Probing extreme gravity in stellar collapse
APA
Barcelo, C. (2017). Probing extreme gravity in stellar collapse. Perimeter Institute. https://pirsa.org/17110086
MLA
Barcelo, Carlos. Probing extreme gravity in stellar collapse. Perimeter Institute, Nov. 09, 2017, https://pirsa.org/17110086
BibTex
@misc{ pirsa_PIRSA:17110086, doi = {10.48660/17110086}, url = {https://pirsa.org/17110086}, author = {Barcelo, Carlos}, keywords = {Quantum Gravity}, language = {en}, title = {Probing extreme gravity in stellar collapse}, publisher = {Perimeter Institute}, year = {2017}, month = {nov}, note = {PIRSA:17110086 see, \url{https://pirsa.org}} }
Institute of Astrophysics of Andalusia
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Abstract
The standard way to understand quantum corrected black holes leads to the information loss paradox and the lifetime dilemma. A radical way out of this situation is to give up a hypothesis which is tacitly assumed in the vast majority of works on the subject: that the classical singularity is substituted by something effectively acting as a sink for a long period of time, as seen by asymptotic observers.
Eliminating this characteristic changes drastically much of the physics now associated to black holes. A nice feature of the new hypothesis it that it offers a
clear possibility of experimental falsifiability with upcoming gravitational waves observations. In this talk I will discuss these possibilities.