Leptogenesis from -dominated early universe
arXiv:hep-ph/0109030 · doi:10.1103/PhysRevD.65.043512
Abstract
We investigate in detail the leptogenesis by the decay of coherent right-handed sneutrino having dominated the energy density of the early universe, which was originally proposed by HM and TY. Once the dominant universe is realized, the amount of the generated lepton asymmetry (and hence baryon asymmetry) is determined only by the properties of the right-handed neutrino, regardless of the history before it dominates the universe. Moreover, thanks to the entropy production by the decay of the right-handed sneutrino, thermally produced relics are sufficiently diluted. In particular, the cosmological gravitino problem can be avoided even when the reheating temperature of the inflation is higher than $10^{10}\GeV$, in a wide range of the gravitino mass $m_{3/2}\simeq 10\MeV$--$100\TeV$. If the gravitino mass is in the range $m_{3/2}\simeq 10\MeV$--$1\GeV$ as in the some gauge-mediated supersymmetry breaking models, the dark matter in our universe can be dominantly composed of the gravitino. Quantum fluctuation of the during inflation causes an isocurvature fluctuation which may be detectable in the future.
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