Published March 15, 2012
| Published + Accepted Version
Journal Article
Open
Symmetric and asymmetric light dark matter
- Creators
-
Lin, Tongyan
- Yu, Hai-Bo
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Zurek, Kathryn M.
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
PhysRevD.85.063503.pdf
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Additional details
- Alternative title
- On Symmetric and Asymmetric Light Dark Matter
- Eprint ID
- 96398
- Resolver ID
- CaltechAUTHORS:20190613-164147504
- NNX10AD85G
- NASA
- NNX11AI17G
- NASA
- PHY-1049896
- NSF
- Created
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2019-06-14Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field