G-Bounce
APA
Vikman, A. (2012). G-Bounce. Perimeter Institute. https://pirsa.org/12030103
MLA
Vikman, Alexander. G-Bounce. Perimeter Institute, Mar. 19, 2012, https://pirsa.org/12030103
BibTex
@misc{ pirsa_PIRSA:12030103, doi = {10.48660/12030103}, url = {https://pirsa.org/12030103}, author = {Vikman, Alexander}, keywords = {Cosmology}, language = {en}, title = {G-Bounce}, publisher = {Perimeter Institute}, year = {2012}, month = {mar}, note = {PIRSA:12030103 see, \url{https://pirsa.org}} }
European Organization for Nuclear Research (CERN)
Collection
Talk Type
Subject
Abstract
I will discuss a wide class of models which realise a bounce in a spatially flat Friedmann universe in standard General Relativity. The key ingredient is a noncanonical, minimally coupled scalar field
belonging to the class of theories with Kinetic Gravity Braiding/Galileon-like self-couplings. In these models, the universe smoothly volves from contraction to expansion, suffering neither from ghosts
nor gradient instabilities around the turning point. The end-point of he evolution can be a standard radiation-domination era or an nflationary phase.
The talk is based on arXiv:1109.1047v2 [hep-th], JCAP11(2011)021.
belonging to the class of theories with Kinetic Gravity Braiding/Galileon-like self-couplings. In these models, the universe smoothly volves from contraction to expansion, suffering neither from ghosts
nor gradient instabilities around the turning point. The end-point of he evolution can be a standard radiation-domination era or an nflationary phase.
The talk is based on arXiv:1109.1047v2 [hep-th], JCAP11(2011)021.