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Search for Solar Axions by the CERN Axion Solar Telescope with 3He Buffer Gas : Closing the Hot Dark Matter Gap (CROSBI ID 204925)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

Arik, M. ; Aune, S. ; Barth, K. ; Belov, A. ; Borghi, S. ; Bräuninger, H. ; Cantatore, G. ; Carmona, J.M. ; Cetin, S.A. ; Collar, J.I. et al. Search for Solar Axions by the CERN Axion Solar Telescope with 3He Buffer Gas : Closing the Hot Dark Matter Gap // Physical review letters, 112 (2014), 091302-1-091302-6. doi: 10.1103/PhysRevLett.112.091302

Podaci o odgovornosti

Arik, M. ; Aune, S. ; Barth, K. ; Belov, A. ; Borghi, S. ; Bräuninger, H. ; Cantatore, G. ; Carmona, J.M. ; Cetin, S.A. ; Collar, J.I. ; Da Riva, E. ; Dafni, T. ; Davenport, M. ; Eleftheriadis, C. ; Elias, N. ; Fanourakis, G. ; Ferrer-Ribas, E. ; Friedrich, P. ; Galán, J. ; García, J.A. ; Gardikiotis, A. ; Garza, J.G. ; Gazis, E.N. ; Geralis, T. ; Georgiopoulou, E. ; Giomataris, I. ; Gninenko, S. ; Gómez, H. ; Gómez Marzoa, M. ; Gruber, E. ; Guthörl, T. ; Hartmann, R. ; Hauf, S. ; Haug, F. ; Hasinoff, M.D. ; Hoffmann, D.H.H. ; Iguaz, F.J. ; Irastorza, I.G. ; Jacoby, J. ; Jakovčić, Krešimir ; Karuza, Marin ; Königsmann, K. ; Kotthaus, R. ; Krčmar, Milica ; Kuster, M. ; Lakić, Biljana ; Lang, P.M. ; Laurent, J.M. ; Liolios, A. ; Ljubičić, Ante ; Luzón, G. ; Neff, S. ; Niinikoski, T. ; Nordt, A. ; Papaevangelou, T. ; Pivovaroff, M.J. ; Raffelt, G. ; Riege, H. ; Rodríguez, A. ; Rosu, M. ; Ruz, J. ; Savvidis, I. ; Shilon, I. ; Silva, P.S. ; Solanki, S.K. ; Stewart, L. ; Tomás, A. ; Tsagri, M. ; van Bibber, K. ; Vafeiadis, T. ; Villar, J. ; Vogel, J.K. ; Yildiz, S.C. ; Zioutas, K.

engleski

Search for Solar Axions by the CERN Axion Solar Telescope with 3He Buffer Gas : Closing the Hot Dark Matter Gap

The CERN Axion Solar Telescope has finished its search for solar axions with 3He buffer gas, covering the search range 0.64 eV < m_a < 1.17 eV. This closes the gap to the cosmological hot dark matter limit and actually overlaps with it. 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 < 3.3×10^(−10) GeV^(−1) at 95% C.L., with the exact value depending on the pressure setting. Future direct solar axion searches will focus on increasing the sensitivity to smaller values of g_aγ, for example by the currently discussed next generation helioscope International AXion Observatory.

solar axions; photons; dark matter

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Podaci o izdanju

112

2014.

091302-1-091302-6

objavljeno

0031-9007

10.1103/PhysRevLett.112.091302

Povezanost rada

Fizika

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