Ultra-high energy cosmic rays from annihilation of superheavy dark matter

Details Ultra-high energy cosmic rays from annihilation of superheavy dark matter Ultra-high energy cosmic rays from annihilation of superheavy dark matter

2001-05-14

arxiv.org/abs/astro-ph/0105232v3

Astropart.Phys.18:57-66,2002

Astronomy and Astrophysics

Astrophysics

13 pages, 4 figures, to appear in Astropart. Phys

Scientific paper

We consider the possibility that ultra-high energy cosmic rays originate from the annihilation of relic superheavy dark-matter particles. We find that a cross section of ~ 10^{-26}cm^2 (M_X/10^{12}GeV)^{3/2} is required to account for the observed rate of super-GZK events if the superheavy dark matter follows a Navarro-Frenk-White density profile. This would require extremely large-l contributions to the annihilation cross section. We also calculate the possible signature from annihilation in sub-galactic clumps of dark matter and find that the signal from sub-clumps dominates and may explain the observed flux with a much smaller cross section than if the superheavy dark matter is smoothly distributed. Finally, we discuss the expected anisotropy in the arrival directions of the cosmic rays, which is a characteristic signature of this scenario.

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