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We study the indirect detection of dark matter when the local dark matter velocity distribution depends upon position, as expected for the Milky Way and its dwarf spheroidal satellites, and the annihilation cross-section is not purely s-wave.
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N. Arkani-Hamed, D. P. Finkbeiner, T. R. Slatyer, and N. Weiner, A Theory of Dark Matter, Phys.Rev
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D. Hooper and T. Linden, On The Origin Of The Gamma Rays From The Galactic Center, Phys.Rev
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J. Diemand and B. Moore, The structure and evolution of cold dark matter halos, Adv.Sci.Lett
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