kluck, H., Kobychev, V. V., Koskas, F., Kozlov, V., Kraus, H., Kudryavtsev, V. A., Le Sueur, H., Loidl, M., Magnier, P., Makarov, E. P., Mancuso, Michele, De Marcillac, P., Marnieros, S., Marrache Kikuchi, C., Menshikov, A., Nasonov, S. G., Navick, X. F., Nones, C., Olivieri, E., Pari, P., Paul, B., Penichot, Y., Pessina, G., Piro, M. C., Plantevin, O., Poda, D. V., Redon, T., Robinson, M., Rodrigues, M., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Shlegel, V. N., Siebenborn, B., Strazzer, O., Tcherniakhovski, D., Tenconi, M., Torres, L., Tretyak, V. I., Vagneron, L., Vasiliev, Y. a. V., Velazquez, M., Viraphong, O., Walker, R. J., Weber, M., Yakushev, E., Zhang, X., Zhdankov, V. N., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-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 de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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), Institut Néel (NEEL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université de Bordeaux (UB), Laboratoire d'Intégration des Systèmes et des Technologies (LIST), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), 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), Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Université Paris-Saclay-Direction de Recherche Technologique (CEA) (DRT (CEA)), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Institut de Physique Nucléaire de Lyon ( IPNL ), 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 ), Centre de Sciences Nucléaires et de Sciences de la Matière ( CSNSM ), 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 ), Institut Néel ( NEEL ), Université Grenoble Alpes [Saint Martin d'Hères]-Centre National de la Recherche Scientifique ( CNRS ), Institut d'astrophysique spatiale ( IAS ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Université de Bordeaux ( UB ), Laboratoire d'Intégration des Systèmes et des Technologies ( LIST ), Hélium : du fondamental aux applications (NEEL - HELFA), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Karlsruhe Institute of Technology (KIT), Joint Institute for Nuclear Research (JINR), Cryogénie (NEEL - Cryo), Kiev Institute for Nuclear Research (KINR), Ukrainian Academy of Sciences, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), University of Oxford, Kirchhoff Institut für Physik, Universität Heidelberg [Heidelberg] = Heidelberg University, Nikolaev Institute of Inorganic Chemistry [Novosibirsk] (NIC), Siberian Branch of the Russian Academy of Sciences (SB RAS), University of Sheffield [Sheffield], Laboratoire National Henri Becquerel (LNHB), Département Métrologie Instrumentation & Information (DM2I), Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département d'instrumentation Numérique (DIN (CEA-LIST)), Istituto Nazionale di Fisica Nucleare, Sezione di Milano (INFN), Istituto Nazionale di Fisica Nucleare (INFN), CML Ltd., University of Torino, INFN, and Fornengo, Nicolao (ed.) (University of Torino and INFN)
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History ,Physics - Instrumentation and Detectors ,design ,hierarchy ,7. Clean energy ,01 natural sciences ,neutrino mass ,law.invention ,Crystal ,molybdenum ,law ,energy resolution: measured ,beta-rays ,neutrino: mass ,Nuclear Experiment (nucl-ex) ,[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex] ,Nuclear Experiment ,[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,nuclear instrumentation ,Physics ,instrumentation ,Detector ,Resolution (electron density) ,double-beta decay ,Instrumentation and Detectors (physics.ins-det) ,high energy resolution ,3. Good health ,Computer Science Applications ,particle: interaction ,experimental equipment ,radioactivity ,technology ,Neutrino ,ionizing radiation ,performance ,FOS: Physical sciences ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,Education ,crystal ,Nuclear physics ,interaction particle ,Physics and Astronomy (all) ,bolometer ,double-beta decay: (0neutrino) ,Double beta decay ,0103 physical sciences ,Sensitivity (control systems) ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,010306 general physics ,scintillation counter ,detector ,010308 nuclear & particles physics ,background ,Bolometer ,Neutrinoless ,sensitivity ,energy resolution: high ,Energy (signal processing) ,experimental results - Abstract
The LUMINEU is designed to investigate the possibility to search for neutrinoless double beta decay in $^{100}$Mo by means of a large array of scintillating bolometers based on ZnMoO$_4$ crystals enriched in $^{100}$Mo. High energy resolution and relatively fast detectors, which are able to measure both the light and the heat generated upon the interaction of a particle in a crystal, are very promising for the recognition and rejection of background events. We present the LUMINEU concepts and the experimental results achieved aboveground and underground with large-mass natural and enriched crystals. The measured energy resolution, the $\alpha/\beta$ discrimination power and the radioactive internal contamination are all within the specifications for the projected final LUMINEU sensitivity. Simulations and preliminary results confirm that the LUMINEU technology can reach zero background in the region of interest (around 3 MeV) with exposures of the order of hundreds kg$\times$years, setting the bases for a next generation $0\nu2\beta$ decay experiment capable to explore the inverted hierarchy region of the neutrino mass pattern., Comment: 5 pages, 3 figures, submitted as proceedings of the TAUP 2015 conference
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- 2015
175. Possible indication for non-zero neutrino mass and additional neutrino species from cosmological observations
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Burenin, R. A.
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- 2013
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176. Direct neutrino mass measurements
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Weinheimer, Christian
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- 2013
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177. A natural connection between neutrino mass generation and the lightness of a next-to-minimal supersymmetric Standard Model pseudoscalar
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DAS, DEBOTTAM, ABADA, ASMAA, BHATTACHARYYA, GAUTAM, and WEILAND, CÉDRIC
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- 2012
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178. Neutrinoless double beta decay
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ZUBER, KAI
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- 2012
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179. Theoretical aspects of neutrino mass and lepton flavour violation
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ROSS, GRAHAM G
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- 2012
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180. An Improved ZnMoO4 Scintillating Bolometer for the Search for Neutrinoless Double Beta Decay of 100Mo
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Beeman, J. W., Danevich, F. A., Degoda, V. Y., Galashov, E. N., Giuliani, A., Ivanov, I. M., Mancuso, M., Marnieros, S., Nones, C., Pessina, G., Olivieri, E., Rusconi, C., Shlegel, V. N., Tretyak, V. I., and Vasiliev, Y. V.
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- 2012
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181. Neutrino Physics with Low-Temperature Detectors
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Giuliani, A.
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- 2012
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182. Development of Metallic Magnetic Calorimeters for High Precision Measurements of Calorimetric 187Re and 163Ho Spectra
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Ranitzsch, P. C.-O., Porst, J.-P., Kempf, S., Pies, C., Schäfer, S., Hengstler, D., Fleischmann, A., Enss, C., and Gastaldo, L.
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- 2012
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183. CUORE: The Challenge of a 988 Bolometer Array
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Gironi, L.
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- 2012
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184. MARE-1 in Milan: Status and Perspectives
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Ferri, E., Arnaboldi, C., Ceruti, G., Faverzani, M., Gatti, F., Giachero, A., Gotti, C., Kilbourne, C., Kraft-Bermuth, S., Nucciotti, A., Pessina, G., Schaeffer, D., and Sisti, M.
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- 2012
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185. DeepCMB: Lensing reconstruction of the cosmic microwave background with deep neural networks.
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Caldeira, J., Wu, W.L.K., Nord, B., Avestruz, C., Trivedi, S., and Story, K.T.
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NEUTRINO mass ,COSMIC background radiation ,GRAVITATIONAL potential ,NEUTRINOS ,CONSTRAINTS (Physics) ,GRAVITATIONAL lenses ,SIGNAL-to-noise ratio ,PARAMETER estimation - Abstract
Next-generation cosmic microwave background (CMB) experiments will have lower noise and therefore increased sensitivity, enabling improved constraints on fundamental physics parameters such as the sum of neutrino masses and the tensor-to-scalar ratio r. Achieving competitive constraints on these parameters requires high signal-to-noise extraction of the projected gravitational potential from the CMB maps. Standard methods for reconstructing the lensing potential employ the quadratic estimator (QE). However, the QE is known to perform suboptimally at the low noise levels expected in upcoming experiments. Other methods, like maximum likelihood estimators (MLE), are under active development. In this work, we demonstrate reconstruction of the CMB lensing potential with deep convolutional neural networks (CNN) — i.e., a ResUNet. The network is trained and tested on simulated data, and otherwise has no physical parametrization related to the physical processes of the CMB and gravitational lensing. We show that, over a wide range of angular scales, ResUNets recover the input gravitational potential with a higher signal-to-noise ratio than the QE method, reaching levels comparable to analytic approximations of MLE methods. We demonstrate that the network outputs quantifiably different lensing maps when given input CMB maps generated with different cosmologies. We also show we can use the reconstructed lensing map for cosmological parameter estimation. This application of CNNs provides a few innovations at the intersection of cosmology and machine learning. First, while training and regressing on images, this application predicts a continuous-variable field rather than discrete classes. Second, we are able to establish uncertainty measures for the network output that are analogous to standard methods. Beyond this first demonstration, we expect this approach to excel in capturing hard-to-model non-Gaussian astrophysical foreground and noise contributions. [ABSTRACT FROM AUTHOR]
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- 2019
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186. Neutrino-less double beta decays and Majorana neutrinos: Overview of the present and future experiments
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Ejiri, Hiroyasu
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- 2011
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187. Neutrino mass hierarchy and lepton flavor mixing
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Xing, Zhi-zhong
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- 2011
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188. The development of a super-stable datum point for monitoring the energy scale of electron spectrometers in the energy range up to 20 keV
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Vénos, D., Zbořil, M., Kašpar, J., Dragoun, O., Bonn, J., Kovalík, A., Lebeda, O., Lebedev, N. A., Ryšavý, M., Schlösser, K., Špalek, A., and Weinheimer, Ch.
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- 2010
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189. Searching the absolute neutrino mass in tritium β-decay—interplay between nuclear, atomic and molecular physics
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Otten, Ernst
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- 2010
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190. Leptogenesis with supersymmetric Higgs triplets in the TeV region
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Senami, M and Yamamoto, K
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leptogenesis ,supersymmetry ,neutrino mass ,Higgs triplet - Published
- 2006
191. Direct neutrino mass measurements after PLANCK
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Joseph A. Formaggio, Massachusetts Institute of Technology. Department of Physics, Massachusetts Institute of Technology. Laboratory for Nuclear Science, and Formaggio, Joseph A.
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Physics ,Particle physics ,Oscillation ,Astronomy and Astrophysics ,Beta decay ,Cosmological model ,Solar neutrino problem ,Cosmology ,symbols.namesake ,Neutrino mass ,Space and Planetary Science ,symbols ,Mass scale ,Neutrino ,Planck ,Electron capture - Abstract
The absolute mass scale of neutrinos remains an open question subject to experimental investigation from both particle physics and cosmology. Over the next decade, a number of experiments from both disciplines will attempt to probe the mass scale further to the very limits of the predictions from oscillation results. This paper provides a broad overview of the experimental program in neutrino mass scale measurements, with a particular focus on direct experimental probes due to come online over the next decade., United States. Dept. of Energy (Contract DE-FG02-06ER-41420)
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- 2014
192. Elementary muon, pion, and kaon particles as resonators for neutrino quanta. Calculations of mass ratios for e, μ, π0, π±, K 0, K ±, and ν e
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Buravov, L. I.
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- 2009
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193. The MARE Project
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Nucciotti, A.
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- 2008
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194. Development and Characterization of Microcalorimeters for a Next Generation 187Re Beta-Decay Experiment
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Kraft-Bermuth, S., Arnaboldi, C., Ferri, E., Kilbourne, C., Margesin, B., McCammon, D., Monfardini, A., Nucciotti, A., Pessina, G., Previtali, E., Schaeffer, D., and Sisti, M.
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- 2008
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195. Parameterization of neutrino (e,μ,τ,τ’) “flavor” oscillations in a simplified SM4 model
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Makowitz, H.
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- 2007
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196. Neutrinoless ββ decay and the electron neutrino mass
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Civitarese, Osvaldo and Suhonen, Jouni
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- 2006
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197. Hans Bethe, the sun and the neutrinos
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Rajasekaran, G
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- 2005
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198. Mean square number fluctuation for a fermion source and its dependence on neutrino mass for the universal cosmic neutrino background
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Jawkar, Swapnil S. and Jha, Sudhanshu S.
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- 2005
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199. Search for Majorana Neutrinos in B− → π+ μ− μ− Decays
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Aaij, R, Adeva, B, Adinolfi, M, Affolder, A, Ajaltouni, Z, Albrecht, J, Alessio, F, Alexander, M, Ali, S, Alkhazov, G, Alvarez Cartelle, P, Alves, A. A, Amato, S, Amerio, S, Amhis, Y, Anderlini, L, Anderson, J, Andreassen, R, Andreotti, M, Andrews, J. E, Appleby, R. B, Aquines Gutierrez, O, Archilli, F, Artamonov, A, Artuso, M, Aslanides, E, Auriemma, G, Baalouch, M, Bachmann, S, Back, J. J, Badalov, A, Balagura, V, Baldini, W, Barlow, R. J, Barschel, C, Barsuk, S, Barter, W, Batozskaya, V, Bauer, T, Bay, A, Beddow, J, Bedeschi, F, Bediaga, I, Belogurov, S, Belous, K, Belyaev, I, Ben Haim, E, Bencivenni, G, Benson, S, Benton, J, Berezhnoy, A, Bernet, R, Bettler, M. O, van Beuzekom, M, Bien, A, Bifani, S, Bird, T, Bizzeti, A, Bjørnstad, P. M, Blake, T, Blanc, F, Blouw, J, Blusk, S, Bocci, V, Bondar, A, Bondar, N, Bonivento, W, Borghi, S, Borgia, A, Borsato, M, Bowcock, T. J. V, Bowen, E, Bozzi, C, Brambach, T, van den Brand, J, Bressieux, J, Brett, D, Britsch, M, Britton, T, Brook, N. H, Brown, H, Bursche, A, Busetto, G, Buytaert, J, Cadeddu, S, Calabrese, R, Callot, O, Calvi, M, Calvo Gomez, M, Camboni, A, Campana, P, Campora Perez, D, Carbone, A, Carboni, G, Cardinale, R, Cardini, A, Carranza Mejia, H, Carson, L, Carvalho Akiba, K, Casse, G, Castillo Garcia, L, Cattaneo, M, Cauet, C, Cenci, R, Charles, M, Charpentier, P, Cheung, S. F, Chiapolini, N, Chrzaszcz, M, Ciba, K, Cid Vidal, X, Ciezarek, G, Clarke, P. E. L, Clemencic, M, Cliff, H. V, Closier, J, Coca, C, Coco, V, Cogan, J, Cogneras, E, Collins, P, Comerma Montells, A, Contu, A, Cook, A, Coombes, M, Coquereau, S, Corti, G, Counts, I, Couturier, B, Cowan, G. A, Craik, D. C, Cruz Torres, M, Cunliffe, S, Currie, R, D'Ambrosio, C, Dalseno, J, David, P, David, P. N. Y, Davis, A, De Bonis, I, De Bruyn, K, De Capua, S, De Cian, M, De Miranda, J. M, De Paula, L, De Silva, W, De Simone, P, Decamp, D, Deckenhoff, M, Del Buono, L, Déléage, N, Derkach, D, Deschamps, O, Dettori, F, Di Canto, A, Dijkstra, H, Donleavy, S, Dordei, F, Dorigo, M, Dorosz, P, Dosil Suárez, A, Dossett, D, Dovbnya, A, Dupertuis, F, Durante, P, Dzhelyadin, R, Dziurda, A, Dzyuba, A, Easo, S, Egede, U, Egorychev, V, Eidelman, S, Eisenhardt, S, Eitschberger, U, Ekelhof, R, Eklund, L, El Rifai, I, Elsasser, C, Falabella, A, Färber, C, Farinelli, C, Farry, S, Ferguson, D, Fernandez Albor, V, Ferreira Rodrigues, F, Ferro Luzzi, M, Filippov, S, Fiore, M, Fiorini, M, Fitzpatrick, C, Fontana, M, Fontanelli, F, Forty, R, Francisco, O, Frank, M, Frei, C, Frosini, M, Furfaro, E, Gallas Torreira, A, Galli, D, Gandelman, M, Gandini, P, Gao, Y, Garofoli, J, Garra Tico, J, Garrido, L, Gaspar, C, Gauld, R, Gersabeck, E, Gersabeck, M, Gershon, T, Ghez, P, Gianelle, A, Gibson, V, Giubega, L, Gligorov, V. V, Göbel, C, Golubkov, D, Golutvin, A, Gomes, A, Gordon, H, Grabalosa Gándara, M, Graciani Diaz, R, Granado Cardoso, L. A, Graugés, E, Graziani, G, Grecu, A, Greening, E, Gregson, S, Griffith, P, Grillo, L, Grünberg, O, Gui, B, Gushchin, E, Guz, Y, Gys, T, Hadjivasiliou, C, Haefeli, G, Haen, C, Hafkenscheid, T. W, Haines, S. C, Hall, S, Hamilton, B, Hampson, T, Hansmann Menzemer, S, Harnew, N, Harnew, S. T, Harrison, J, Hartmann, T, He, J, Head, T, Heijne, V, Hennessy, K, Henrard, P, Hernando Morata, J. A, van Herwijnen, E, Heß, M, Hicheur, A, Hill, D, Hoballah, M, Hombach, C, Hulsbergen, W, Hunt, P, Huse, T, Hussain, N, Hutchcroft, D, Hynds, D, Iakovenko, V, Idzik, M, Ilten, P, Jacobsson, R, Jaeger, A, Jans, E, Jaton, P, Jawahery, A, Jing, F, John, M, Johnson, D, Jones, C. R, Joram, C, Jost, B, Jurik, N, Kaballo, M, Kandybei, S, Kanso, W, Karacson, M, Karbach, T. M, Kenyon, I. R, Ketel, T, Khanji, B, Khurewathanakul, C, Klaver, S, Kochebina, O, Komarov, I, Koopman, R. F, Koppenburg, P, Korolev, M, Kozlinskiy, A, Kravchuk, L, Kreplin, K, Kreps, M, Krocker, G, Krokovny, P, Kruse, F, Kucharczyk, M, Kudryavtsev, V, Kurek, K, Kvaratskheliya, T, La Thi, V. N, Lacarrere, D, Lafferty, G, Lai, A, Lambert, D, Lambert, R. W, Lanciotti, E, Lanfranchi, G, Langenbruch, C, Latham, T, Lazzeroni, C, Le Gac, R, van Leerdam, J, Lees, J. P, Lefèvre, R, Leflat, A, Lefrançois, J, Leo, S, Leroy, O, Lesiak, T, Leverington, B, Li, Y, Liles, M, Lindner, R, Linn, C, Lionetto, F, Liu, B, Liu, G, Lohn, S, Longstaff, I, Lopes, J. H, Lopez March, N, Lowdon, P, Lu, H, Lucchesi, D, Luisier, J, Luo, H, Luppi, E, Lupton, O, Machefert, F, Machikhiliyan, I. V, Maciuc, F, Maev, O, Malde, S, Manca, G, Mancinelli, G, Manzali, M, Maratas, J, Marconi, U, Marino, P, Märki, R, Marks, J, Martellotti, G, Martens, A, Martín Sánchez, A, Martinelli, M, Martinez Santos, D, Martins Tostes, D, Massafferri, A, Matev, R, Mathe, Z, Matteuzzi, C, Mazurov, A, Mccann, M, Mccarthy, J, Mcnab, A, Mcnulty, R, Mcskelly, B, Meadows, B, Meier, F, Meissner, M, Merk, M, Milanes, D. A, Minard, M. N, Molina Rodriguez, J, Monteil, S, Moran, D, Morandin, M, Morawski, P, Mordà, A, Morello, M. J, Mountain, R, Mous, I, Muheim, F, Müller, K, Muresan, R, Muryn, B, Muster, B, Naik, P, Nakada, T, Nandakumar, R, Nasteva, I, Needham, M, Neubert, S, Neufeld, N, Nguyen, A. D, Nguyen, T. D, Nguyen Mau, C, Nicol, M, Niess, V, Niet, R, Nikitin, N, Nikodem, T, Novoselov, A, Oblakowska Mucha, A, Obraztsov, V, Oggero, S, Ogilvy, S, Okhrimenko, O, Oldeman, R, Onderwater, G, Orlandea, M, Otalora Goicochea, J. M, Owen, P, Oyanguren, A, Pal, B. K, Palano, A, Palutan, M, Panman, J, Papanestis, A, Pappagallo, M, Pappalardo, L, Parkes, C, Parkinson, C. J, Passaleva, G, Patel, G. D, Patel, M, Patrignani, C, Pavel Nicorescu, C, Pazos Alvarez, A, Pearce, A, Pellegrino, A, Penso, G, Pepe Altarelli, M, Perazzini, S, Perez Trigo, E, Perret, P, Perrin Terrin, M, Pescatore, L, Pesen, E, Pessina, G, Petridis, K, Petrolini, A, Picatoste Olloqui, E, Pietrzyk, B, Pilař, T, Pinci, D, Pistone, A, Playfer, S, Plo Casasus, M, Polci, F, Polok, G, Poluektov, A, Polycarpo, E, Popov, A, Popov, D, Popovici, B, Potterat, C, Powell, A, Prisciandaro, J, Pritchard, A, Prouve, C, Pugatch, V, Puig Navarro, A, Punzi, G, Qian, W, Rachwal, B, Rademacker, J. H, Rakotomiaramanana, B, Rama, M, Rangel, M. S, Raniuk, I, Rauschmayr, N, Raven, G, Redford, S, Reichert, S, Reid, M. M, dos Reis, A. C, Ricciardi, S, Richards, A, Rinnert, K, Rives Molina, V, Roa Romero, D. A, Robbe, P, Roberts, D. A, Rodrigues, A. B, Rodrigues, E, Rodriguez Perez, P, Roiser, S, Romanovsky, V, Romero Vidal, A, Rotondo, M, Rouvinet, J, Ruf, T, Ruffini, F, Ruiz, H, Ruiz Valls, P, Sabatino, G, Saborido Silva, J. J, Sagidova, N, Sail, P, Saitta, B, Salustino Guimaraes, V, Sanmartin Sedes, B, Santacesaria, R, Santamarina Rios, C, Santovetti, E, Sapunov, M, Sarti, A, Satriano, C, Satta, A, Savrie, M, Savrina, D, Schiller, M, Schindler, H, Schlupp, M, Schmelling, M, Schmidt, B, Schneider, O, Schopper, A, Schune, M. H, Schwemmer, R, Sciascia, B, Sciubba, A, Seco, M, Semennikov, A, Senderowska, K, Sepp, I, Serra, N, Serrano, J, Seyfert, P, Shapkin, M, Shapoval, I, Shcheglov, Y, Shears, T, Shekhtman, L, Shevchenko, O, Shevchenko, V, Shires, A, Silva Coutinho, R, Simi, G, Sirendi, M, Skidmore, N, Skwarnicki, T, Smith, N. A, Smith, E, Smith, J, Smith, M, Snoek, H, Sokoloff, M. D, Soler, F. J. 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Waldi, R, Wallace, C, Wallace, R, Wandernoth, S, Wang, J, Ward, D, Watson, N, Webber, A, Websdale, D, Whitehead, M, Wicht, J, Wiechczynski, J, Wiedner, D, Wiggers, L, Wilkinson, G, Williams, M, Wilson, F, Wimberley, J, Wishahi, J, Wislicki, W, Witek, M, Wormser, G, Wotton, S, Wright, S, Wu, S, Wyllie, K, Xie, Y, Xing, Z, Yang, Z, Yuan, X, Yushchenko, O, Zangoli, M, Zavertyaev, M, Zhang, F, Zhang, L, Zhang, W, Zhang, Y, Zhelezov, A, Zhokhov, A, Zhong, L, and Zvyagin, A
- Subjects
Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,14.40.Nd ,LHCb - Abteilung Hofmann ,Decay mode ,Fourth generation ,Physics and Astronomy (all) ,Center-of-mass energies ,Tellurium compounds ,Neutrino mass ,Leptonic semileptonic and radiative decays of bottom meson ,Branching fractions ,High energy physics ,Neutrons ,Integrated luminosity ,High Energy Physics::Phenomenology ,13.35.Hb ,Upper limits ,Decays of heavy neutrino ,LHCb ,13.20.He ,0%29%22">Bottom mesons (|B|>0) ,High Energy Physics::Experiment ,LHC ,Branching fractions, Center-of-mass energies, Decay mode, Fourth generation, Integrated luminosity, Majorana neutrino, Neutrino mass, Upper limits ,High energy physics, Tellurium compounds ,Majorana neutrino - Abstract
A search for heavy Majorana neutrinos produced in the $B^- \to \pi^+\mu^-\mu^-$ decay mode is performed using 3 fb$^{-1}$ of integrated luminosity collected with the LHCb detector in $pp$ collisions at center-of-mass energies of 7 TeV and 8 TeV at the LHC. Neutrinos with masses in the range 250-5000 MeV and lifetimes from zero to 1000 ps are probed. In the absence of a signal, upper limits are set on the branching fraction ${\cal{B}}(B^- \to \pi^+\mu^-\mu^-)$ as functions of neutrino mass and lifetime. These limits are on the order of $10^{-9}$ for short neutrino lifetimes of 1 ps or less. Limits are also set on the coupling between the muon and a possible fourth-generation neutrino.
- Published
- 2014
200. Investigations of background due to secondary electron emission in the KATRIN-experiment
- Author
-
Leiber, Benjamin and Drexlin, G.
- Subjects
Neutrino mass ,Secondary electron emission ,Background ,Physics::Instrumentation and Detectors ,Physics ,Astrophysics::High Energy Astrophysical Phenomena ,ddc:530 ,KATRIN - Abstract
KATRIN will determine the effective mass of the electron anti-neutrino with a sensitivity of 200 meV (90% C.L.) by scanning the tritium-beta-spectrum close to the endpoint energy with unprecedented precision. The focus of this work lies on the detailed investigation of one of two main background sources of the experiment: the emission of secondary electrons from the large inner surface of the stainless steel vessel which are caused caused by cosmic ray muons and environmental radiation.
- Published
- 2014
- Full Text
- View/download PDF
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