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The annihilation cross section of TeV scale dark matter particles $\chi^0$ with electroweak charges into photons is affected by large quantum corrections due to Sudakov logarithms and the Sommerfeld effect.
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M. Bauer, T. Cohen, R. J. Hill and M. P. Solon, Soft Collinear Effective Theory for Heavy WIMP Annihilation
2015
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G. Ovanesyan, T. R. Slatyer and I. W. Stewart, Heavy Dark Matter Annihilation from Effective Field Theory
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M. Beneke, R. Szafron and K. Urban , work in preparation
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M. Beneke, A. Bharucha, A. Hryczuk, S. Recksiegel and P. Ruiz-Femenia, The last refuge of mixed wino-Higgsino dark matter
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M. Baumgart, T. Cohen, I. Moult, N. L. Rodd, T. R. Slatyer, M. P. Solon, I. W. Stewart and V. Vaidya, Resummed Photon Spectra for WIMP Annihilation
2018
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