English

Increasing Temperature toward the Completion of Reheating

Cosmology and Nongalactic Astrophysics 2021-06-10 v2 High Energy Physics - Phenomenology

Abstract

Reheating is a process where the energy density of a dominant component of the universe other than radiation, such as a matter component, is transferred into radiation. It is usually assumed that the temperature of the universe decreases due to cosmic expansion even during the reheating process, in which case the maximal temperature of the universe is much higher than the reheat temperature. We point out that the temperature of the universe during reheating may in fact increase in well-motivated scenarios. We derive the necessary conditions for the temperature to increase during reheating and discuss concrete examples involving a scalar field. We comment on implications for particle physics and cosmology due to an increasing temperature during reheating.

Keywords

Cite

@article{arxiv.2007.04328,
  title  = {Increasing Temperature toward the Completion of Reheating},
  author = {Raymond T. Co and Eric Gonzalez and Keisuke Harigaya},
  journal= {arXiv preprint arXiv:2007.04328},
  year   = {2021}
}

Comments

24 pages, 7 figures

R2 v1 2026-06-23T16:57:43.132Z