New gamma ray signal from gravitationally boosted neutralinos at the galactic center
Autor: | Cannoni, M., Gomez, M. E., Perez-Garcia, M. A., Vergados, J. D. |
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Rok vydání: | 2012 |
Předmět: | |
Zdroj: | Phys. Rev. D 85, 115015 (2012) |
Druh dokumentu: | Working Paper |
DOI: | 10.1103/PhysRevD.85.115015 |
Popis: | 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. Comment: 5 pages, 3 figures |
Databáze: | arXiv |
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