Inflation, baryogenesis and gravitino dark matter at ultra low reheat temperatures.

Kohri, Kazunori and Mazumdar, Anupam and Sahu, Narendra (2009) Inflation, baryogenesis and gravitino dark matter at ultra low reheat temperatures. Physical Review D, 80 (10). ISSN 1550-7998

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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. TR∼1–10 MeV. 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.

Item Type: Journal Article
Journal or Publication Title: Physical Review D
Additional Information: © 2009 The American Physical Society
Uncontrolled Keywords: /dk/atira/pure/researchoutput/libraryofcongress/qc
Subjects:
Departments: Faculty of Science and Technology > Physics
ID Code: 31504
Deposited By: Dr Anupam Mazumdar
Deposited On: 27 Jan 2010 15:29
Refereed?: Yes
Published?: Published
Last Modified: 19 Sep 2019 23:47
URI: https://eprints.lancs.ac.uk/id/eprint/31504

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