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Sneutrino condensate as a candidate for the hot big bang cosmology

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Sneutrino condensate as a candidate for the hot big bang cosmology. / Mazumdar, Anupam; Pérez-Lorenzana, A.
In: Physical Review D, Vol. 70, No. 8, 083526, 20.10.2004.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Mazumdar, A & Pérez-Lorenzana, A 2004, 'Sneutrino condensate as a candidate for the hot big bang cosmology', Physical Review D, vol. 70, no. 8, 083526. https://doi.org/10.1103/PhysRevD.70.083526

APA

Mazumdar, A., & Pérez-Lorenzana, A. (2004). Sneutrino condensate as a candidate for the hot big bang cosmology. Physical Review D, 70(8), Article 083526. https://doi.org/10.1103/PhysRevD.70.083526

Vancouver

Mazumdar A, Pérez-Lorenzana A. Sneutrino condensate as a candidate for the hot big bang cosmology. Physical Review D. 2004 Oct 20;70(8):083526. doi: 10.1103/PhysRevD.70.083526

Author

Mazumdar, Anupam ; Pérez-Lorenzana, A. / Sneutrino condensate as a candidate for the hot big bang cosmology. In: Physical Review D. 2004 ; Vol. 70, No. 8.

Bibtex

@article{19a96b8ba66341959a95fe5ca136b992,
title = "Sneutrino condensate as a candidate for the hot big bang cosmology",
abstract = "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.",
author = "Anupam Mazumdar and A. P{\'e}rez-Lorenzana",
note = "{\textcopyright} 2004 The American Physical Society 19 pages, 3 figures. Some discussion on neutrino masses and baryogenesis, and other small changes added",
year = "2004",
month = oct,
day = "20",
doi = "10.1103/PhysRevD.70.083526",
language = "English",
volume = "70",
journal = "Physical Review D",
issn = "1550-7998",
publisher = "American Physical Society",
number = "8",

}

RIS

TY - JOUR

T1 - Sneutrino condensate as a candidate for the hot big bang cosmology

AU - Mazumdar, Anupam

AU - Pérez-Lorenzana, A.

N1 - © 2004 The American Physical Society 19 pages, 3 figures. Some discussion on neutrino masses and baryogenesis, and other small changes added

PY - 2004/10/20

Y1 - 2004/10/20

N2 - 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.

AB - 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.

U2 - 10.1103/PhysRevD.70.083526

DO - 10.1103/PhysRevD.70.083526

M3 - Journal article

VL - 70

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 8

M1 - 083526

ER -