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Inflation models after WMAP year three

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Inflation models after WMAP year three. / Alabidi, L.; Lyth, D. H.
In: Journal of Cosmology and Astroparticle Physics, 2006.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Alabidi, L & Lyth, DH 2006, 'Inflation models after WMAP year three', Journal of Cosmology and Astroparticle Physics. https://doi.org/10.1088/1475-7516/2006/08/013

APA

Alabidi, L., & Lyth, D. H. (2006). Inflation models after WMAP year three. Journal of Cosmology and Astroparticle Physics. https://doi.org/10.1088/1475-7516/2006/08/013

Vancouver

Alabidi L, Lyth DH. Inflation models after WMAP year three. Journal of Cosmology and Astroparticle Physics. 2006. doi: 10.1088/1475-7516/2006/08/013

Author

Alabidi, L. ; Lyth, D. H. / Inflation models after WMAP year three. In: Journal of Cosmology and Astroparticle Physics. 2006.

Bibtex

@article{cf9563823d9e4a498c6da6c35af5ef1a,
title = "Inflation models after WMAP year three",
abstract = "The survey of models in astro-ph/0510441 is updated. For the first time, a large fraction of the models is ruled out at more than 3σ.",
keywords = "CMBR experiments, inflation",
author = "L. Alabidi and Lyth, {D. H.}",
year = "2006",
doi = "10.1088/1475-7516/2006/08/013",
language = "English",
journal = "Journal of Cosmology and Astroparticle Physics",
publisher = "IOP Publishing",

}

RIS

TY - JOUR

T1 - Inflation models after WMAP year three

AU - Alabidi, L.

AU - Lyth, D. H.

PY - 2006

Y1 - 2006

N2 - The survey of models in astro-ph/0510441 is updated. For the first time, a large fraction of the models is ruled out at more than 3σ.

AB - The survey of models in astro-ph/0510441 is updated. For the first time, a large fraction of the models is ruled out at more than 3σ.

KW - CMBR experiments

KW - inflation

U2 - 10.1088/1475-7516/2006/08/013

DO - 10.1088/1475-7516/2006/08/013

M3 - Journal article

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

ER -