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Final reheating temperature on a single brane

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Final reheating temperature on a single brane. / Allahverdi, Rouzbeh; Mazumdar, Anupam; Pérez-Lorenzana, A.
In: Physics Letters B, Vol. 516, No. 3-4, 20.09.2001, p. 431-438.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Allahverdi, R, Mazumdar, A & Pérez-Lorenzana, A 2001, 'Final reheating temperature on a single brane', Physics Letters B, vol. 516, no. 3-4, pp. 431-438. https://doi.org/10.1016/S0370-2693(01)00967-4

APA

Allahverdi, R., Mazumdar, A., & Pérez-Lorenzana, A. (2001). Final reheating temperature on a single brane. Physics Letters B, 516(3-4), 431-438. https://doi.org/10.1016/S0370-2693(01)00967-4

Vancouver

Allahverdi R, Mazumdar A, Pérez-Lorenzana A. Final reheating temperature on a single brane. Physics Letters B. 2001 Sept 20;516(3-4):431-438. doi: 10.1016/S0370-2693(01)00967-4

Author

Allahverdi, Rouzbeh ; Mazumdar, Anupam ; Pérez-Lorenzana, A. / Final reheating temperature on a single brane. In: Physics Letters B. 2001 ; Vol. 516, No. 3-4. pp. 431-438.

Bibtex

@article{45d92f9c92404f8a9fc39ecf48e7758a,
title = "Final reheating temperature on a single brane",
abstract = "We make a generic remark on thermal history of a single brane cosmology in models with an infinitely large single extra dimension. We point out that the reheat temperature of the Universe is bounded by an excess production of gravitons from the thermal bath. The actual bound is given by the brane tension. If the initial temperature of the Universe is larger than this bound, then an efficient graviton production shall prevail. However, the brane cools down gradually as the Kaluza-Klein gravitons take the energy in excess away from the brane. The cooling continues until the radiation dominated phase is restored, which occurs before the Big Bang Nucleosynthesis. We argue whatsoever be the early evolution of the Universe, the final radiation dominated phase always starts after the Universe transits from non-conventional era to the standard cosmological era.",
author = "Rouzbeh Allahverdi and Anupam Mazumdar and A. P{\'e}rez-Lorenzana",
note = "11 pages, no figures. Major changes. Bounds on brane tension removed",
year = "2001",
month = sep,
day = "20",
doi = "10.1016/S0370-2693(01)00967-4",
language = "English",
volume = "516",
pages = "431--438",
journal = "Physics Letters B",
issn = "0370-2693",
publisher = "ELSEVIER SCIENCE BV",
number = "3-4",

}

RIS

TY - JOUR

T1 - Final reheating temperature on a single brane

AU - Allahverdi, Rouzbeh

AU - Mazumdar, Anupam

AU - Pérez-Lorenzana, A.

N1 - 11 pages, no figures. Major changes. Bounds on brane tension removed

PY - 2001/9/20

Y1 - 2001/9/20

N2 - We make a generic remark on thermal history of a single brane cosmology in models with an infinitely large single extra dimension. We point out that the reheat temperature of the Universe is bounded by an excess production of gravitons from the thermal bath. The actual bound is given by the brane tension. If the initial temperature of the Universe is larger than this bound, then an efficient graviton production shall prevail. However, the brane cools down gradually as the Kaluza-Klein gravitons take the energy in excess away from the brane. The cooling continues until the radiation dominated phase is restored, which occurs before the Big Bang Nucleosynthesis. We argue whatsoever be the early evolution of the Universe, the final radiation dominated phase always starts after the Universe transits from non-conventional era to the standard cosmological era.

AB - We make a generic remark on thermal history of a single brane cosmology in models with an infinitely large single extra dimension. We point out that the reheat temperature of the Universe is bounded by an excess production of gravitons from the thermal bath. The actual bound is given by the brane tension. If the initial temperature of the Universe is larger than this bound, then an efficient graviton production shall prevail. However, the brane cools down gradually as the Kaluza-Klein gravitons take the energy in excess away from the brane. The cooling continues until the radiation dominated phase is restored, which occurs before the Big Bang Nucleosynthesis. We argue whatsoever be the early evolution of the Universe, the final radiation dominated phase always starts after the Universe transits from non-conventional era to the standard cosmological era.

U2 - 10.1016/S0370-2693(01)00967-4

DO - 10.1016/S0370-2693(01)00967-4

M3 - Journal article

VL - 516

SP - 431

EP - 438

JO - Physics Letters B

JF - Physics Letters B

SN - 0370-2693

IS - 3-4

ER -