Quasi-single and Multiple Field Inflation
APA
(2011). Quasi-single and Multiple Field Inflation. Perimeter Institute. https://pirsa.org/11110002
MLA
Quasi-single and Multiple Field Inflation. Perimeter Institute, Nov. 08, 2011, https://pirsa.org/11110002
BibTex
@misc{ pirsa_PIRSA:11110002, doi = {10.48660/11110002}, url = {https://pirsa.org/11110002}, author = {}, keywords = {Cosmology}, language = {en}, title = {Quasi-single and Multiple Field Inflation}, publisher = {Perimeter Institute}, year = {2011}, month = {nov}, note = {PIRSA:11110002 see, \url{https://pirsa.org}} }
Collection
Talk Type
Subject
Abstract
The talk consists of two parts: (1) Quasi-single inflation, where the isocurvature direction has mass of order Hubble parameter. This part is based on 0911.3380 and new results about higher mass, and a sharp turn in trajectory. (2) Multi-stream inflation, where the inflationary trajectory bifurcates. This part is based on 0903.2123, 1006.5021 and a on-going project on calculating the bifurcation probability in a complicated landscape.