Some Possible Ways to Observe Consequences of Loop Quantum Gravity
APA
Barrau, A. (2013). Some Possible Ways to Observe Consequences of Loop Quantum Gravity. Perimeter Institute. https://pirsa.org/13070036
MLA
Barrau, Aurelien. Some Possible Ways to Observe Consequences of Loop Quantum Gravity. Perimeter Institute, Jul. 22, 2013, https://pirsa.org/13070036
BibTex
@misc{ pirsa_PIRSA:13070036, doi = {10.48660/13070036}, url = {https://pirsa.org/13070036}, author = {Barrau, Aurelien}, keywords = {}, language = {en}, title = {Some Possible Ways to Observe Consequences of Loop Quantum Gravity}, publisher = {Perimeter Institute}, year = {2013}, month = {jul}, note = {PIRSA:13070036 see, \url{https://pirsa.org}} }
Laboratoire de Physique Subatomique et de Cosmologie (LPSC Grenoble)
Collection
Talk Type
Abstract
In this talk, I'll briefly review some possible observational consequences of loop quantum gravity. I will first address the issue of the closure of the algebra of constraints in holonomy-corrected effective loop quantum cosmology for tensor, vector, and scalar modes. I will underline some unexpected features like a possible change of signature. The associated primordial power spectrum and the basics of the related CMB analysis will be presented. The "asymptotic silence" hypothesis will be mentioned as a promising alternative. Then, I'll address the issue of the probability for inflation and the prediction of its duration from a new perspective. Finally, I'll present some prospect about the evaporation of black holes in LQG.