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We delineate the allowed parameter and mass range for a wino-like dark matter particle containing some Higgsino admixture in the MSSM by analysing the constraints from diffuse gamma-rays from the dwarf spheroidal galaxies, galactic cosmic rays, direct detection and cosmic microwave background anisotropies.
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M. Beneke, C. Hellmann and P. Ruiz-Femenia, Non-relativistic pair annihilation of nearly mass degenerate neutralinos and charginos I. General framework and S-wave annihilation
2013
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2015
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G. Giesen, M. Boudaud, Y. Génolini, V. Poulin, M. Cirelli, P. Salati and P. D. Serpico, AMS-02 antiprotons, at last! Secondary astrophysical component and immediate implications for Dark Matter
2015
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2015
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M. Beneke, A. Bharucha, F. Dighera, C. Hellmann, A. Hryczuk, S. Recksiegel and P. Ruiz-Femenia, Relic density of wino-like dark matter in the MSSM
2016
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P. Ullio and M. Valli, A critical reassessment of particle Dark Matter limits from dwarf satellites
2016
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