Black hole information loss and discreteness of quantum geometry
APA
Perez, A. (2015). Black hole information loss and discreteness of quantum geometry. Perimeter Institute. https://pirsa.org/15040068
MLA
Perez, Alejandro. Black hole information loss and discreteness of quantum geometry. Perimeter Institute, Apr. 23, 2015, https://pirsa.org/15040068
BibTex
@misc{ pirsa_PIRSA:15040068, doi = {10.48660/15040068}, url = {https://pirsa.org/15040068}, author = {Perez, Alejandro}, keywords = {Quantum Gravity}, language = {en}, title = {Black hole information loss and discreteness of quantum geometry}, publisher = {Perimeter Institute}, year = {2015}, month = {apr}, note = {PIRSA:15040068 see, \url{https://pirsa.org}} }
In an approach to quantum gravity where space-time arises from coarse graining of fundamentally discrete structures, black hole formation and subsequent evaporation could be described by a unitary evolution without the problems encountered by standard remnant scenarios or the schemes where information is assumed to come out with the radiation while semiclassical evaporation (firewalls and complementarity). I point out the possibility that the final state is purified by correlations with the fundamental pre-geometric structures (in the sense of Wheeler) which are available in such approaches, and, like defects in the underlying space-time weave, can carry zero energy.