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Stability, reheating and leptogenesis

2019/03/20 by Djuna Croon, Nicolas Fernandez, Croon, Djuna +5 · 2 citations
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph

paper · pdf · doi:10.48550/arxiv.1903.08658

18 pages 3 figures, JHEP version DOI: 10.1007/JHEP06(2019)098

arxiv created 2019/08/01 · arxiv updated 2019/08/02

Abstract

In a minimal model of leptogenesis, the observed baryon asymmetry is realized after high-scale reheating into the lightest sterile neutrino. We consider constraints on this scenario from the stability of the Higgs vacuum during pre-heating. Depending on the reheat temperature, the lightest sterile neutrino may be in or out of thermal equilibrium at production. Demanding stability of the Higgs vacuum during pre-heating, we find strong constraints which primarily impact the parameter space of thermal leptogenesis.

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