Holographic Cosmology Inflation and Entropy
APA
Banks, T. (2011). Holographic Cosmology Inflation and Entropy. Perimeter Institute. https://pirsa.org/11070007
MLA
Banks, Tom. Holographic Cosmology Inflation and Entropy. Perimeter Institute, Jul. 15, 2011, https://pirsa.org/11070007
BibTex
@misc{ pirsa_PIRSA:11070007, doi = {10.48660/11070007}, url = {https://pirsa.org/11070007}, author = {Banks, Tom}, keywords = {Cosmology}, language = {en}, title = {Holographic Cosmology Inflation and Entropy}, publisher = {Perimeter Institute}, year = {2011}, month = {jul}, note = {PIRSA:11070007 see, \url{https://pirsa.org}} }
Rutgers University
Talk Type
Subject
Abstract
I provide a mathematical model of holographic cosmology whose coarse grained description is that of a homogeneous isotropic, flat universe, which makes a transitions from an FRW to an eternal de Sitter regime. Based on this model, I suggest some heuristic ideas which explain the low initial entropy of the universe and may provide a description of an inflationary era with small fluctuations.