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- W2094736812 abstract "Gravitino produced in the inflationary universe are studied. When the gravitino decays into a neutrino and a sneutrino, the emitted high energy neutrinos scatter off the background neutrinos and produce charged leptons (mainly electrons and positrons), which cause the electro-magnetic cascades and produce many soft photons. We obtain the spectra of the high energy neutrinos as well as the spectrum of the high energy photon by integrating a set of Boltzmann equations. Requiring these photons should not alter the abundances of the light elements (D, $^3$He, $^4$He) in the universe, we can set the stringent upperbound on the reheating temperature after the inflation. We find that $T_R lesssim (10^{10}-10^{12})$GeV for $m_{3/2}sim (100GEV - 1TEV)$, which is more stringent than the constraints in the previous works." @default.
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- W2094736812 date "1995-03-01" @default.
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- W2094736812 title "Gravitino decay into a neutrino and a sneutrino in the inflationary universe" @default.
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- W2094736812 doi "https://doi.org/10.1016/0370-2693(94)01644-r" @default.
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