%0 Journal Article
%T Dips in the diffuse supernova neutrino background
%A Farzan, Y.
%A Palomares-Ruiz, S.
%J Journal of Cosmology and Astroparticle Physics
%D 2014
%V 06
%N 6
%I Iop Publishing Ltd
%@ 1475-7516
%G English
%F Farzan+Palomares-Ruiz2014
%O WOS:000346407200014
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=2046), last updated on Thu, 08 Jan 2015 16:40:24 +0000
%X 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.
%K dark matter theory
%K supernova neutrinos
%K cosmological neutrinos
%R 10.1088/1475-7516/2014/06/014
%U http://arxiv.org/abs/1401.7019
%U https://doi.org/10.1088/1475-7516/2014/06/014
%P 014-21pp