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タイトルSupernova Bounds on the Dark Photon Using Its Electromagnetic Decay
本文(外部サイト)http://hdl.handle.net/2060/20150012730
著者(英)Kazanas, Demos; Nussinov, Shmuel; Mohapatra, Rabindra N.; Teplitz, Vigdor L.; Zhang, Yongchao
著者所属(英)NASA Goddard Space Flight Center
発行日2014-11-13
言語eng
内容記述The hypothetical massive dark photon (gamma) which has kinetic mixing with the SM photon can decay electromagnetically to e+ e pairs if its mass m exceeds 2m(sub e), and otherwise into three SM photons. These decays yield cosmological and supernovae associated signatures. We briefly discuss these signatures, particularly in connection with the supernova SN1987A, and delineate the extra constraints that arise on the mass and mixing parameter of the dark photon. In particular, we find that for dark photon mass m(sub gamma') in the 5-20 MeV range arguments based on supernova 1987A observations lead to a bound on epsilon which is about 300 times stronger than the presently existing bounds based on energy loss arguments.
NASA分類Physics of Elementary Particles and Fields; Astrophysics
レポートNOGSFC-E-DAA-TN24032
権利Copyright, Distribution as joint owner in the copyright


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