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The CERN Axion Solar Telescope (CAST)

dc.contributor.authorFanourakis, G
dc.contributor.authorSampieto, M
dc.contributor.authorSarsa, M
dc.contributor.authorSavvidis, I
dc.contributor.authorStipcevic, M
dc.contributor.authorThomas, CW
dc.contributor.authorThompson, RC
dc.contributor.authorValco, P
dc.contributor.authorVillar, JA
dc.contributor.authorVillierme, B
dc.contributor.authorWalckiers, L
dc.contributor.authorWilcox, W
dc.contributor.authorZachariadou, K
dc.contributor.authorZioutas, K
dc.contributor.authorCelebi, G
dc.contributor.authorGolubev, NA
dc.contributor.authorHasinoff, M
dc.contributor.authorHoffmann, D
dc.contributor.authorIrastorza, IG
dc.contributor.authorJacoby, J
dc.contributor.authorJeanneau, F
dc.contributor.authorKnopf, MA
dc.contributor.authorKovzelev, AV
dc.contributor.authorKotthaus, R
dc.contributor.authorKrcmar, M
dc.contributor.authorKrecak, Z
dc.contributor.authorLakic, B
dc.contributor.authorAalseth, CE
dc.contributor.authorArik, E
dc.contributor.authorAutiero, D
dc.contributor.authorAvignone, FT
dc.contributor.authorBarth, K
dc.contributor.authorBowyer, SM
dc.contributor.authorBrauninger, H
dc.contributor.authorBrodzinski, RL
dc.contributor.authorCarmona, JM
dc.contributor.authorCebrian, S
dc.contributor.authorCetin, S
dc.contributor.authorCollar, JI
dc.contributor.authorCreswick, R
dc.contributor.authorDelbart, A
dc.contributor.authorDelattre, M
dc.contributor.authorDiLella, L
dc.contributor.authorDe Oliveira, R
dc.contributor.authorEleftheriadis, C
dc.contributor.authorErdutan, N
dc.contributor.authorFarach, HA
dc.contributor.authorFiorini, C
dc.contributor.authorGeralis, T
dc.contributor.authorGiomataris, I
dc.contributor.authorGirard, TA
dc.contributor.authorGninenko, SN
dc.contributor.authorLiolios, A
dc.contributor.authorLjubicic, A
dc.contributor.authorLutz, G
dc.contributor.authorLongoni, A
dc.contributor.authorLuzon, G
dc.contributor.authorMailov, A
dc.contributor.authorMatveev, VA
dc.contributor.authorMiley, HS
dc.contributor.authorMorales, A
dc.contributor.authorMorales, J
dc.contributor.authorMutterer, M
dc.contributor.authorNikolaidis, A
dc.contributor.authorNussinov, S
dc.contributor.authorOrtiz, A
dc.contributor.authorPitts, WK
dc.contributor.authorPlacci, A
dc.contributor.authorPostoev, VE
dc.contributor.authorRaffelt, GG
dc.contributor.authorRiege, H
dc.date.accessioned2021-03-05T10:34:44Z
dc.date.available2021-03-05T10:34:44Z
dc.identifier.citationAalseth C., Arik E., Autiero D., Avignone F., Barth K., Bowyer S., Brauninger H., Brodzinski R., Carmona J., Cebrian S., et al., "The CERN Axion Solar Telescope (CAST)", NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, cilt.110, ss.85-87, 2002
dc.identifier.issn0920-5632
dc.identifier.othervv_1032021
dc.identifier.otherav_a3d1e718-3e78-47c4-b67c-3dd78391f122
dc.identifier.urihttp://hdl.handle.net/20.500.12627/109654
dc.identifier.urihttp://www.sciencedirect.com/science/article/pii/S0920563202014597
dc.identifier.urihttps://doi.org/10.1016/s0920-5632(02)01459-7
dc.description.abstractA decommissioned LHC test magnet is being prepared as the CERN Axion Solar Telescope (CAST) experiment. The magnet has a field of 9.6 Tesla and length of 10 meters. It is being mounted on a platform to track the sun over +/-8(0) vertically and +/-45(0), horizontally. A sensitivity in axion-photon coupling g(agammagamma) < 5 x 10(-11)GeV(-1) can be reached for m(a) less than or equal to 10(-2) eV, and with a gas filled tube-can reach g(agammagamma) less than or equal to 10(-10)GeV(-1) for axion masses m(a) < 2eV.
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectFİZİK, PARTİKLER VE ALANLAR
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectTemel Parçacıklar ve Alanlar
dc.titleThe CERN Axion Solar Telescope (CAST)
dc.typeMakale
dc.relation.journalNUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS
dc.contributor.department, ,
dc.identifier.volume110
dc.identifier.startpage85
dc.identifier.endpage87
dc.contributor.firstauthorID727979


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