On the graceful exit problem in warm inflation
General Relativity and Quantum Cosmology
2021-06-16 v2 Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
High Energy Physics - Theory
Abstract
A seemingly simple question, how does warm inflation exit gracefully?, has a more complex answer than in a cold paradigm. It has been highlighted here that whether warm inflation exits gracefully depends on three independent choices: The form of the potential, the choice of the warm inflation model (i.e., on the form of its dissipative coefficient) and the regime, of weak or strong dissipation, characterizing the warm inflation dynamics. Generic conditions on slow-roll parameters and several constraints on the different model parameters required for warm inflation to exit gracefully are derived.
Cite
@article{arxiv.2005.01122,
title = {On the graceful exit problem in warm inflation},
author = {Suratna Das and Rudnei O. Ramos},
journal= {arXiv preprint arXiv:2005.01122},
year = {2021}
}
Comments
8 pages, 4 figures, double column, v2: 12 pages, 5 figures, version matched with the published version in PRD