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dc.contributor.authorÇetin, Serkant Ali
dc.contributor.authorCAST Collaboration
dc.date.accessioned2015-11-18T14:40:59Z
dc.date.available2015-11-18T14:40:59Z
dc.date.issued2008
dc.identifier.citationLakic, B., Arık, E., Aune, S., Autiero, D., Barth, K., Belov, A. ... CAST Collaboration. (2008). Search for solar axions with the CAST experiment. In Identification of dark matter 2008 (pp. 1-6). Trieste, Italy: Proceedings of Science, SISSA.en_US
dc.identifier.uri1824-8039
dc.identifier.urihttp://hdl.handle.net/11376/2203
dc.descriptionÇetin, Serkant Ali (Dogus Author) -- Conference full title: Identification of dark matter 2008 : idm2008, August 18-22, 2008, Stockholm, Swedenen_US
dc.description.abstractThe CERN Axion Solar Telescope (CAST) is searching for axions produced by the Primakoff process in the solar core. CAST is using a dipole magnet where axions could be converted back into X-rays. Phase I data analysis resulted in the most restrictive experimental limit on the axion-photon coupling constant for ma ≲ 0.02 eV In CAST Phase II, the sensitivity is extended to higher axion masses. Results of the analysis of 2005 and 2006 data, covering the range ma ≲ 0.4 eV, will be presented. Currently CAST is searching for axions with masses up to 1.2 eV.en_US
dc.language.isoengen_US
dc.publisherSISSAen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectCERN Axion Solar Telescopesen_US
dc.subjectCoupling Constantsen_US
dc.subjectDipole Magnetsen_US
dc.subjectPhase Ien_US
dc.subjectPhase IIen_US
dc.subjectSolar Axionsen_US
dc.titleSearch for solar axions with the CAST experimenten_US
dc.typeconferenceObjecten_US
dc.relation.journalProceedings of IDM2008en_US
dc.contributor.departmentDoğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümüen_US
dc.contributor.authorIDTR3959en_US
dc.identifier.startpage1en_US
dc.identifier.endpage6en_US


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