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Search for solar axions: the CAST experiment at CERN
Hypothetical axion-like particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field they would be transformed into X-rays with energies of a few keV. The CAST experiment at CERN is using a decommissioned LHC magnet as an axion heliosc...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2005
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/849134 |
_version_ | 1780906916446208000 |
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author | Beltran, Berta Andriamonje, S. Arsov, V. Aune, S. Autiero, D. Avignone, F. Barth, K. Belov, A. Brauninger, H. Carmona, J.M. Cebrian, S. Chesi, E. Collar, J.I. Creswick, R. Dafni, T. Davenport, M. Di Lella, L. Eleftheriadis, C. Englhauser, J. Fanourakis, G. Farach, H. Ferrer, E. Fischer, H. Franz, J. Friedrich, P. Geralis, T. Giomataris, I. Gninenko, S. Goloubev, N. Hartmann, R. Hasinoff, M.D. Heinsius, F.H. Hoffmann, D.H.H. Irastorza, I.G. Jacoby, J. Kang, D. Konigsmann, Kay Kotthaus, R. Krcmar, M. Kousouris, K. Kuster, M. Lakic, B. Lasseur, C. Liolios, A. Ljubicic, A. Lutz, G. Luzon, G. Miller, David Wilkins Morales, A. Morales, J. Mutterer, M. Nikolaidis, A. Ortiz, A. Papaevangelou, T. Placci, A. Raffelt, G. Ruz, J. Riege, H. Sarsa, M.L. Savvidis, I. Serber, W. Serpico, P. Semertzidis, Y. Stewart, L. Vieira, J.D. Villar, J. Walckiers, L. Zachariadou, K. Zioutas, K. |
author_facet | Beltran, Berta Andriamonje, S. Arsov, V. Aune, S. Autiero, D. Avignone, F. Barth, K. Belov, A. Brauninger, H. Carmona, J.M. Cebrian, S. Chesi, E. Collar, J.I. Creswick, R. Dafni, T. Davenport, M. Di Lella, L. Eleftheriadis, C. Englhauser, J. Fanourakis, G. Farach, H. Ferrer, E. Fischer, H. Franz, J. Friedrich, P. Geralis, T. Giomataris, I. Gninenko, S. Goloubev, N. Hartmann, R. Hasinoff, M.D. Heinsius, F.H. Hoffmann, D.H.H. Irastorza, I.G. Jacoby, J. Kang, D. Konigsmann, Kay Kotthaus, R. Krcmar, M. Kousouris, K. Kuster, M. Lakic, B. Lasseur, C. Liolios, A. Ljubicic, A. Lutz, G. Luzon, G. Miller, David Wilkins Morales, A. Morales, J. Mutterer, M. Nikolaidis, A. Ortiz, A. Papaevangelou, T. Placci, A. Raffelt, G. Ruz, J. Riege, H. Sarsa, M.L. Savvidis, I. Serber, W. Serpico, P. Semertzidis, Y. Stewart, L. Vieira, J.D. Villar, J. Walckiers, L. Zachariadou, K. Zioutas, K. |
author_sort | Beltran, Berta |
collection | CERN |
description | Hypothetical axion-like particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field they would be transformed into X-rays with energies of a few keV. The CAST experiment at CERN is using a decommissioned LHC magnet as an axion helioscope in order to search for these axion-like particles. The analysis of the 2003 data has shown no signal above the background, thus implying an upper limit to the axion-photon coupling < 1.16*10^{-10} GeV^{-1} at 95% CL for m_{a} <~ 0.02 eV. The stable operation of the experiment during 2004 data taking allow us to anticipate that this value will be improved. At the end of 2005 we expect to start with the so-called second phase of CAST, when the magnet pipes will be filled with a buffer gas so that the axion-photon coherence will be extended. In this way we will be able to search for axions with masses up to 1 eV. |
id | cern-849134 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2005 |
record_format | invenio |
spelling | cern-8491342023-03-14T17:16:04Zhttp://cds.cern.ch/record/849134engBeltran, BertaAndriamonje, S.Arsov, V.Aune, S.Autiero, D.Avignone, F.Barth, K.Belov, A.Brauninger, H.Carmona, J.M.Cebrian, S.Chesi, E.Collar, J.I.Creswick, R.Dafni, T.Davenport, M.Di Lella, L.Eleftheriadis, C.Englhauser, J.Fanourakis, G.Farach, H.Ferrer, E.Fischer, H.Franz, J.Friedrich, P.Geralis, T.Giomataris, I.Gninenko, S.Goloubev, N.Hartmann, R.Hasinoff, M.D.Heinsius, F.H.Hoffmann, D.H.H.Irastorza, I.G.Jacoby, J.Kang, D.Konigsmann, KayKotthaus, R.Krcmar, M.Kousouris, K.Kuster, M.Lakic, B.Lasseur, C.Liolios, A.Ljubicic, A.Lutz, G.Luzon, G.Miller, David WilkinsMorales, A.Morales, J.Mutterer, M.Nikolaidis, A.Ortiz, A.Papaevangelou, T.Placci, A.Raffelt, G.Ruz, J.Riege, H.Sarsa, M.L.Savvidis, I.Serber, W.Serpico, P.Semertzidis, Y.Stewart, L.Vieira, J.D.Villar, J.Walckiers, L.Zachariadou, K.Zioutas, K.Search for solar axions: the CAST experiment at CERNParticle Physics - ExperimentHypothetical axion-like particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field they would be transformed into X-rays with energies of a few keV. The CAST experiment at CERN is using a decommissioned LHC magnet as an axion helioscope in order to search for these axion-like particles. The analysis of the 2003 data has shown no signal above the background, thus implying an upper limit to the axion-photon coupling < 1.16*10^{-10} GeV^{-1} at 95% CL for m_{a} <~ 0.02 eV. The stable operation of the experiment during 2004 data taking allow us to anticipate that this value will be improved. At the end of 2005 we expect to start with the so-called second phase of CAST, when the magnet pipes will be filled with a buffer gas so that the axion-photon coherence will be extended. In this way we will be able to search for axions with masses up to 1 eV.Hypothetical axion-like particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field they would be transformed into X-rays with energies of a few keV. The CAST experiment at CERN is using a decommissioned LHC magnet as an axion helioscope in order to search for these axion-like particles. The analysis of the 2003 data has shown no signal above the background, thus implying an upper limit to the axion-photon coupling < $1.16*10^{-10} GeV^{-1}$ at 95% CL for $m_{a}$ <~ 0.02 eV. The stable operation of the experiment during 2004 data taking allow us to anticipate that this value will be improved. At the end of 2005 we expect to start with the so-called second phase of CAST, when the magnet pipes will be filled with a buffer gas so that the axion-photon coherence will be extended. In this way we will be able to search for axions with masses up to 1 eV.hep-ex/0507007oai:cds.cern.ch:8491342005-07-01 |
spellingShingle | Particle Physics - Experiment Beltran, Berta Andriamonje, S. Arsov, V. Aune, S. Autiero, D. Avignone, F. Barth, K. Belov, A. Brauninger, H. Carmona, J.M. Cebrian, S. Chesi, E. Collar, J.I. Creswick, R. Dafni, T. Davenport, M. Di Lella, L. Eleftheriadis, C. Englhauser, J. Fanourakis, G. Farach, H. Ferrer, E. Fischer, H. Franz, J. Friedrich, P. Geralis, T. Giomataris, I. Gninenko, S. Goloubev, N. Hartmann, R. Hasinoff, M.D. Heinsius, F.H. Hoffmann, D.H.H. Irastorza, I.G. Jacoby, J. Kang, D. Konigsmann, Kay Kotthaus, R. Krcmar, M. Kousouris, K. Kuster, M. Lakic, B. Lasseur, C. Liolios, A. Ljubicic, A. Lutz, G. Luzon, G. Miller, David Wilkins Morales, A. Morales, J. Mutterer, M. Nikolaidis, A. Ortiz, A. Papaevangelou, T. Placci, A. Raffelt, G. Ruz, J. Riege, H. Sarsa, M.L. Savvidis, I. Serber, W. Serpico, P. Semertzidis, Y. Stewart, L. Vieira, J.D. Villar, J. Walckiers, L. Zachariadou, K. Zioutas, K. Search for solar axions: the CAST experiment at CERN |
title | Search for solar axions: the CAST experiment at CERN |
title_full | Search for solar axions: the CAST experiment at CERN |
title_fullStr | Search for solar axions: the CAST experiment at CERN |
title_full_unstemmed | Search for solar axions: the CAST experiment at CERN |
title_short | Search for solar axions: the CAST experiment at CERN |
title_sort | search for solar axions: the cast experiment at cern |
topic | Particle Physics - Experiment |
url | http://cds.cern.ch/record/849134 |
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