Supersymmetry and primordial black hole abundance constraints
نویسنده
چکیده
and MBH is the PBH mass in grams. The standard picture of PBH evaporation is that all particles which appear elementary at the energy scale of the PBH and have rest mass less than TBH are emitted directly [3]. For instance PBHs with TBH above the QCD quark-hadron transition scale ΛQH ≈ 250− 300 MeV, emit relativistic quark and gluon jets which then fragment into photons, leptons and hadrons as in high energy accelerator collisions. The mass loss, in grams per second, is given by
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