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The curvature perturbation in a box.

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The curvature perturbation in a box. / Lyth, David H.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2007, No. 12, 19.12.2007, p. 0016.

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

Harvard

Lyth, DH 2007, 'The curvature perturbation in a box.', Journal of Cosmology and Astroparticle Physics, vol. 2007, no. 12, pp. 0016. https://doi.org/10.1088/1475-7516/2007/12/016

APA

Lyth, D. H. (2007). The curvature perturbation in a box. Journal of Cosmology and Astroparticle Physics, 2007(12), 0016. https://doi.org/10.1088/1475-7516/2007/12/016

Vancouver

Lyth DH. The curvature perturbation in a box. Journal of Cosmology and Astroparticle Physics. 2007 Dec 19;2007(12):0016. doi: 10.1088/1475-7516/2007/12/016

Author

Lyth, David H. / The curvature perturbation in a box. In: Journal of Cosmology and Astroparticle Physics. 2007 ; Vol. 2007, No. 12. pp. 0016.

Bibtex

@article{01b7f64135d14c80b3a2d6622f760bc2,
title = "The curvature perturbation in a box.",
abstract = "The stochastic properties of cosmological perturbations are best defined through the Fourier expansion in a finite box. I discuss the reasons for that with reference to the curvature perturbation, and explore some issues arising from it.",
keywords = "cosmological perturbation theory, inflation, physics of the early universe",
author = "Lyth, {David H.}",
year = "2007",
month = dec,
day = "19",
doi = "10.1088/1475-7516/2007/12/016",
language = "English",
volume = "2007",
pages = "0016",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",
number = "12",

}

RIS

TY - JOUR

T1 - The curvature perturbation in a box.

AU - Lyth, David H.

PY - 2007/12/19

Y1 - 2007/12/19

N2 - The stochastic properties of cosmological perturbations are best defined through the Fourier expansion in a finite box. I discuss the reasons for that with reference to the curvature perturbation, and explore some issues arising from it.

AB - The stochastic properties of cosmological perturbations are best defined through the Fourier expansion in a finite box. I discuss the reasons for that with reference to the curvature perturbation, and explore some issues arising from it.

KW - cosmological perturbation theory

KW - inflation

KW - physics of the early universe

U2 - 10.1088/1475-7516/2007/12/016

DO - 10.1088/1475-7516/2007/12/016

M3 - Journal article

VL - 2007

SP - 0016

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 12

ER -