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High energy photon flux prediction from neutralino annihilation in the globular cluster Palomar 13

E. Giraud·G. Meylan·M. Sapinski·A. Falvard·A. Jacholkowska·K. Jedamzik·J. Lavalle·E. Nuss·G. Moultaka·F. Piron·P. Salati·R. Taillet
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Abstract

The distant globular cluster Palomar 13 has been found to have a very high mass-to-light ratio and its profile can be well fitted either by a King model with a tail, or with a NFW model. This cluster may be the first case of the many clumps predicted by CDM simulations that would not be disrupted by the galactic halo potential. We make the hypothesis that Pal 13 is made of neutralinos and run the DarkSuspect code to estimate the high-energy photon flux due to the annihilation of neutralinos through various channels in some benchmark scenarios. These low fluxes may be used as targets to be reached in proposals for future ground-based high altitude Cerenkov telescopes.

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E. Giraud, G. Meylan, M. Sapinski, A. Falvard, A. Jacholkowska, K. Jedamzik, J. Lavalle, E. Nuss, G. Moultaka, F. Piron, P. Salati, R. Taillet. 2002-09-11. High energy photon flux prediction from neutralino annihilation in the globular cluster Palomar 13. https://doi.org/10.1007/10857580_49

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