Sneutrino condensate as a candidate for the hot big bang cosmology

Mazumdar, Anupam and Pérez-Lorenzana, A. (2004) Sneutrino condensate as a candidate for the hot big bang cosmology. Physical Review D, 70 (8): 083526. ISSN 1550-7998

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If inflationary paradigm is correct, then it must create conditions for the hot big bang model with all observed matter, baryons and the seed perturbations for the structure formation. In this paper we propose a scenario where the inflaton energy density is dumped into the bulk in a brane world setup, and all the required physical conditions are created by the right handed neutrino sector within supersymmetry. The scalar component of the right handed Majorana neutrino is responsible for generating the scale invariant fluctuations in the cosmic microwave background radiation, reheating the Universe at a temperature~$T_{rh}\leq 10^{9}$ GeV, and finally generating the lepton/baryon asymmetry, $n_{B}/s\sim 10^{-10}$, with no lepton/baryon isocurvature fluctuations.

Item Type:
Journal Article
Journal or Publication Title:
Physical Review D
Additional Information:
© 2004 The American Physical Society 19 pages, 3 figures. Some discussion on neutrino masses and baryogenesis, and other small changes added
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Deposited On:
01 May 2013 13:28
Last Modified:
15 Jul 2024 13:45