Dips in the diffuse supernova neutrino background

被引:48
|
作者
Farzan, Yasaman [1 ]
Palomares-Ruiz, Sergio [2 ]
机构
[1] Inst Res Fundamental Sci IPM, Sch Phys, Tehran, Iran
[2] Univ Valencia, CSIC, Inst Fis Corpuscular IFIC, E-46071 Valencia, Spain
关键词
dark matter theory; supernova neutrinos; cosmological neutrinos; HUGE MISSING MASS; RELIC NEUTRINOS; ABSORPTION; EVOLUTION; SPECTRUM; SEARCH;
D O I
10.1088/1475-7516/2014/06/014
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Scalar (fermion) dark matter with mass in the MeV range coupled to ordinary neutrinos and another fermion (scalar) is motivated by scenarios that establish a link between radiatively generated neutrino masses and the dark matter relic density. With such a coupling, cosmic supernova neutrinos, on their way to us, could resonantly interact with the background (lark matter particles, giving rise to a dip in their redshift-integrated spectra. Current and future neutrino detectors, such as Super-Kamiokande. LENA and HyperKamiokande, could be able to detect this distortion.
引用
收藏
页数:21
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