Probing extreme gravity in stellar collapse

          @misc{ scivideos_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 for Theoretical Physics},
            year = {2017},
            month = {nov},
            note = {PIRSA:17110086 see, \url{https://scivideos.org/index.php/pirsa/17110086}}
          }
          

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.