Chaotic Dark Matter
classification
🌌 astro-ph
keywords
fieldmassarisechaoticclosecoupleddarkdiscuss
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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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