Gravitinos and a Low Ultimate Temperature for the Early Universe
arXiv:hep-th/9404044 · doi:10.1016/0370-2693(94)91254-8
Abstract
We obtain new stronger bounds by orders of magnitude, on the ultimate temperature of the universe by exploiting the copious production of gravitinos at finite temperature.
14 PAGES (3 figs. as separate uuencoded file) UTTG-04-94 Change in estimate
References in corpus (2)
Cited by in corpus (17)
- Baryogenesis from Flat Directions of the Supersymmetric Standard Model
- Big Bang nucleosynthesis and physics beyond the Standard Model
- Thermal Inflation and the Moduli Problem
- Thermal production of gravitinos
- Cosmology with a TeV mass GUT Higgs
- Solving the Cosmological Moduli Problem with Weak Scale Inflation
- On the Thermal Regeneration Rate for Light Gravitinos in the Early Universe
- Successful Supersymmetric Inflation
- Reheating of the universe after inflation with f(phi)R gravity
- Gravitino Decay into a Neutrino and a Sneutrino in the Inflationary Universe
- Supersymmetry, Finite Temperature and Gravitino Production in the Early Universe
- False Vacuum Inflation with a Quartic Potential
- Moduli Inflation from Dynamical Supersymmetry Breaking
- Supersymmetry and SU(2)xU(1) breaking with naturally vanishing vacuum energy
- Constraints on Supergravity Chaotic Inflationary Models
- Gravitino production in a thermal Universe revisited
- Inflation and Generalized O'Raifeartaigh SUSY models