Chaotic Dark Matter
天体物理学
2009-10-22 v1
摘要
A very weakly coupled scalar field with mass and initial vacuum expectation value will provide enough mass to close the universe provided . We discuss possible models in which such a field could arise.
引用
@article{arxiv.astro-ph/9205005,
title = {Chaotic Dark Matter},
author = {R. Rangarajan and M. Srednicki},
journal= {arXiv preprint arXiv:astro-ph/9205005},
year = {2009}
}
备注
5 pages