“School of Physic”
Back to Papers HomeBack to Papers of School of Physic
| Paper IPM / Physic / 13367 |
|
||||
| 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 dark matter particles, giving rise to a dip in their redshift-integrated spectra. Current and future neutrino detectors, such as Super-Kamiokande, LENA and Hyper-Kamiokande, could be able to detect this distortion.
Download TeX format |
|||||
| back to top | |||||
