Supersymmetry breaking and loop corrections at the end of inflation
arXiv:hep-ph/9905208 · doi:10.1103/PhysRevD.62.023514
Abstract
We show that quantum corrections to the effective potential in supersymmetric hybrid inflation can be calculated all the way from the inflationary period - when the Universe is dominated by a false vacuum energy density - till the fields settle down to the global supersymmetric minimum of the potential. These are crucial for getting a continuous description of the evolution of the fields.
minor corrections; version to be published in Phys. Rev. D
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