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Curvature perturbation from symmetry breaking the end of inflation

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Curvature perturbation from symmetry breaking the end of inflation. / Alabidi, L.; Lyth, D. H.
In: Journal of Cosmology and Astroparticle Physics, 2006.

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Alabidi L, Lyth DH. Curvature perturbation from symmetry breaking the end of inflation. Journal of Cosmology and Astroparticle Physics. 2006. doi: 10.1088/1475-7516/2006/08/006

Author

Alabidi, L. ; Lyth, D. H. / Curvature perturbation from symmetry breaking the end of inflation. In: Journal of Cosmology and Astroparticle Physics. 2006.

Bibtex

@article{1ec13412f71b4abbacfb9c1b8728dc52,
title = "Curvature perturbation from symmetry breaking the end of inflation",
abstract = "We consider a two-field hybrid inflation model, in which the curvature perturbation is predominantly generated at the end of inflation. By finely tuning the coupling of the fields to the waterfall we find that we can get a measurable amount of non-Gaussianity.",
author = "L. Alabidi and Lyth, {D. H.}",
year = "2006",
doi = "10.1088/1475-7516/2006/08/006",
language = "English",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",

}

RIS

TY - JOUR

T1 - Curvature perturbation from symmetry breaking the end of inflation

AU - Alabidi, L.

AU - Lyth, D. H.

PY - 2006

Y1 - 2006

N2 - We consider a two-field hybrid inflation model, in which the curvature perturbation is predominantly generated at the end of inflation. By finely tuning the coupling of the fields to the waterfall we find that we can get a measurable amount of non-Gaussianity.

AB - We consider a two-field hybrid inflation model, in which the curvature perturbation is predominantly generated at the end of inflation. By finely tuning the coupling of the fields to the waterfall we find that we can get a measurable amount of non-Gaussianity.

U2 - 10.1088/1475-7516/2006/08/006

DO - 10.1088/1475-7516/2006/08/006

M3 - Journal article

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

ER -