@Article{Farzan+Palomares-Ruiz2014,
author="Farzan, Y.
and Palomares-Ruiz, S.",
title="Dips in the diffuse supernova neutrino background",
journal="Journal of Cosmology and Astroparticle Physics",
year="2014",
publisher="Iop Publishing Ltd",
volume="06",
number="6",
pages="014--21pp",
optkeywords="dark matter theory; supernova neutrinos; cosmological neutrinos",
abstract="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.",
optnote="WOS:000346407200014",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=2046), last updated on Thu, 08 Jan 2015 16:40:24 +0000",
issn="1475-7516",
doi="10.1088/1475-7516/2014/06/014",
opturl="http://arxiv.org/abs/1401.7019",
opturl="https://doi.org/10.1088/1475-7516/2014/06/014",
archivePrefix="arXiv",
eprint="1401.7019",
language="English"
}