_version_ 1866916506691960832
author CAST Collaboration
Altenmüller, K.
Anastassopoulos, V.
Arguedas-Cuendis, S.
Aune, S.
Baier, J.
Barth, K.
Bräuninger, H.
Cantatore, G.
Caspers, F.
Castel, J. F.
Çetin, S. A.
Christensen, F.
Cogollos, C.
Dafni, T.
Davenport, M.
Decker, T. A.
Desch, K.
Díez-Ibáñez, D.
Döbrich, B.
Ferrer-Ribas, E.
Fischer, H.
Funk, W.
Galán, J.
García, J. A.
Gardikiotis, A.
Giomataris, I.
Golm, J.
Hailey, C. H.
Hasinoff, M. D.
Hoffmann, D. H. H.
Irastorza, I. G.
Jacoby, J.
Jakobsen, A. C.
Jakovčić, K.
Kaminski, J.
Karuza, M.
Kostoglou, S.
Krieger, C.
Lakić, B.
Laurent, J. M.
Luzón, G.
Malbrunot, C.
Margalejo, C.
Maroudas, M.
Miceli, L.
Mirallas, H.
Navarro, P.
Obis, L.
Özbey, A.
Özbozduman, K.
Papaevangelou, T.
Pérez, O.
Pivovaroff, M. J.
Rosu, M.
Ruiz-Chóliz, E.
Ruz, J.
Schmidt, S.
Schumann, M.
Semertzidis, Y. K.
Solanki, S. K.
Stewart, L.
Vafeiadis, T.
Vogel, J. K.
Zioutas, K.
author_facet CAST Collaboration
Altenmüller, K.
Anastassopoulos, V.
Arguedas-Cuendis, S.
Aune, S.
Baier, J.
Barth, K.
Bräuninger, H.
Cantatore, G.
Caspers, F.
Castel, J. F.
Çetin, S. A.
Christensen, F.
Cogollos, C.
Dafni, T.
Davenport, M.
Decker, T. A.
Desch, K.
Díez-Ibáñez, D.
Döbrich, B.
Ferrer-Ribas, E.
Fischer, H.
Funk, W.
Galán, J.
García, J. A.
Gardikiotis, A.
Giomataris, I.
Golm, J.
Hailey, C. H.
Hasinoff, M. D.
Hoffmann, D. H. H.
Irastorza, I. G.
Jacoby, J.
Jakobsen, A. C.
Jakovčić, K.
Kaminski, J.
Karuza, M.
Kostoglou, S.
Krieger, C.
Lakić, B.
Laurent, J. M.
Luzón, G.
Malbrunot, C.
Margalejo, C.
Maroudas, M.
Miceli, L.
Mirallas, H.
Navarro, P.
Obis, L.
Özbey, A.
Özbozduman, K.
Papaevangelou, T.
Pérez, O.
Pivovaroff, M. J.
Rosu, M.
Ruiz-Chóliz, E.
Ruz, J.
Schmidt, S.
Schumann, M.
Semertzidis, Y. K.
Solanki, S. K.
Stewart, L.
Vafeiadis, T.
Vogel, J. K.
Zioutas, K.
contents Hypothetical axions provide a compelling explanation for dark matter and could be emitted from the hot solar interior. The CERN Axion Solar Telescope (CAST) has been searching for solar axions via their back conversion to X-ray photons in a 9-T 10-m long magnet directed towards the Sun. We report on an extended run with the IAXO (International Axion Observatory) pathfinder detector, doubling the previous exposure time. The detector was operated with a xenon-based gas mixture for part of the new run, providing technical insights for future detector configurations in IAXO. No counts are detected in the 95% signal-encircling region during the new run, while 0.75 are expected. The new data improve the axion-photon coupling limit to 5.8$\times 10^{-11}\,$GeV$^{-1}$ at 95% C.L. (for $m_a \lesssim 0.02$ eV), the most restrictive experimental limit to date.
format Preprint
id arxiv_https___arxiv_org_abs_2406_16840
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle A new upper limit on the axion-photon coupling with an extended CAST run with a Xe-based Micromegas detector
CAST Collaboration
Altenmüller, K.
Anastassopoulos, V.
Arguedas-Cuendis, S.
Aune, S.
Baier, J.
Barth, K.
Bräuninger, H.
Cantatore, G.
Caspers, F.
Castel, J. F.
Çetin, S. A.
Christensen, F.
Cogollos, C.
Dafni, T.
Davenport, M.
Decker, T. A.
Desch, K.
Díez-Ibáñez, D.
Döbrich, B.
Ferrer-Ribas, E.
Fischer, H.
Funk, W.
Galán, J.
García, J. A.
Gardikiotis, A.
Giomataris, I.
Golm, J.
Hailey, C. H.
Hasinoff, M. D.
Hoffmann, D. H. H.
Irastorza, I. G.
Jacoby, J.
Jakobsen, A. C.
Jakovčić, K.
Kaminski, J.
Karuza, M.
Kostoglou, S.
Krieger, C.
Lakić, B.
Laurent, J. M.
Luzón, G.
Malbrunot, C.
Margalejo, C.
Maroudas, M.
Miceli, L.
Mirallas, H.
Navarro, P.
Obis, L.
Özbey, A.
Özbozduman, K.
Papaevangelou, T.
Pérez, O.
Pivovaroff, M. J.
Rosu, M.
Ruiz-Chóliz, E.
Ruz, J.
Schmidt, S.
Schumann, M.
Semertzidis, Y. K.
Solanki, S. K.
Stewart, L.
Vafeiadis, T.
Vogel, J. K.
Zioutas, K.
High Energy Physics - Experiment
Hypothetical axions provide a compelling explanation for dark matter and could be emitted from the hot solar interior. The CERN Axion Solar Telescope (CAST) has been searching for solar axions via their back conversion to X-ray photons in a 9-T 10-m long magnet directed towards the Sun. We report on an extended run with the IAXO (International Axion Observatory) pathfinder detector, doubling the previous exposure time. The detector was operated with a xenon-based gas mixture for part of the new run, providing technical insights for future detector configurations in IAXO. No counts are detected in the 95% signal-encircling region during the new run, while 0.75 are expected. The new data improve the axion-photon coupling limit to 5.8$\times 10^{-11}\,$GeV$^{-1}$ at 95% C.L. (for $m_a \lesssim 0.02$ eV), the most restrictive experimental limit to date.
title A new upper limit on the axion-photon coupling with an extended CAST run with a Xe-based Micromegas detector
topic High Energy Physics - Experiment
url https://arxiv.org/abs/2406.16840