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Asymmetric Dark Matter: Theories, signatures, and constraints

2013/08/31 by Kathryn M. Zurek · 10 citations
Physics and Astronomy · #Asymmetry #COSMIC cancer database #Collider #Cosmic background radiation #Cosmic microwave background #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Pulsars and Gravitational Waves Research #astro-ph.CO #astro-ph.HE #hep-ph

paper · pdf · doi:10.1016/j.physrep.2013.12.001

69 pages, 12 figures. Invited Review for Physics Reports. v2: added references, updated to reflect published version

arxiv created 2013/11/19 · openalex publication_date 2013/12/12 · arxiv updated 2015/06/16 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

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.

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