Chaotic Dark Matter
arXiv:astro-ph/9205005 · doi:10.1103/PhysRevD.46.3350
Abstract
A very weakly coupled scalar field with mass and initial vacuum expectation value will provide enough mass to close the universe provided $V\simeq (3\times 10^8\gev)(100\gev/m)^{1/4}$. We discuss possible models in which such a field could arise.
5 pages