Pregled bibliografske jedinice broj: 537217
Search for sub-eV mass solar axions by the CERN Axion Solar Telescope with 3He buffer gas
Search for sub-eV mass solar axions by the CERN Axion Solar Telescope with 3He buffer gas // Physical Review Letters, 107 (2011), 26; 261302-1 doi:10.1103/PhysRevLett.107.261302 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 537217 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Search for sub-eV mass solar axions by the CERN Axion Solar Telescope with 3He buffer gas
Autori
Arik, M. ; Aune, S. ; Barth, K. ; Belov, A. ; Borghi, S. ; Brauninger, H. ; Cantatore, G. ; Carmona, J.M. ; Cetin, S.A. ; Collar, J.I. ; Dafni, T. ; Davenport, M. ; Eleftheriadis, C. ; Elias, N. ; Ezer, C. ; Fanourakis, G. ; Ferrer-Ribas, E. ; Friedrich, P. ; Galan, J. ; Garcia, J.A. ; Gardikiotis, A. ; Gazis, E.N. ; Geralis, T. ; Giomataris, I. ; Gninenko, S. ; Gomez, H. ; Gruber, E. ; Guthorl, T. ; Hartmann, R. ; Haug, F. ; Hasinoff, M.D. ; Hoffmann, H.H. ; Iguaz, F.J. ; Irastorza, I.G. ; Jacoby, J. ; Jakovčić, Krešimir ; Karuza, Marin ; Konigsmann, K. ; Kotthaus, R. ; Krčmar, Milica ; Kuster, M. ; Lakić, Biljana ; Laurent, J.M. ; Liolios, A. ; Ljubičić, Ante ; Lozza, V. ; Lutz, G. ; Luzon, G. ; Morales, J. ; Niinikoski, T. ; Nordt, A. ; Papaevangelou, T. ; Pivovaroff, M.J. ; Raffelt, G. ; Rashba, T. ; Riege, H. ; Rodriguez, A. ; Rosu, M. ; Ruz, J. ; Savvidis, I. ; Silva, P.S. ; Solanki, S.K. ; Stewart, L. ; Tomas, A. ; Tsagri, M. ; van Bibber, K. ; Vafeiadis, T. ; Villar, J. ; Vogel, K. ; Yildiz, S.C. ; Zioutas, K.
Izvornik
Physical Review Letters (0031-9007) 107
(2011), 26;
261302-1
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
solar axions; photons; dark matter
Sažetak
The CERN Axion Solar Telescope (CAST) has extended its search for solar axions by using 3He 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 4He. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39 eV <_ ma<_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 ga <_2.3×10−10 GeV−1 at 95% CL, the exact value depending on the pressure setting. KSVZ axions are excluded at the upper end of our mass range, the first time ever for any solar axion search. In future we will extend our search to ma <_1.15 eV, comfortably overlapping with cosmological hot dark matter bounds.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
098-0982887-2872 - Masivni neutrini i astročestice: od fizike čestica do kozmologije (Ljubičić, Ante, MZOS ) ( CroRIS)
Ustanove:
Institut "Ruđer Bošković", Zagreb
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus
- MEDLINE