Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 4, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2007/04/007
Keywords
CMBR theory; inflation
Ask authors/readers for more resources
The scalar mode density perturbations in the warm inflationary scenario are analysed with a view to predicting the amount of non-Gaussianity produced by this scenario. The analysis assumes that the inflaton evolution is strongly damped by the radiation, with damping terms that are temperature independent. Entropy fluctuations during warm inflation play a crucial role in generating non-Gaussianity and result in a distinctive signal which should be observable by the Planck satellite.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available