Thermal relics in hidden sectors

Dark matter may be hidden, with no standard model gauge interactions. At the same time, in WIMPless models (WIMP: weakly interacting massive particles) with hidden matter masses proportional to hidden gauge couplings squared, the hidden dark matter's thermal relic density may naturally be in th...

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Bibliographic Details
Published inJournal of cosmology and astroparticle physics Vol. 2008; no. 10; p. 043
Main Authors Feng, Jonathan L, Tu, Huitzu, Yu, Hai-Bo
Format Journal Article
LanguageEnglish
Published United States IOP Publishing 01.10.2008
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