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In the early Universe, any particle carrying a conserved quantum number and in chemical equilibrium with the thermal bath will unavoidably inherit a particle-antiparticle asymmetry.
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2011
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2012
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2014
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M. Low and L.-T. Wang, Neutralino dark matter at 14 TeV and 100 TeV
2014
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2014
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R. J. Hill and M. P. Solon, WIMP-nucleon scattering with heavy WIMP effective theory
2014
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2014
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N. F. Bell, S. Horiuchi and I. M. Shoemaker, Annihilating Asymmetric Dark Matter
2015
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