Inflation, baryogenesis, and gravitino dark matter at ultralow reheat temperatures

Kazunori Kohri, Anupam Mazumdar, and Narendra Sahu
Phys. Rev. D 80, 103504 – Published 5 November 2009

Abstract

It is quite possible that the reheat temperature of the Universe is extremely low close to the scale of big bang nucleosynthesis, i.e. TR110MeV. At such low reheat temperatures generating matter, antimatter asymmetry and synthesizing dark matter particles are challenging issues which need to be addressed within a framework of beyond the standard model physics. In this paper we point out that a successful cosmology can emerge naturally provided the R-parity violating interactions are responsible for the excess in baryons over antibaryons and at the same time they can explain the longevity of dark matter with the right abundance.

  • Received 1 June 2009

DOI:https://doi.org/10.1103/PhysRevD.80.103504

©2009 American Physical Society

Authors & Affiliations

Kazunori Kohri1, Anupam Mazumdar1,2, and Narendra Sahu1

  • 1Physics Department, Lancaster University, Lancaster, LA1 4YB, United Kingdom
  • 2Niels Bohr Institute, Blegdamsvej-17, Copenhagen, DK-2100, Denmark

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Issue

Vol. 80, Iss. 10 — 15 November 2009

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