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arXiv · 1205.1709

New gamma ray signal from gravitationally boosted neutralinos at the galactic center

M. Cannoni·M. E. Gomez·M. A. Perez-Garcia·J. D. Vergados
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Abstract

We discuss on the possibility that colliding dark matter particles in the form of neutralinos may be gravitationally boosted near the super-massive black hole at the galactic center so that they can have enough collision energy to annihilate into a stau pair. Since in some phenomenologically favored supersymmetric models the mass splitting between the neutralino and the lightest stau, one of the two scalar superpartners of the tau lepton, is a few GeVs, this channel may be allowed. In addition, staus can only decay into a tau lepton and another neutralino. We calculate the gamma-ray spectrum and flux generated by the tau pair discussing the observability of the obtained features.

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M. Cannoni, M. E. Gomez, M. A. Perez-Garcia, J. D. Vergados. 2012-06-23. New gamma ray signal from gravitationally boosted neutralinos at the galactic center. https://doi.org/10.1103/physrevd.85.115015

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