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Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation.

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

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Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation. / Bueno-Sanchez, Juan Carlos; Dimopoulos, Konstantinos.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2007, No. 11, 09.11.2007, p. 007.

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

Harvard

Bueno-Sanchez, JC & Dimopoulos, K 2007, 'Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation.', Journal of Cosmology and Astroparticle Physics, vol. 2007, no. 11, pp. 007. https://doi.org/10.1088/1475-7516/2007/11/007

APA

Bueno-Sanchez, J. C., & Dimopoulos, K. (2007). Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation. Journal of Cosmology and Astroparticle Physics, 2007(11), 007. https://doi.org/10.1088/1475-7516/2007/11/007

Vancouver

Bueno-Sanchez JC, Dimopoulos K. Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation. Journal of Cosmology and Astroparticle Physics. 2007 Nov 9;2007(11):007. doi: 10.1088/1475-7516/2007/11/007

Author

Bueno-Sanchez, Juan Carlos ; Dimopoulos, Konstantinos. / Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation. In: Journal of Cosmology and Astroparticle Physics. 2007 ; Vol. 2007, No. 11. pp. 007.

Bibtex

@article{3729a50766e44887b9e4a316b45a4914,
title = "Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation.",
abstract = "Curvaton reheating is studied in non-oscillatory models of inflation, with the aim of obtaining bounds on the parameters of curvaton models and finding out whether low scale inflation can be attained. Using a minimal curvaton model, it is found that the allowed parameter space is considerably larger than in the case of the usual oscillatory inflation models. In particular, inflation with a Hubble scale as low as 1 TeV is comfortably allowed.",
keywords = "inflation, cosmology of theories beyond the SM",
author = "Bueno-Sanchez, {Juan Carlos} and Konstantinos Dimopoulos",
year = "2007",
month = nov,
day = "9",
doi = "10.1088/1475-7516/2007/11/007",
language = "English",
volume = "2007",
pages = "007",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",
number = "11",

}

RIS

TY - JOUR

T1 - Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation.

AU - Bueno-Sanchez, Juan Carlos

AU - Dimopoulos, Konstantinos

PY - 2007/11/9

Y1 - 2007/11/9

N2 - Curvaton reheating is studied in non-oscillatory models of inflation, with the aim of obtaining bounds on the parameters of curvaton models and finding out whether low scale inflation can be attained. Using a minimal curvaton model, it is found that the allowed parameter space is considerably larger than in the case of the usual oscillatory inflation models. In particular, inflation with a Hubble scale as low as 1 TeV is comfortably allowed.

AB - Curvaton reheating is studied in non-oscillatory models of inflation, with the aim of obtaining bounds on the parameters of curvaton models and finding out whether low scale inflation can be attained. Using a minimal curvaton model, it is found that the allowed parameter space is considerably larger than in the case of the usual oscillatory inflation models. In particular, inflation with a Hubble scale as low as 1 TeV is comfortably allowed.

KW - inflation

KW - cosmology of theories beyond the SM

U2 - 10.1088/1475-7516/2007/11/007

DO - 10.1088/1475-7516/2007/11/007

M3 - Journal article

VL - 2007

SP - 007

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 11

ER -