Beyond the big bang in Loop Quantum Cosmology
APA
Singh, P. (2008). Beyond the big bang in Loop Quantum Cosmology . Perimeter Institute. https://pirsa.org/08060170
MLA
Singh, Parampreet. Beyond the big bang in Loop Quantum Cosmology . Perimeter Institute, Jun. 06, 2008, https://pirsa.org/08060170
BibTex
@misc{ pirsa_PIRSA:08060170, doi = {10.48660/08060170}, url = {https://pirsa.org/08060170}, author = {Singh, Parampreet}, keywords = {Quantum Fields and Strings, Particle Physics, Cosmology}, language = {en}, title = {Beyond the big bang in Loop Quantum Cosmology }, publisher = {Perimeter Institute}, year = {2008}, month = {jun}, note = {PIRSA:08060170 see, \url{https://pirsa.org}} }
Louisiana State University
Collection
Talk Type
Abstract
Loop quantum cosmology is a non-perturbative canonical quantization of simple cosmological models based on loop quantum gravity. In recent years, a greater control on the underlying quantum theory has revealed a picture where the big bang is replaced by a quantum bounce at Planck scale. The evolution across the bounce is unitary and non-singular without a need of choice of exotic potential or matter. By analysis of an exactly solvable model of a homogeneous and isotropic spacetime we will describe how the backward evolution of our universe with the quantum constraint leads to a pre big bang branch. We will also discuss the way it predicts modifications to Friedman dynamics at high curvatures, contrasts with the Wheeler-DeWitt scenario and semi-classicality across the bounce.