Search for solar axions: the CAST experiment at CERN (CROSBI ID 131864)
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Podaci o odgovornosti
Andriamonje, S. ; Arsov, V. ; Aune, S. ; Autiero, D. ; Avignone, F. ; Barth, K. ; Belov, A. ; Beltran, B. ; Braeuninger, H. ; Carmona, J. M. ; Cebrian, S. ; Chesi, E. ; Collar, J. I. ; Creswick, R. ; Dafni, T. ; Davenport, M. ; Di Lela, 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. ; Koenigsmann, K. ; Kotthaus, R. ; Krčmar, Milica ; Kousouris, K. ; Kuster, M. ; Lakić, Biljana ; Lasseur, C. ; Liolios, A. ; Ljubičić, Ante ; Lutz, G. ; Luzon, G. ; Miller, D. W. ; 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.
engleski
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 helioscope in order to search for these axion-like particles. The analysis of the 2003 data [1] has shown no signal above the background, thus implying an upper limit to the axion-photon coupling of g(alpha gamma) < 1.16 x 10(-10) GeV-1 at 95% CL for m(alpha) less than or similar to 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 approximate to 1 eV.
solar axions; dark matter; low background
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