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Search for sub-eV mass solar axions by the CERN axion solar telescope with He3 buffer gas

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dc.contributor.author Arik, M en
dc.contributor.author Aune, S en
dc.contributor.author Barth, K en
dc.contributor.author Belov, A en
dc.contributor.author Borghi, S en
dc.contributor.author Brauninger, H en
dc.contributor.author Cantatore, G en
dc.contributor.author Carmona, JM en
dc.contributor.author Cetin, SA en
dc.contributor.author Collar, JI en
dc.contributor.author Dafni, T en
dc.contributor.author Davenport, M en
dc.contributor.author Eleftheriadis, C en
dc.contributor.author Elias, N en
dc.contributor.author Ezer, C en
dc.contributor.author Fanourakis, G en
dc.contributor.author Ferrer-Ribas, E en
dc.contributor.author Friedrich, P en
dc.contributor.author Galan, J en
dc.contributor.author Garcia, JA en
dc.contributor.author Gardikiotis, A en
dc.contributor.author Gazis, EN en
dc.contributor.author Geralis, T en
dc.contributor.author Giomataris, I en
dc.contributor.author Gninenko, S en
dc.contributor.author Gomez, H en
dc.contributor.author Gruber, E en
dc.contributor.author Guthorl, T en
dc.contributor.author Hartmann, R en
dc.contributor.author Haug, F en
dc.contributor.author Hasinoff, MD en
dc.contributor.author Hoffmann, DHH en
dc.contributor.author Iguaz, FJ en
dc.contributor.author Irastorza, IG en
dc.contributor.author Jacoby, J en
dc.contributor.author Jakovcic, K en
dc.contributor.author Karuza, M en
dc.contributor.author Konigsmann, K en
dc.contributor.author Kotthaus, R en
dc.contributor.author Krcmar, M en
dc.contributor.author Kuster, M en
dc.contributor.author Lakic, B en
dc.contributor.author Laurent, JM en
dc.contributor.author Liolios, A en
dc.contributor.author Ljubicic, A en
dc.contributor.author Lozza, V en
dc.contributor.author Lutz, G en
dc.contributor.author Luzon, G en
dc.contributor.author Morales, J en
dc.contributor.author Niinikoski, T en
dc.contributor.author Nordt, A en
dc.contributor.author Papaevangelou, T en
dc.contributor.author Pivovaroff, MJ en
dc.contributor.author Raffelt, G en
dc.contributor.author Rashba, T en
dc.contributor.author Riege, H en
dc.contributor.author Rodriguez, A en
dc.contributor.author Rosu, M en
dc.contributor.author Ruz, J en
dc.contributor.author Savvidis, I en
dc.contributor.author Silva, PS en
dc.contributor.author Solanki, SK en
dc.contributor.author Stewart, L en
dc.contributor.author Tomas, A en
dc.contributor.author Tsagri, M en
dc.contributor.author Van Bibber, K en
dc.contributor.author Vafeiadis, T en
dc.contributor.author Villar, JA en
dc.contributor.author Vogel, JK en
dc.contributor.author Yildiz, SC en
dc.contributor.author Zioutas, K en
dc.date.accessioned 2014-03-01T02:03:53Z
dc.date.available 2014-03-01T02:03:53Z
dc.date.issued 2011 en
dc.identifier.issn 00319007 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/29379
dc.subject.other Buffer gas en
dc.subject.other CERN axion solar telescopes en
dc.subject.other Hot dark matter en
dc.subject.other Physical societies en
dc.subject.other Pressure settings en
dc.subject.other Solar axions en
dc.subject.other Upper limits en
dc.subject.other Upper-end en
dc.subject.other Bosons en
dc.subject.other Helium en
dc.subject.other Optical telescopes en
dc.subject.other Telescopes en
dc.title Search for sub-eV mass solar axions by the CERN axion solar telescope with He3 buffer gas en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevLett.107.261302 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevLett.107.261302 en
heal.identifier.secondary 261302 en
heal.publicationDate 2011 en
heal.abstract The CERN Axion Solar Telescope (CAST) has extended its search for solar axions by using He3 as a buffer gas. At T=1.8K this allows for larger pressure settings and hence sensitivity to higher axion masses than our previous measurements with He4. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39eVma0.64eV. 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 gaγ2.3×10-10GeV-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 ma1.15eV, comfortably overlapping with cosmological hot dark matter bounds. Published by the American Physical Society under the terms of the http://creativecommons.org/licenses/by/3.0/Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. en
heal.journalName Physical Review Letters en
dc.identifier.doi 10.1103/PhysRevLett.107.261302 en
dc.identifier.volume 107 en
dc.identifier.issue 26 en


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