A New Dark Matter Candidate: Non-thermal Sterile Neutrinos
Abstract
We propose a new and unique dark matter candidate: eV to keV sterile neutrinos produced via lepton number-driven resonant MSW (Mikheyev-Smirnov-Wolfenstein) conversion of active neutrinos. The requisite lepton number asymmetries in any of the active neutrino flavors range from 10 to 10 of the photon number - well within primordial nucleosynthesis bounds. The unique feature here is that the adiabaticity condition of the resonance strongly favors the production of lower energy sterile neutrinos. The resulting non-thermal (cold) energy spectrum can cause these sterile neutrinos to revert to non-relativistic kinematics at an early epoch, so that free-streaming lengths at or below the dwarf galaxy scale are possible. Therefore, the main problem associated with light neutrino dark matter candidates can be circumvented in our model.
Keywords
Cite
@article{arxiv.astro-ph/9810076,
title = {A New Dark Matter Candidate: Non-thermal Sterile Neutrinos},
author = {Xiangdong Shi and George M. Fuller},
journal= {arXiv preprint arXiv:astro-ph/9810076},
year = {2009}
}
Comments
Latex 11 pages + 1 figure