A Cosmological Upper Bound on Superpartner Masses
Hall, Lawrence J. · Ruderman, Joshua T. · Volansky, Tomer
الأصل · EN
If some superpartners were in thermal equilibrium in the early universe, and if the lightest superpartner is a cosmologically stable gravitino, then there is a powerful upper bound on the scale of the superpartner masses. Typically the bound is below tens of TeV, often much lower, and has similar parametrics to the WIMP miracle.
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