A Cosmological Upper Bound on Superpartner Masses [PDF]
Lawrence J. Hall, Joshua T. Ruderman, Tomer VolanskyIf 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.View original: http://arxiv.org/abs/1302.2620
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