Self-interacting dark matter from an SU(3)_L \otimes U(1)_N electroweak model
High Energy Physics - Phenomenology
2009-11-07 v5
Abstract
Recently has been showed that models which consider self-interacting particles as dark matter candidates can be able to account all the discrepancies between N-body simulations and astronomical observations of the galactic structure. In the present work we show that the 3-3-1-electroweak model can provide a realistic candidate to this kind of dark matter. This dark matter particle is not arbitrarily imposed and no new symmetry is need for to stabilize it.
Keywords
Cite
@article{arxiv.hep-ph/0209119,
title = {Self-interacting dark matter from an SU(3)_L \otimes U(1)_N electroweak model},
author = {Douglas Fregolente and Mauro D. Tonasse},
journal= {arXiv preprint arXiv:hep-ph/0209119},
year = {2009}
}
Comments
Final version published in PLB