The properties of dark matter
General Physics
2011-04-14 v1
Abstract
Observations of density profiles of galaxies and clusters constrain the properties of dark matter. Formation of stable halos by collisional fluids with very low mass particles appears as the most probable interpretation, while halos formed by high mass particles, left over from a hot big bang, can scarcely explain the observed density distributions. Detection methods of dark matter are discussed.
Cite
@article{arxiv.1104.2525,
title = {The properties of dark matter},
author = {Ernst Fischer},
journal= {arXiv preprint arXiv:1104.2525},
year = {2011}
}
Comments
8 pages