Journal
PHYSICAL REVIEW D
Volume 89, Issue 10, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.89.105015
Keywords
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Funding
- DFG [SFB TR 33]
- ERC grant BSMOXFORD [228169]
- U.S. Department of Energy [DE-SC0010137]
- U.S. National Science Foundation [PHY-1342611]
- Division Of Physics
- Direct For Mathematical & Physical Scien [1342611] Funding Source: National Science Foundation
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Theories with dark forces and dark sectors are of interest for dark matter models. In this paper we find the region in parameter space that is constrained by supernova cooling constraints when the models include dark sector particles with masses around 100 MeV or less. We include only interactions with electrons and positrons. The constraint is important for small mixing parameters. We do not include in this work interactions with nucleons, which could give other important constraints.
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