作者
V Anastassopoulos, S Aune, K Barth, A Belov, G Cantatore, JM Carmona, JF Castel, SA Cetin, F Christensen, JI Collar, T Dafni, M Davenport, TA Decker, A Dermenev, K Desch, C Eleftheriadis, G Fanourakis, E Ferrer-Ribas, H Fischer, JA Garcia, A Gardikiotis, JG Garza, EN Gazis, T Geralis, I Giomataris, S Gninenko, CJ Hailey, MD Hasinoff, DHH Hoffmann, FJ Iguaz, IG Irastorza, A Jakobsen, J Jacoby, K Jakovcic, J Kaminski, M Karuza, N Kralj, M Krcmar, S Kostoglou, Ch Krieger, B Lakic, JM Laurent, A Liolios, A Ljubicic, G Luzón, M Maroudas, L Miceli, S Neff, I Ortega, T Papaevangelou, K Paraschou, MJ Pivovaroff, G Raffelt, M Rosu, J Ruz, E Ruiz Chóliz, I Savvidis, S Schmidt, YK Semertzidis, SK Solanki, L Stewart, T Vafeiadis, JK Vogel, SC Yildiz, K Zioutas, CAST collaboration
发表日期
2017/5/5
期刊
arXiv preprint arXiv:1705.02290
简介
During 2003--2015, the CERN Axion Solar Telescope (CAST) has searched for conversion in the 9 T magnetic field of a refurbished LHC test magnet that can be directed toward the Sun. In its final phase of solar axion searches (2013--2015), CAST has returned to evacuated magnet pipes, which is optimal for small axion masses. The absence of a significant signal above background provides a world leading limit of (95% C.L.) on the axion-photon coupling strength for eV. Compared with the first vacuum phase (2003--2004), the sensitivity was vastly increased with low-background x-ray detectors and a new x-ray telescope. These innovations also serve as pathfinders for a possible next-generation axion helioscope.
学术搜索中的文章
V Anastassopoulos, S Aune, K Barth, A Belov… - arXiv preprint arXiv:1705.02290, 2017