Search for solar axions with the CAST experiment

Biljana Lakic; E. Arik; S. Aune; D. Autiero; K. Barth; A. Belov; B. Beltrán; S. Borghi; G. Bourlis; F. S. Boydag; H. Bräuninger; J. M. Carmona; S. Cebrián; S. A. Cetin; J. I. Collar; T. Dafni; M. Davenport; L. Di Lella; O. B. Dogan; C. Eleftheriadis; N. Elias; G. Fanourakis; E. Ferrer-Ribas; H. Fischer; P. Friedrich; J. Franz; J. Galán; T. Geralis; I. Giomataris; S. Gninenko; H. Gómez; R. Hartmann; M. Hasinoff; F. H. Heinsius; I. Hikmet; D. H.H. Hoffmann; I. G. Irastorza; J. Jacoby; K. Jakovcic; D. Kang; K. Königsmann; R. Kotthaus; M. Krcmar; K. Kousouris; M. Kuster; C. Lasseur; A. Liolios; A. Ljubicic; G. Lutz; G. Luzón; D. Miller; J. Morales; T. Niinikoski; A. Nordt; A. Ortiz; T. Papaevangelou; M. J. Pivovaroff; A. Placci; G. Raffelt; H. Riege; A. Rodríguez; J. Ruz; I. Savvidis; Y. Semertzidis; P. Serpico; R. Soufli; L. Stewart; K. Van Bibber; J. Villar; J. Vogel; L. Walckiers; K. Zioutas

Search for solar axions with the CAST experiment

Biljana Lakic
, E. Arik
, S. Aune
, D. Autiero
, K. Barth
, A. Belov
, B. Beltrán
, S. Borghi
, G. Bourlis
, F. S. Boydag
, H. Bräuninger
, J. M. Carmona
, S. Cebrián
, S. A. Cetin
, J. I. Collar
, T. Dafni
, M. Davenport
, L. Di Lella
, O. B. Dogan
, C. Eleftheriadis

N. Elias, G. Fanourakis, E. Ferrer-Ribas, H. Fischer, P. Friedrich, J. Franz, J. Galán, T. Geralis, I. Giomataris, S. Gninenko, H. Gómez, R. Hartmann, M. Hasinoff, F. H. Heinsius, I. Hikmet, D. H.H. Hoffmann, I. G. Irastorza, J. Jacoby, K. Jakovcic, D. Kang, K. Königsmann, R. Kotthaus, M. Krcmar, K. Kousouris, M. Kuster, C. Lasseur, A. Liolios, A. Ljubicic, G. Lutz, G. Luzón, D. Miller, J. Morales, T. Niinikoski, A. Nordt, A. Ortiz, T. Papaevangelou, M. J. Pivovaroff, A. Placci, G. Raffelt, H. Riege, A. Rodríguez, J. Ruz, I. Savvidis, Y. Semertzidis, P. Serpico, R. Soufli, L. Stewart, K. Van Bibber, J. Villar, J. Vogel, L. Walckiers, K. Zioutas

Ruder Boskovic Institute
Dogus University
Centre d' Etudes Nucléaires de Saclay (CEA-Saclay)
CERN
Institute de Physique Nucléaire
Russian Academy of Sciences
University of Zaragoza
Queen's University Kingston
University of Glasgow
Hellenic Open University
Max Planck Institute for Extraterrestrial Physics
The University of Chicago
Scuola Normale Superiore di Pisa
Aristotle University of Thessaloniki
Demokritos National Centre for Scientific Research
University of Freiburg
University of British Columbia
Ruhr University Bochum
Technische Universität Darmstadt
Goethe University Frankfurt
Karlsruhe Institute of Technology
Max Planck Institute for Physics (Werner Heisenberg Institute)
Fermi National Accelerator Laboratory
Chem./Materials Science Directorate
University of Patras
Brookhaven National Laboratory

Research output: Contribution to journal › Conference article › peer-review

Abstract

The CERN Axion Solar Telescope (CAST) is searching for axions produced by the Primakoff process in the solar core. CAST is using a dipole magnet where axions could be converted back into X-rays. Phase I data analysis resulted in the most restrictive experimental limit on the axion-photon coupling constant for m_a ≲ 0.02 eV In CAST Phase II, the sensitivity is extended to higher axion masses. Results of the analysis of 2005 and 2006 data, covering the range m_a ≲ 0.4 eV, will be presented. Currently CAST is searching for axions with masses up to 1.2 eV.

Original language	English
Journal	Proceedings of Science
State	Published - 2008
Externally published	Yes
Event	Identification of Dark Matter 2008, IDM 2008 - Stockholm, Sweden Duration: 18 Aug 2008 → 22 Aug 2008

Cite this

@article{43dc5cf4281a4f8087a44b76e8a1f5f7,

title = "Search for solar axions with the CAST experiment",

abstract = "The CERN Axion Solar Telescope (CAST) is searching for axions produced by the Primakoff process in the solar core. CAST is using a dipole magnet where axions could be converted back into X-rays. Phase I data analysis resulted in the most restrictive experimental limit on the axion-photon coupling constant for ma ≲ 0.02 eV In CAST Phase II, the sensitivity is extended to higher axion masses. Results of the analysis of 2005 and 2006 data, covering the range ma ≲ 0.4 eV, will be presented. Currently CAST is searching for axions with masses up to 1.2 eV.",

author = "Biljana Lakic and E. Arik and S. Aune and D. Autiero and K. Barth and A. Belov and B. Beltr{\'a}n and S. Borghi and G. Bourlis and Boydag, \{F. S.\} and H. Br{\"a}uninger and Carmona, \{J. M.\} and S. Cebri{\'a}n and Cetin, \{S. A.\} and Collar, \{J. I.\} and T. Dafni and M. Davenport and \{Di Lella\}, L. and Dogan, \{O. B.\} and C. Eleftheriadis and N. Elias and G. Fanourakis and E. Ferrer-Ribas and H. Fischer and P. Friedrich and J. Franz and J. Gal{\'a}n and T. Geralis and I. Giomataris and S. Gninenko and H. G{\'o}mez and R. Hartmann and M. Hasinoff and Heinsius, \{F. H.\} and I. Hikmet and Hoffmann, \{D. H.H.\} and Irastorza, \{I. G.\} and J. Jacoby and K. Jakovcic and D. Kang and K. K{\"o}nigsmann and R. Kotthaus and M. Krcmar and K. Kousouris and M. Kuster and C. Lasseur and A. Liolios and A. Ljubicic and G. Lutz and G. Luz{\'o}n and D. Miller and J. Morales and T. Niinikoski and A. Nordt and A. Ortiz and T. Papaevangelou and Pivovaroff, \{M. J.\} and A. Placci and G. Raffelt and H. Riege and A. Rodr{\'i}guez and J. Ruz and I. Savvidis and Y. Semertzidis and P. Serpico and R. Soufli and L. Stewart and \{Van Bibber\}, K. and J. Villar and J. Vogel and L. Walckiers and K. Zioutas",

year = "2008",

language = "英语",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

note = "Identification of Dark Matter 2008, IDM 2008 ; Conference date: 18-08-2008 Through 22-08-2008",

}

Lakic, B, Arik, E, Aune, S, Autiero, D, Barth, K, Belov, A, Beltrán, B, Borghi, S, Bourlis, G, Boydag, FS, Bräuninger, H, Carmona, JM, Cebrián, S, Cetin, SA, Collar, JI, Dafni, T, Davenport, M, Di Lella, L, Dogan, OB, Eleftheriadis, C, Elias, N, Fanourakis, G, Ferrer-Ribas, E, Fischer, H, Friedrich, P, Franz, J, Galán, J, Geralis, T, Giomataris, I, Gninenko, S, Gómez, H, Hartmann, R, Hasinoff, M, Heinsius, FH, Hikmet, I, Hoffmann, DHH, Irastorza, IG, Jacoby, J, Jakovcic, K, Kang, D, Königsmann, K, Kotthaus, R, Krcmar, M, Kousouris, K, Kuster, M, Lasseur, C, Liolios, A, Ljubicic, A, Lutz, G, Luzón, G, Miller, D, Morales, J, Niinikoski, T, Nordt, A, Ortiz, A, Papaevangelou, T, Pivovaroff, MJ, Placci, A, Raffelt, G, Riege, H, Rodríguez, A, Ruz, J, Savvidis, I, Semertzidis, Y, Serpico, P, Soufli, R, Stewart, L, Van Bibber, K, Villar, J, Vogel, J, Walckiers, L & Zioutas, K 2008, 'Search for solar axions with the CAST experiment', Proceedings of Science.

TY - JOUR

T1 - Search for solar axions with the CAST experiment

AU - Lakic, Biljana

AU - Arik, E.

AU - Aune, S.

AU - Autiero, D.

AU - Barth, K.

AU - Belov, A.

AU - Beltrán, B.

AU - Borghi, S.

AU - Bourlis, G.

AU - Boydag, F. S.

AU - Bräuninger, H.

AU - Carmona, J. M.

AU - Cebrián, S.

AU - Cetin, S. A.

AU - Collar, J. I.

AU - Dafni, T.

AU - Davenport, M.

AU - Di Lella, L.

AU - Dogan, O. B.

AU - Eleftheriadis, C.

AU - Elias, N.

AU - Fanourakis, G.

AU - Ferrer-Ribas, E.

AU - Fischer, H.

AU - Friedrich, P.

AU - Franz, J.

AU - Galán, J.

AU - Geralis, T.

AU - Giomataris, I.

AU - Gninenko, S.

AU - Gómez, H.

AU - Hartmann, R.

AU - Hasinoff, M.

AU - Heinsius, F. H.

AU - Hikmet, I.

AU - Hoffmann, D. H.H.

AU - Irastorza, I. G.

AU - Jacoby, J.

AU - Jakovcic, K.

AU - Kang, D.

AU - Königsmann, K.

AU - Kotthaus, R.

AU - Krcmar, M.

AU - Kousouris, K.

AU - Kuster, M.

AU - Lasseur, C.

AU - Liolios, A.

AU - Ljubicic, A.

AU - Lutz, G.

AU - Luzón, G.

AU - Miller, D.

AU - Morales, J.

AU - Niinikoski, T.

AU - Nordt, A.

AU - Ortiz, A.

AU - Papaevangelou, T.

AU - Pivovaroff, M. J.

AU - Placci, A.

AU - Raffelt, G.

AU - Riege, H.

AU - Rodríguez, A.

AU - Ruz, J.

AU - Savvidis, I.

AU - Semertzidis, Y.

AU - Serpico, P.

AU - Soufli, R.

AU - Stewart, L.

AU - Van Bibber, K.

AU - Villar, J.

AU - Vogel, J.

AU - Walckiers, L.

AU - Zioutas, K.

PY - 2008

Y1 - 2008

N2 - The CERN Axion Solar Telescope (CAST) is searching for axions produced by the Primakoff process in the solar core. CAST is using a dipole magnet where axions could be converted back into X-rays. Phase I data analysis resulted in the most restrictive experimental limit on the axion-photon coupling constant for ma ≲ 0.02 eV In CAST Phase II, the sensitivity is extended to higher axion masses. Results of the analysis of 2005 and 2006 data, covering the range ma ≲ 0.4 eV, will be presented. Currently CAST is searching for axions with masses up to 1.2 eV.

AB - The CERN Axion Solar Telescope (CAST) is searching for axions produced by the Primakoff process in the solar core. CAST is using a dipole magnet where axions could be converted back into X-rays. Phase I data analysis resulted in the most restrictive experimental limit on the axion-photon coupling constant for ma ≲ 0.02 eV In CAST Phase II, the sensitivity is extended to higher axion masses. Results of the analysis of 2005 and 2006 data, covering the range ma ≲ 0.4 eV, will be presented. Currently CAST is searching for axions with masses up to 1.2 eV.

UR - https://www.scopus.com/pages/publications/84882430218

M3 - 会议文章

AN - SCOPUS:84882430218

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

T2 - Identification of Dark Matter 2008, IDM 2008

Y2 - 18 August 2008 through 22 August 2008

ER -

Search for solar axions with the CAST experiment

Abstract

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