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MeV dark matter: has it been detected?

Abstract:
We discuss the possibility that the recent detection of 511 keV gamma rays from the galactic bulge, as observed by INTEGRAL, is a consequence of low mass (1-100 MeV) particle dark matter annihilations. We discuss the type of halo profile favored by the observations as well as the size of the annihilation cross section needed to account for the signal. We find that such a scenario is consistent with the observed dark matter relic density and other constraints from astrophysics and particle physics.
Publication status:
Published

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Publisher copy:
10.1103/physrevlett.92.101301

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Journal:
Physical Review Letters More from this journal
Volume:
92
Issue:
10
Pages:
101301
Publication date:
2004-03-01
DOI:
EISSN:
1079-7114
ISSN:
0031-9007


Language:
English
Pubs id:
pubs:26295
UUID:
uuid:193c6fda-a8c8-4df8-a8c5-437d25594c0a
Local pid:
pubs:26295
Source identifiers:
26295
Deposit date:
2012-12-19
ARK identifier:

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