期刊
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
卷 -, 期 7, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2009/07/020
关键词
dark matter theory; X-ray telescopes; gamma ray theory; gamma ray experiments
资金
- US Department of Energy, Office of Science, High Energy Physics [DEFG02-04ER41268]
- NASA [NNX08AV72G]
- NSF [PHY-0757911]
- Direct For Mathematical & Physical Scien [757911] Funding Source: National Science Foundation
- Division Of Physics [757911] Funding Source: National Science Foundation
- NASA [94122, NNX08AV72G] Funding Source: Federal RePORTER
We calculate the extragalactic diffuse emission originating from the up-scattering of cosmic microwave photons by energetic electrons and positrons produced in particle dark matter annihilation events at all redshifts and in all halos. We outline the observational constraints on this emission and we study its dependence on both the particle dark matter model (including the particle mass and its dominant annihilation final state) and on assumptions on structure formation and on the density profile of halos. We find that for low-mass dark matter models, data in the X-ray band provide the most stringent constraints, while the gamma-ray energy range probes models featuring large masses and pair-annihilation rates, and a hard spectrum for the injected electrons and positrons. Specifically, we point out that the all-redshift, all-halo inverse Compton emission from many dark matter models that might provide an explanation to the anomalous positron fraction measured by the Pamela payload severely overproduces the observed extragalactic gamma-ray background.
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