CaltechAUTHORS
Published March 15, 2012 | Version Published + Accepted Version
Journal Article Open

Symmetric and asymmetric light dark matter

Creators

  • 1. ROR icon Harvard University
  • 2. ROR icon University of Michigan–Ann Arbor

Abstract

We examine cosmological, astrophysical and collider constraints on thermal dark matter (DM) with mass

Additional Information

© 2012 American Physical Society. (Received 26 November 2011; published 5 March 2012) We thank Doug Finkbeiner, Manoj Kaplinghat, Lisa Randall, Brian Shuve, Tracy Slatyer, Luca Vecchi, and Tomer Volansky for useful discussions. H. B. Y. and T. L. thank the Theory Division of CERN, and H. B. Y. and K. M. Z. thank the Aspen Center for Physics where part of the work was done. The work of T. L. was partially supported by NASA Theory Program Grant No. NNX10AD85G. The work of H. B. Y. and K. M. Z. was supported by NASA Theory Program Grant No. NNX11AI17G and by NSF CAREER award PHY 1049896.

Attached Files

Published - PhysRevD.85.063503.pdf

Accepted Version - 1111.0293.pdf

Files

1111.0293.pdf

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Additional details

Additional titles

Alternative title
On Symmetric and Asymmetric Light Dark Matter

Identifiers

Eprint ID
96398
Resolver ID
CaltechAUTHORS:20190613-164147504

Related works

Describes
https://arxiv.org/abs/1111.0293 (URL)

Funding

NASA
NNX10AD85G
NASA
NNX11AI17G
NSF
PHY-1049896

Dates

Created
2019-06-14
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Physics Department