_version_ 1866908493962805248
author 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.
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.
Schiffer, T.
Schmidt, S.
Schumann, M.
Semertzidis, Y. K.
Solanki, S. K.
Stewart, L.
Vafeiadis, T.
Vogel, J. K.
Zioutas, K.
author_facet 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.
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.
Schiffer, T.
Schmidt, S.
Schumann, M.
Semertzidis, Y. K.
Solanki, S. K.
Stewart, L.
Vafeiadis, T.
Vogel, J. K.
Zioutas, K.
contents We present a search for solar axions produced through the axion-electron coupling $(g_{ae})$ using data from a novel 7-GridPix detector installed at the CERN Axion Solar Telescope (CAST). The detector, featuring ultra-thin silicon nitride windows and multiple veto systems, collected approximately 160 hours of solar tracking data between 2017-2018. Using machine learning techniques and the veto systems, we achieved a background rate of $1.06\times 10^{-5}\,\text{keV}^{-1}\text{cm}^{-2}\text{s}^{-1}$ at a signal efficiency of about $80\,\%$ in the $0.2$-$8\,\text{keV}$ range. Analysis of the data yielded no significant excess above background, allowing us to set a new upper limit on the product of the axion-electron and axion-photon couplings of $g_{ae}\cdot g_{aγ} < 7.35\times 10^{-23}\,\text{GeV}^{-1}$ at $95\,\%$ confidence level. This result improves upon the previous best helioscope limit and demonstrates the potential of GridPix technology for rare event searches. Additionally, we derived a limit on the axion-photon coupling of $g_{aγ} < 9.0\times 10^{-11}\,\text{GeV}^{-1}$ at $95\,\%$ CL, which, while not surpassing CAST's best limit, provides complementary constraints on axion models.
format Preprint
id arxiv_https___arxiv_org_abs_2505_05909
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Search for solar axions produced through the axion-electron coupling $g_{ae}$ using a new GridPix detector at CAST
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.
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.
Schiffer, T.
Schmidt, S.
Schumann, M.
Semertzidis, Y. K.
Solanki, S. K.
Stewart, L.
Vafeiadis, T.
Vogel, J. K.
Zioutas, K.
High Energy Physics - Experiment
We present a search for solar axions produced through the axion-electron coupling $(g_{ae})$ using data from a novel 7-GridPix detector installed at the CERN Axion Solar Telescope (CAST). The detector, featuring ultra-thin silicon nitride windows and multiple veto systems, collected approximately 160 hours of solar tracking data between 2017-2018. Using machine learning techniques and the veto systems, we achieved a background rate of $1.06\times 10^{-5}\,\text{keV}^{-1}\text{cm}^{-2}\text{s}^{-1}$ at a signal efficiency of about $80\,\%$ in the $0.2$-$8\,\text{keV}$ range. Analysis of the data yielded no significant excess above background, allowing us to set a new upper limit on the product of the axion-electron and axion-photon couplings of $g_{ae}\cdot g_{aγ} < 7.35\times 10^{-23}\,\text{GeV}^{-1}$ at $95\,\%$ confidence level. This result improves upon the previous best helioscope limit and demonstrates the potential of GridPix technology for rare event searches. Additionally, we derived a limit on the axion-photon coupling of $g_{aγ} < 9.0\times 10^{-11}\,\text{GeV}^{-1}$ at $95\,\%$ CL, which, while not surpassing CAST's best limit, provides complementary constraints on axion models.
title Search for solar axions produced through the axion-electron coupling $g_{ae}$ using a new GridPix detector at CAST
topic High Energy Physics - Experiment
url https://arxiv.org/abs/2505.05909