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MSSM inflation.

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MSSM inflation. / Lyth, David H.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2007, No. 4, 11.04.2007, p. 006.

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

Harvard

Lyth, DH 2007, 'MSSM inflation.', Journal of Cosmology and Astroparticle Physics, vol. 2007, no. 4, pp. 006. https://doi.org/10.1088/1475-7516/2007/04/006

APA

Lyth, D. H. (2007). MSSM inflation. Journal of Cosmology and Astroparticle Physics, 2007(4), 006. https://doi.org/10.1088/1475-7516/2007/04/006

Vancouver

Lyth DH. MSSM inflation. Journal of Cosmology and Astroparticle Physics. 2007 Apr 11;2007(4):006. doi: 10.1088/1475-7516/2007/04/006

Author

Lyth, David H. / MSSM inflation. In: Journal of Cosmology and Astroparticle Physics. 2007 ; Vol. 2007, No. 4. pp. 006.

Bibtex

@article{e1ba9772a4c148fead77bd0f37311a7a,
title = "MSSM inflation.",
abstract = "Variants of the A-term model of hep-ph/0605035 are considered. They are equally successful, indicating that the model is quite robust once the relation between A and the soft mass is regarded as tunable. Alternatively a flat direction might support modular inflation.",
keywords = "cosmological perturbation theory, inflation, cosmology of theories beyond the SM, physics of the early universe",
author = "Lyth, {David H.}",
year = "2007",
month = apr,
day = "11",
doi = "10.1088/1475-7516/2007/04/006",
language = "English",
volume = "2007",
pages = "006",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",
number = "4",

}

RIS

TY - JOUR

T1 - MSSM inflation.

AU - Lyth, David H.

PY - 2007/4/11

Y1 - 2007/4/11

N2 - Variants of the A-term model of hep-ph/0605035 are considered. They are equally successful, indicating that the model is quite robust once the relation between A and the soft mass is regarded as tunable. Alternatively a flat direction might support modular inflation.

AB - Variants of the A-term model of hep-ph/0605035 are considered. They are equally successful, indicating that the model is quite robust once the relation between A and the soft mass is regarded as tunable. Alternatively a flat direction might support modular inflation.

KW - cosmological perturbation theory

KW - inflation

KW - cosmology of theories beyond the SM

KW - physics of the early universe

U2 - 10.1088/1475-7516/2007/04/006

DO - 10.1088/1475-7516/2007/04/006

M3 - Journal article

VL - 2007

SP - 006

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 4

ER -