Home > Research > Publications & Outputs > Warm hilltop inflation

Associated organisational unit

View graph of relations

Warm hilltop inflation

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Article number123527
<mark>Journal publication date</mark>15/06/2008
<mark>Journal</mark>Physical Review D
Issue number12
Publication StatusPublished
<mark>Original language</mark>English


We study the low-temperature limit of warm inflation in a hilltop model. This limit remains valid up to the end of inflation, allowing an analytic description of the entire inflationary stage. In the weak dissipative regime, if the kinetic density of the inflaton dominates after inflation, low-scale inflation is attained with Hubble scale as low as 1 GeV. In the strong dissipative regime, the model satisfies the observational requirements for the spectral index with a mild tuning of the model parameters, while also overcoming the eta-problem of inflation. However, there is some danger of gravitino overproduction unless the particle content of the theory is large.