Chaotic Dark Matter

Details Chaotic Dark Matter Chaotic Dark Matter

1992-05-09

arxiv.org/abs/astro-ph/9205005v1

Phys.Rev. D46 (1992) 3350-3351

Astronomy and Astrophysics

Astrophysics

5 pages

Scientific paper

10.1103/PhysRevD.46.3350

A very weakly coupled scalar field with mass $m$ and initial vacuum
expectation value $V$ 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.

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