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Enhancement of Line Gamma Ray Signature from Bino-like Dark Matter Annihilation due to CP Violation

Shigeki Matsumoto·Joe Sato·Yoshio Sato
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Abstract

We study the line gamma ray signature from the Galactic Center originating from Bino-like dark matter pair annihilation, when CP is not conserved. We consider the case that the Bino is nearly degenerate with a sfermion in mass. Although an indirect detection of Bino-like dark matter is difficult in general, the signal of Bino-like dark matter pair annihialtion in this case is enormously enhanced due to the threshold singularity.

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Shigeki Matsumoto, Joe Sato, Yoshio Sato. 2005-08-04. Enhancement of Line Gamma Ray Signature from Bino-like Dark Matter Annihilation due to CP Violation. https://arxiv.org/abs/hep-ph/0505160

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