Search for Solar Axions Using Fe-57

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dc.creatorKrcmar, M.
dc.creatorKrecak, Z.
dc.creatorStipcevic, M.
dc.creatorLjubicic, A.
dc.creatorBradley, D. A.
dc.date1998-01-22
dc.date1998-10-08
dc.date.accessioned2026-07-07T10:34:32Z
dc.date.available2026-07-07T10:34:32Z
dc.descriptionWe have made a search for Fe-57 gamma rays of energy 14.4 keV induced by resonant absorption of monochromatic solar axions, as proposed by Moriyama. The proposed axions are suggested to be emitted from the Sun, in M1 transitions between the first, thermally excited state and the ground state of Fe-57. An upper limit on hadronic axion mass of 745 eV is obtained at the 95% confidence level, it being assumed that z=0.56 and S=0.5.
dc.description4 pages, latex, revtex source, 1 postscript figure included, Title revised, some references added and expanded discussion. Version accepted by Phys. Lett. B
dc.identifierhttps://arxiv.org/abs/nucl-ex/9801005
dc.identifierhttp://arxiv.org/abs/nucl-ex/9801005
dc.identifierPhys.Lett.B442:38,1998
dc.identifierdoi:10.1016/S0370-2693(98)01231-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179503
dc.subjectNuclear Experiment
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.titleSearch for Solar Axions Using Fe-57
dc.typetext

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