| Literature DB >> 22243149 |
M Arik1, S Aune, K Barth, A Belov, S Borghi, H Bräuninger, G Cantatore, J M Carmona, S A Cetin, J I Collar, T Dafni, M Davenport, C Eleftheriadis, N Elias, C Ezer, G Fanourakis, E Ferrer-Ribas, P Friedrich, J Galán, J A García, A Gardikiotis, E N Gazis, T Geralis, I Giomataris, S Gninenko, H Gómez, E Gruber, T Guthörl, R Hartmann, F Haug, M D Hasinoff, D H H Hoffmann, F J Iguaz, I G Irastorza, J Jacoby, K Jakovčić, M Karuza, K Königsmann, R Kotthaus, M Krčmar, M Kuster, B Lakić, J M Laurent, A Liolios, A Ljubičić, V Lozza, G Lutz, G Luzón, J Morales, T Niinikoski, A Nordt, T Papaevangelou, M J Pivovaroff, G Raffelt, T Rashba, H Riege, A Rodríguez, M Rosu, J Ruz, I Savvidis, P S Silva, S K Solanki, L Stewart, A Tomás, M Tsagri, K van Bibber, T Vafeiadis, J A Villar, J K Vogel, S C Yildiz, K Zioutas.
Abstract
The CERN Axion Solar Telescope (CAST) has extended its search for solar axions by using (3)He as a buffer gas. At T=1.8 K this allows for larger pressure settings and hence sensitivity to higher axion masses than our previous measurements with (4)He. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39 eV≲m(a)≲0.64 eV. From the absence of excess x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g(aγ)≲2.3×10(-10) GeV(-1) at 95% C.L., the exact value depending on the pressure setting. Kim-Shifman-Vainshtein-Zakharov axions are excluded at the upper end of our mass range, the first time ever for any solar axion search. In the future we will extend our search to m(a)≲1.15 eV, comfortably overlapping with cosmological hot dark matter bounds.Entities:
Year: 2011 PMID： 22243149 DOI： 10.1103/PhysRevLett.107.261302
Source DB: PubMed Journal: Phys Rev Lett ISSN： 0031-9007 Impact factor: 9.161