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High Energy Physics - Phenomenology

arXiv:1305.4939 (hep-ph)
[Submitted on 21 May 2013 (v1), last revised 1 Aug 2013 (this version, v3)]

Title:Review of asymmetric dark matter

Authors:Kalliopi Petraki, Raymond R. Volkas
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Abstract:Asymmetric dark matter models are based on the hypothesis that the present-day abundance of dark matter has the same origin as the abundance of ordinary or visible matter: an asymmetry in the number densities of particles and antiparticles. They are largely motivated by the observed similarity in the mass densities of dark and visible matter, with the former observed to be about five times the latter. This review discusses the construction of asymmetric dark matter models, summarizes cosmological and astrophysical implications and bounds, and touches on direct detection prospects and collider signatures.
Comments: Invited review for the International Journal of Modern Physics A. Published version, 60 pages
Subjects: High Energy Physics - Phenomenology (hep-ph); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Astrophysical Phenomena (astro-ph.HE)
Report number: NIKHEF-2013-016
Cite as: arXiv:1305.4939 [hep-ph]
  (or arXiv:1305.4939v3 [hep-ph] for this version)
  https://doi.org/10.48550/arXiv.1305.4939
Journal reference: Int. J. Mod. Phys. A 28, 1330028 (2013)
Related DOI: https://doi.org/10.1142/S0217751X13300287

Submission history

From: Kalliopi Petraki [view email]
[v1] Tue, 21 May 2013 20:00:07 UTC (76 KB)
[v2] Thu, 13 Jun 2013 16:01:39 UTC (83 KB)
[v3] Thu, 1 Aug 2013 08:24:44 UTC (83 KB)
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