Bueno-Sanchez, Juan Carlos and Dimopoulos, Konstantinos (2007) Curvaton reheating allows a TeV Hubble scale in non-oscillatory inflation. Journal of Cosmology and Astroparticle Physics, 2007 (11). 007. ISSN 1475-7516Full text not available from this repository.
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.
|Journal or Publication Title:||Journal of Cosmology and Astroparticle Physics|
|Uncontrolled Keywords:||inflation ; cosmology of theories beyond the SM|
|Subjects:||Q Science > QC Physics|
|Departments:||Faculty of Science and Technology > Physics|
|Deposited On:||28 Oct 2008 11:12|
|Last Modified:||03 Nov 2015 14:09|
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