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Anisotropic non-Gaussianity from vector field perturbations

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Anisotropic non-Gaussianity from vector field perturbations. / Karciauskas, Mindaugas; Dimopoulos, Konstantinos; Lyth, David H.
In: Physical Review D, Vol. 80, No. 2, 15.07.2009, p. 023509.

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Karciauskas M, Dimopoulos K, Lyth DH. Anisotropic non-Gaussianity from vector field perturbations. Physical Review D. 2009 Jul 15;80(2):023509. doi: 10.1103/PhysRevD.80.023509

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Karciauskas, Mindaugas ; Dimopoulos, Konstantinos ; Lyth, David H. / Anisotropic non-Gaussianity from vector field perturbations. In: Physical Review D. 2009 ; Vol. 80, No. 2. pp. 023509.

Bibtex

@article{25ba6342e5454a718874f2e800dc2fb8,
title = "Anisotropic non-Gaussianity from vector field perturbations",
abstract = "We suppose that a vector field perturbation causes part of the primordial curvature perturbation. The non-Gaussianity parameter f_NL is then, in general, statistically anisotropic. We calculate its form and magnitude in the curvaton scenario and in the end-of-inflation scenario. We show that this anisotropy could easily be observable.",
author = "Mindaugas Karciauskas and Konstantinos Dimopoulos and Lyth, {David H.}",
year = "2009",
month = jul,
day = "15",
doi = "10.1103/PhysRevD.80.023509",
language = "English",
volume = "80",
pages = "023509",
journal = "Physical Review D",
issn = "1550-7998",
publisher = "American Physical Society",
number = "2",

}

RIS

TY - JOUR

T1 - Anisotropic non-Gaussianity from vector field perturbations

AU - Karciauskas, Mindaugas

AU - Dimopoulos, Konstantinos

AU - Lyth, David H.

PY - 2009/7/15

Y1 - 2009/7/15

N2 - We suppose that a vector field perturbation causes part of the primordial curvature perturbation. The non-Gaussianity parameter f_NL is then, in general, statistically anisotropic. We calculate its form and magnitude in the curvaton scenario and in the end-of-inflation scenario. We show that this anisotropy could easily be observable.

AB - We suppose that a vector field perturbation causes part of the primordial curvature perturbation. The non-Gaussianity parameter f_NL is then, in general, statistically anisotropic. We calculate its form and magnitude in the curvaton scenario and in the end-of-inflation scenario. We show that this anisotropy could easily be observable.

UR - http://www.scopus.com/inward/record.url?scp=69249124126&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.80.023509

DO - 10.1103/PhysRevD.80.023509

M3 - Journal article

VL - 80

SP - 023509

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 2

ER -