Speaker
Ms
Sukannya Bhattacharya
(Saha Institute of Nuclear Physics)
Description
The dissipative mechanism in warm inflation scenario can provide the inflating universe with a warm exit to the radiation dominated era rather than a supercooled exit to a reheating phase. In this work, we constrain the model parameters for warm inflation from Planck 2015 data. In addition, the reheating era can be optimized by varying the number of $e$-folds of inflation. Best fit values for the model parameters are estimated with and without the contribution to fluctuation from thermal excitations.
Primary author
Ms
Sukannya Bhattacharya
(Saha Institute of Nuclear Physics)
Co-authors
Prof.
Koushik Dutta
(Saha Institute of Nuclear Physics)
Prof.
Mar Bastero Gil
(University of Granada)
