Video URL
https://pirsa.org/22110045Shapes of non-Gaussianity in warm inflation
APA
Mirbabayi, M. (2022). Shapes of non-Gaussianity in warm inflation. Perimeter Institute for Theoretical Physics. https://pirsa.org/22110045
MLA
Mirbabayi, Mehrdad. Shapes of non-Gaussianity in warm inflation. Perimeter Institute for Theoretical Physics, Nov. 29, 2022, https://pirsa.org/22110045
BibTex
@misc{ scivideos_PIRSA:22110045, doi = {10.48660/22110045}, url = {https://pirsa.org/22110045}, author = {Mirbabayi, Mehrdad}, keywords = {Cosmology, Particle Physics}, language = {en}, title = {Shapes of non-Gaussianity in warm inflation}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2022}, month = {nov}, note = {PIRSA:22110045 see, \url{https://scivideos.org/index.php/pirsa/22110045}} }
Mehrdad Mirbabayi Institute for Advanced Study (IAS)
Abstract
Sphaleron heating has been recently proposed as a mechanism to realize warm inflation when inflaton is an axion coupled to pure Yang-Mills. As a result of heating, there is a friction coefficient γ\propto T^3 in the equation of motion for the inflaton, and a thermal contribution to cosmological fluctuations. Without the knowledge of the inflaton potential, non-Gaussianity is the most promising way of searching for the signatures of this model. Building on an earlier work by Bastero-Gil, Berera, Moss and Ramos, we compute the scalar three-point correlation function and point out some distinct features in the squeezed and folded limits. As a detection strategy, we show that the combination of the equilateral template and one new template has a large overlap with the shape of non-Gaussianity over the range 0.01 <= γ/Η <= 1000 and in this range 0.7<|f_NL|<50.
Zoom link: https://pitp.zoom.us/j/95921707772?pwd=NUNhU1QrRm5HaDJNMEYyaTJXQmZnQT09