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Your search keyword '"E. Ruiz-Chóliz"' showing total 4 results
Start Over Author "E. Ruiz-Chóliz" Journal journal of high energy physics
4 results on '"E. Ruiz-Chóliz"'

1. An accurate solar axions ray-tracing response of BabyIAXO

Author

IAXO collaboration, S. Ahyoune, K. Altenmüller, I. Antolín, S. Basso, P. Brun, F. R. Candón, J. F. Castel, S. Cebrián, D. Chouhan, R. Della Ceca, M. Cervera-Cortés, V. Chernov, M. M. Civitani, C. Cogollos, E. Costa, V. Cotroneo, T. Dafní, A. Derbin, K. Desch, M. C. Díaz-Martín, A. Díaz-Morcillo, D. Díez-Ibáñez, C. Diez Pardos, M. Dinter, B. Döbrich, I. Drachnev, A. Dudarev, A. Ezquerro, S. Fabiani, E. Ferrer-Ribas, F. Finelli, I. Fleck, J. Galán, G. Galanti, M. Galaverni, J. A. García, J. M. García-Barceló, L. Gastaldo, M. Giannotti, A. Giganon, C. Goblin, N. Goyal, Y. Gu, L. Hagge, L. Helary, D. Hengstler, D. Heuchel, S. Hoof, R. Iglesias-Marzoa, F. J. Iguaz, C. Iñiguez, I. G. Irastorza, K. Jakovčić, D. Käfer, J. Kaminski, S. Karstensen, M. Law, A. Lindner, M. Loidl, C. Loiseau, G. López-Alegre, A. Lozano-Guerrero, B. Lubsandorzhiev, G. Luzón, I. Manthos, C. Margalejo, A. Marín-Franch, J. Marqués, F. Marutzky, C. Menneglier, M. Mentink, S. Mertens, J. Miralda-Escudé, H. Mirallas, F. Muleri, V. Muratova, J. R. Navarro-Madrid, X. F. Navick, K. Nikolopoulos, A. Notari, A. Nozik, L. Obis, A. Ortiz-de-Solórzano, T. O’Shea, J. von Oy, G. Pareschi, T. Papaevangelou, K. Perez, O. Pérez, E. Picatoste, M. J. Pivovaroff, J. Porrón, M. J. Puyuelo, A. Quintana, J. Redondo, D. Reuther, A. Ringwald, M. Rodrigues, A. Rubini, S. Rueda-Teruel, F. Rueda-Teruel, E. Ruiz-Chóliz, J. Ruz, J. Schaffran, T. Schiffer, S. Schmidt, U. Schneekloth, L. Schönfeld, M. Schott, L. Segui, U. R. Singh, P. Soffitta, D. Spiga, M. Stern, O. Straniero, F. Tavecchio, E. Unzhakov, N. A. Ushakov, G. Vecchi, J. K. Vogel, D. M. Voronin, R. Ward, A. Weltman, C. Wiesinger, R. Wolf, A. Yanes-Díaz, and Y. Yu

Subjects
CP Violation, Dark Matter and Double Beta Decay (experiments), Dark Matter, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract BabyIAXO is the intermediate stage of the International Axion Observatory (IAXO) to be hosted at DESY. Its primary goal is the detection of solar axions following the axion helioscope technique. Axions are converted into photons in a large magnet that is pointing to the sun. The resulting X-rays are focused by appropriate X-ray optics and detected by sensitive low-background detectors placed at the focal spot. The aim of this article is to provide an accurate quantitative description of the different components (such as the magnet, optics, and X-ray detectors) involved in the detection of axions. Our efforts have focused on developing robust and integrated software tools to model these helioscope components, enabling future assessments of modifications or upgrades to any part of the IAXO axion helioscope and evaluating the potential impact on the experiment’s sensitivity. In this manuscript, we demonstrate the application of these tools by presenting a precise signal calculation and response analysis of BabyIAXO’s sensitivity to the axion-photon coupling. Though focusing on the Primakoff solar flux component, our virtual helioscope model can be used to test different production mechanisms, allowing for direct comparisons within a unified framework.

Published
2025
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2. First results of the CAST-RADES haloscope search for axions at 34.67 μeV

Author

I. Tsagris, S. Arguedas Cuendis, M. D. Hasinoff, C. Peña Garay, M. J. Pivovaroff, Konstantin Zioutas, Marc Schumann, E. Widmann, Javier Redondo, K. Özbozduman, A. Gardikiotis, Wolfgang Funk, Sami K. Solanki, Juan Daniel Gallego, L. Stewart, Klaus Kurt Desch, M. Maroudas, S. Calatroni, A. J. Lozano-Guerrero, J. F. Castel, H. Mirallas, Giovanni Cantatore, Benito Gimeno, C. Cogollos, Marin Karuza, P. Navarro, Babette Döbrich, T. Dafni, Yannis K. Semertzidis, Alejandro Díaz-Morcillo, Theodoros Vafeiadis, D. H. H. Hoffmann, Heinrich Bräuninger, J. M. Laurent, J.M. García Barceló, Serkant Ali Cetin, Chloé Malbrunot, J. Baier, Jochen Kaminski, J. Ruz, S. Schmidt, Fritz Caspers, I. G. Irastorza, E. Ruiz Chóliz, S. N. Gninenko, Walter Wuensch, A. V. Dermenev, A. Ozbey, J. Golm, M. Davenport, Jordi Miralda-Escudé, Julia Vogel, K. Barth, G. Luzón, Biljana Lakić, Krešimir Jakovčić, H. Fischer, L. Miceli, J. G. Garza, Alejandro Álvarez Melcón, İstinye Üniversitesi, Serkant Ali Çetin / 0000-0001-5050-8441, Cetin, Serkant Ali, Ministerio de Ciencia, Innovación y Universidades (España), European Commission, German Research Foundation, Department of Energy (US), SCOAP, European Research Council, Generalitat Valenciana, Agencia Estatal de Investigación (España), Ministerio de Economía y Competitividad (España), European Organization for Nuclear Research, Diputación General de Aragón, and Gobierno de Aragón

Subjects
Exotics, Nuclear and High Energy Physics, Dark-Matter, Cavity, Cp Conservation, Library science, QC770-798, 01 natural sciences, High Energy Physics - Experiment, Dark matter, Dark Matter and Double Beta Decay (experiments), Nuclear and particle physics. Atomic energy. Radioactivity, 0103 physical sciences, media_common.cataloged_instance, Dark Matter, European union, 010306 general physics, media_common, Physics, 010308 nuclear & particles physics, hep-ex, European research, Advice (programming), National laboratory, Particle Physics - Experiment
Abstract

et al., We present results of the Relic Axion Dark-Matter Exploratory Setup (RADES), a detector which is part of the CERN Axion Solar Telescope (CAST), searching for axion dark matter in the 34.67 μeV mass range. A radio frequency cavity consisting of 5 sub-cavities coupled by inductive irises took physics data inside the CAST dipole magnet for the first time using this filter-like haloscope geometry. An exclusion limit with a 95% credibility level on the axion-photon coupling constant of gaγ ≳ 4 × 10−13 GeV−1 over a mass range of 34.6738 μeV < ma < 34.6771 μeV is set. This constitutes a significant improvement over the current strongest limit set by CAST at this mass and is at the same time one of the most sensitive direct searches for an axion dark matter candidate above the mass of 25 μeV. The results also demonstrate the feasibility of exploring a wider mass range around the value probed by CAST-RADES in this work using similar coherent resonant cavities., Article funded by SCOAP3., This work has been funded by the Spanish Agencia Estatal de Investigacion (AEI) and Fondo Europeo de Desarrollo Regional (FEDER) under project FPA-2016-76978-C3-2-P (supported by the grant FPI BES-2017-079787) and PID2019-108122GB-C33, and was supported by the CERN Doctoral Studentship programme. The research leading to these results has received funding from the European Research Council and BD, JG and SAC acknowledge support through the European Research Council under grant ERC-2018-StG-802836 (AxScale project). BD also acknowledges fruitful discussions at MIAPP supported by DFG under EXC-2094 – 390783311. IGI acknowledges also support from the European Research Council (ERC) under grant ERC-2017-AdG-788781 (IAXO+ project). JR has been supported by the Ramon y Cajal Fellowship 2012-10597, the grant PGC2018-095328-BI00(FEDER/Agencia estatal de investigación) and FSE-DGA2017-2019-E12/7R (Gobierno de Aragón/FEDER) (MINECO/FEDER), the EU through the ITN “Elusives” H2020-MSCA-ITN-2015/674896 and the Deutsche Forschungsgemeinschaft under grant SFB-1258 as a Mercator Fellow. CPG was supported by PROMETEO II/2014/050 of Generalitat Valenciana, FPA2014-57816-P of MINECO and by the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreements 690575 and 674896. AM is supported by the European Research Council under Grant No. 742104.

Published
2021

3. Conceptual design of BabyIAXO, the intermediate stage towards the International Axion Observatory

Author

The IAXO collaboration, A. Abeln, K. Altenmüller, S. Arguedas Cuendis, E. Armengaud, D. Attié, S. Aune, S. Basso, L. Bergé, B. Biasuzzi, P. T. C. Borges De Sousa, P. Brun, N. Bykovskiy, D. Calvet, J. M. Carmona, J. F. Castel, S. Cebrián, V. Chernov, F. E. Christensen, M. M. Civitani, C. Cogollos, T. Dafní, A. Derbin, K. Desch, D. Díez, M. Dinter, B. Döbrich, I. Drachnev, A. Dudarev, L. Dumoulin, D. D. M. Ferreira, E. Ferrer-Ribas, I. Fleck, J. Galán, D. Gascón, L. Gastaldo, M. Giannotti, Y. Giomataris, A. Giuliani, S. Gninenko, J. Golm, N. Golubev, L. Hagge, J. Hahn, C. J. Hailey, D. Hengstler, P. L. Henriksen, T. Houdy, R. Iglesias-Marzoa, F. J. Iguaz, I. G. Irastorza, C. Iñiguez, K. Jakovčić, J. Kaminski, B. Kanoute, S. Karstensen, L. Kravchuk, B. Lakić, T. Lasserre, P. Laurent, O. Limousin, A. Lindner, M. Loidl, I. Lomskaya, G. López-Alegre, B. Lubsandorzhiev, K. Ludwig, G. Luzón, C. Malbrunot, C. Margalejo, A. Marin-Franch, S. Marnieros, F. Marutzky, J. Mauricio, Y. Menesguen, M. Mentink, S. Mertens, F. Mescia, J. Miralda-Escudé, H. Mirallas, J. P. Mols, V. Muratova, X. F. Navick, C. Nones, A. Notari, A. Nozik, L. Obis, C. Oriol, F. Orsini, A. Ortiz de Solórzano, S. Oster, H. P. Pais Da Silva, V. Pantuev, T. Papaevangelou, G. Pareschi, K. Perez, O. Pérez, E. Picatoste, M. J. Pivovaroff, D. V. Poda, J. Redondo, A. Ringwald, M. Rodrigues, F. Rueda-Teruel, S. Rueda-Teruel, E. Ruiz-Choliz, J. Ruz, E. O. Saemann, J. Salvado, T. Schiffer, S. Schmidt, U. Schneekloth, M. Schott, L. Segui, F. Tavecchio, H. H. J. ten Kate, I. Tkachev, S. Troitsky, D. Unger, E. Unzhakov, N. Ushakov, J. K. Vogel, D. Voronin, A. Weltman, U. Werthenbach, W. Wuensch, and A. Yanes-Díaz

Subjects
Beyond Standard Model, Dark matter, CP violation, Other experiments, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract This article describes BabyIAXO, an intermediate experimental stage of the International Axion Observatory (IAXO), proposed to be sited at DESY. IAXO is a large-scale axion helioscope that will look for axions and axion-like particles (ALPs), produced in the Sun, with unprecedented sensitivity. BabyIAXO is conceived to test all IAXO subsystems (magnet, optics and detectors) at a relevant scale for the final system and thus serve as prototype for IAXO, but at the same time as a fully-fledged helioscope with relevant physics reach itself, and with potential for discovery. The BabyIAXO magnet will feature two 10 m long, 70 cm diameter bores, and will host two detection lines (optics and detector) of dimensions similar to the final ones foreseen for IAXO. BabyIAXO will detect or reject solar axions or ALPs with axion-photon couplings down to g aγ ∼ 1.5 × 10 −11 GeV −1, and masses up to m a ∼ 0.25 eV. BabyIAXO will offer additional opportunities for axion research in view of IAXO, like the development of precision x-ray detectors to identify particular spectral features in the solar axion spectrum, and the implementation of radiofrequency-cavity-based axion dark matter setups.

Published
2021
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4. First results of the CAST-RADES haloscope search for axions at 34.67 μeV

Author

A. Álvarez Melcón, S. Arguedas Cuendis, J. Baier, K. Barth, H. Bräuninger, S. Calatroni, G. Cantatore, F. Caspers, J. F. Castel, S. A. Cetin, C. Cogollos, T. Dafni, M. Davenport, A. Dermenev, K. Desch, A. Díaz-Morcillo, B. Döbrich, H. Fischer, W. Funk, J. D. Gallego, J. M. García Barceló, A. Gardikiotis, J. G. Garza, B. Gimeno, S. Gninenko, J. Golm, M. D. Hasinoff, D. H. H. Hoffmann, I. G. Irastorza, K. Jakovčić, J. Kaminski, M. Karuza, B. Lakić, J. M. Laurent, A. J. Lozano-Guerrero, G. Luzón, C. Malbrunot, M. Maroudas, J. Miralda-Escudé, H. Mirallas, L. Miceli, P. Navarro, A. Ozbey, K. Özbozduman, C. Peña Garay, M. J. Pivovaroff, J. Redondo, J. Ruz, E. Ruiz Chóliz, S. Schmidt, M. Schumann, Y. K. Semertzidis, S. K. Solanki, L. Stewart, I. Tsagris, T. Vafeiadis, J. K. Vogel, E. Widmann, W. Wuensch, and K. Zioutas

Subjects
Dark matter, Dark Matter and Double Beta Decay (experiments), Exotics, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract We present results of the Relic Axion Dark-Matter Exploratory Setup (RADES), a detector which is part of the CERN Axion Solar Telescope (CAST), searching for axion dark matter in the 34.67 μeV mass range. A radio frequency cavity consisting of 5 sub-cavities coupled by inductive irises took physics data inside the CAST dipole magnet for the first time using this filter-like haloscope geometry. An exclusion limit with a 95% credibility level on the axion-photon coupling constant of g aγ ≳ 4 × 10 −13 GeV −1 over a mass range of 34.6738 μeV < m a < 34.6771 μeV is set. This constitutes a significant improvement over the current strongest limit set by CAST at this mass and is at the same time one of the most sensitive direct searches for an axion dark matter candidate above the mass of 25 μeV. The results also demonstrate the feasibility of exploring a wider mass range around the value probed by CAST-RADES in this work using similar coherent resonant cavities.

Published
2021
Full Text
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