TY  - JOUR
AU  - Farzan, Y.
AU  - Palomares-Ruiz, S.
PY  - 2014
DA  - 2014//
TI  - Dips in the diffuse supernova neutrino background
T2  - J. Cosmol. Astropart. Phys.
JO  - Journal of Cosmology and Astroparticle Physics
SP  - 014
EP  - 21pp
VL  - 06
IS  - 6
PB  - Iop Publishing Ltd
KW  - dark matter theory
KW  - supernova neutrinos
KW  - cosmological neutrinos
AB  - 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.
SN  - 1475-7516
UR  - http://arxiv.org/abs/1401.7019
UR  - https://doi.org/10.1088/1475-7516/2014/06/014
DO  - 10.1088/1475-7516/2014/06/014
LA  - English
N1  - WOS:000346407200014
ID  - Farzan+Palomares-Ruiz2014
ER  -