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REVIEW OF ASYMMETRIC DARK MATTER

Nikhef, Science Park 105, 1098 XG Amsterdam, The Netherlands

and

ARC Centre of Excellence for Particle Physics at the Terascale, School of Physics, The University of Melbourne, Victoria 3010, Australia

Corresponding author.

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https://doi.org/10.1142/S0217751X13300287Cited by:342

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 bounds, and touches on direct detection prospects and collider signatures.

Keywords:

PACS: 98.80.Cq, 12.60.-i

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Vol. 28, No. 19

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Received 14 June 2013

Accepted 17 June 2013

Published: 30 July 2013

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REVIEW OF ASYMMETRIC DARK MATTER

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