Journal
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS
Volume 537, Issue 3, Pages 91-121Publisher
ELSEVIER
DOI: 10.1016/j.physrep.2013.12.001
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Funding
- DoE [desc0007859]
- NSF CAREER award [PHY 1049896]
- NASA Astrophysics Theory grant [NNX11AI17G]
- Direct For Mathematical & Physical Scien
- Division Of Physics [1049896] Funding Source: National Science Foundation
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We review theories of Asymmetric Dark Matter (ADM), their cosmological implications and detection. While there are many models of ADM in the literature, our review of existing models will center on highlighting the few common features and important mechanisms for generation and transfer of the matter anti-matter asymmetry between dark and visible sectors. We also survey ADM hidden sectors, the calculation of the relic abundance for ADM, and how the DM asymmetry may be erased at late times through oscillations. We consider cosmological constraints on ADM from the cosmic microwave background, neutron stars, the Sun, and brown and white dwarves. Lastly, we review indirect and direct detection methods for ADM, collider signatures, and constraints. (c) 2014 Elsevier B.V. All rights reserved.
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