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...
Saved in:
Published in | Journal of cosmology and astroparticle physics Vol. 2008; no. 10; p. 043 |
---|---|
Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
United States
IOP Publishing
01.10.2008
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Be the first to leave a comment!