Non--Baryonic Dark Matter
天体物理学
2009-10-28 v1
摘要
The best particle candidates for non--baryonic cold dark matter are reviewed, namely, neutralino, axion, axino and Majoron. These particles are considered in the context of cosmological models with the restrictions given by the observed mass spectrum of large scale structures, data on clusters of galaxies, age of the Universe etc.
引用
@article{arxiv.astro-ph/9601188,
title = {Non--Baryonic Dark Matter},
author = {V. Berezinsky and A. Bottino and G. Mignola},
journal= {arXiv preprint arXiv:astro-ph/9601188},
year = {2009}
}
备注
Latex, 12 pages, espcrc2.sty, 6 figures included, appended as a uuencoded compressed tarred file. Invited talk at the TAUP95 workshop, presented by V. Berezinsky