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Supergravity inspired Vector curvaton

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Supergravity inspired Vector curvaton. / Dimopoulos, Konstantinos.
In: Physical Review D, Vol. 76, No. 6197, 063506, 14.09.2007.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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Dimopoulos K. Supergravity inspired Vector curvaton. Physical Review D. 2007 Sept 14;76(6197):063506. doi: 10.1103/PhysRevD.76.063506

Author

Dimopoulos, Konstantinos. / Supergravity inspired Vector curvaton. In: Physical Review D. 2007 ; Vol. 76, No. 6197.

Bibtex

@article{47a4ef8fbb174ca9a2f3dbc74ab027fe,
title = "Supergravity inspired Vector curvaton",
abstract = "It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing during inflation, can be responsible for the generation of the curvature perturbation in the Universe. Particle production is studied and it is shown that the vector field can obtain a scale-invariant superhorizon spectrum of perturbations with a reasonable choice of kinetic function. After inflation the vector field begins coherent oscillations, during which it corresponds to pressureless isotropic matter. When the vector field dominates the Universe, its perturbations give rise to the observed curvature perturbation following the curvaton scenario. It is found that this is possible if, after the end of inflation, the mass of the vector field increases at a phase transition at temperature of order 1 TeV or lower. Inhomogeneous reheating, whereby the vector field modulates the decay rate of the inflaton, is also studied.",
author = "Konstantinos Dimopoulos",
year = "2007",
month = sep,
day = "14",
doi = "10.1103/PhysRevD.76.063506",
language = "English",
volume = "76",
journal = "Physical Review D",
issn = "1550-7998",
publisher = "American Physical Society",
number = "6197",

}

RIS

TY - JOUR

T1 - Supergravity inspired Vector curvaton

AU - Dimopoulos, Konstantinos

PY - 2007/9/14

Y1 - 2007/9/14

N2 - It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing during inflation, can be responsible for the generation of the curvature perturbation in the Universe. Particle production is studied and it is shown that the vector field can obtain a scale-invariant superhorizon spectrum of perturbations with a reasonable choice of kinetic function. After inflation the vector field begins coherent oscillations, during which it corresponds to pressureless isotropic matter. When the vector field dominates the Universe, its perturbations give rise to the observed curvature perturbation following the curvaton scenario. It is found that this is possible if, after the end of inflation, the mass of the vector field increases at a phase transition at temperature of order 1 TeV or lower. Inhomogeneous reheating, whereby the vector field modulates the decay rate of the inflaton, is also studied.

AB - It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing during inflation, can be responsible for the generation of the curvature perturbation in the Universe. Particle production is studied and it is shown that the vector field can obtain a scale-invariant superhorizon spectrum of perturbations with a reasonable choice of kinetic function. After inflation the vector field begins coherent oscillations, during which it corresponds to pressureless isotropic matter. When the vector field dominates the Universe, its perturbations give rise to the observed curvature perturbation following the curvaton scenario. It is found that this is possible if, after the end of inflation, the mass of the vector field increases at a phase transition at temperature of order 1 TeV or lower. Inhomogeneous reheating, whereby the vector field modulates the decay rate of the inflaton, is also studied.

U2 - 10.1103/PhysRevD.76.063506

DO - 10.1103/PhysRevD.76.063506

M3 - Journal article

VL - 76

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 6197

M1 - 063506

ER -