Home > Research > Publications & Outputs > Enhanced reheating via Bose condensates

Research

Electronic data

  • PhysRevD

    Rights statement: © 2004 The American Physical Society

    Final published version, 104 KB, PDF document

Links

Text available via DOI:

View graph of relations

Enhanced reheating via Bose condensates

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

Published

Standard

Enhanced reheating via Bose condensates. / Allahverdi, Rouzbeh; Brandenberger, Robert; Mazumdar, Anupam.
In: Physical Review D, Vol. 70, No. 8, 29.10.2004.

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

Harvard

Allahverdi, R, Brandenberger, R & Mazumdar, A 2004, 'Enhanced reheating via Bose condensates', Physical Review D, vol. 70, no. 8. https://doi.org/10.1103/PhysRevD.70.083535

APA

Allahverdi, R., Brandenberger, R., & Mazumdar, A. (2004). Enhanced reheating via Bose condensates. Physical Review D, 70(8). https://doi.org/10.1103/PhysRevD.70.083535

Vancouver

Allahverdi R, Brandenberger R, Mazumdar A. Enhanced reheating via Bose condensates. Physical Review D. 2004 Oct 29;70(8). doi: 10.1103/PhysRevD.70.083535

Author

Allahverdi, Rouzbeh ; Brandenberger, Robert ; Mazumdar, Anupam. / Enhanced reheating via Bose condensates. In: Physical Review D. 2004 ; Vol. 70, No. 8.

Bibtex

@article{6305cb54ead24bbc98e3be1ccf831cbc,
title = "Enhanced reheating via Bose condensates",
abstract = "In supersymmetric extensions of the particle physics Standard Model, gauge invariant combinations of squarks and sleptons (flat directions) can acquire large expectation values during a period of cosmological inflation. If the inflaton sector couples to matter fields via these flat directions, then new channels for efficient reheating, in particular via parametric resonance instabilities, are opened up. These can lead to efficient reheating induced by the flat directions even if the bare coupling constants are small. In this Letter we discuss various channels which yield this {"}enhanced reheating{"} effect, and we address some cosmological consequences.",
author = "Rouzbeh Allahverdi and Robert Brandenberger and Anupam Mazumdar",
note = "{\textcopyright} 2004 The American Physical Society 6 pages",
year = "2004",
month = oct,
day = "29",
doi = "10.1103/PhysRevD.70.083535",
language = "English",
volume = "70",
journal = "Physical Review D",
issn = "1550-7998",
publisher = "American Physical Society",
number = "8",

}

RIS

TY - JOUR

T1 - Enhanced reheating via Bose condensates

AU - Allahverdi, Rouzbeh

AU - Brandenberger, Robert

AU - Mazumdar, Anupam

N1 - © 2004 The American Physical Society 6 pages

PY - 2004/10/29

Y1 - 2004/10/29

N2 - In supersymmetric extensions of the particle physics Standard Model, gauge invariant combinations of squarks and sleptons (flat directions) can acquire large expectation values during a period of cosmological inflation. If the inflaton sector couples to matter fields via these flat directions, then new channels for efficient reheating, in particular via parametric resonance instabilities, are opened up. These can lead to efficient reheating induced by the flat directions even if the bare coupling constants are small. In this Letter we discuss various channels which yield this "enhanced reheating" effect, and we address some cosmological consequences.

AB - In supersymmetric extensions of the particle physics Standard Model, gauge invariant combinations of squarks and sleptons (flat directions) can acquire large expectation values during a period of cosmological inflation. If the inflaton sector couples to matter fields via these flat directions, then new channels for efficient reheating, in particular via parametric resonance instabilities, are opened up. These can lead to efficient reheating induced by the flat directions even if the bare coupling constants are small. In this Letter we discuss various channels which yield this "enhanced reheating" effect, and we address some cosmological consequences.

U2 - 10.1103/PhysRevD.70.083535

DO - 10.1103/PhysRevD.70.083535

M3 - Journal article

VL - 70

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 8

ER -