Black hole evaporation in random matrix theory (RMT) and statistical CFTs
APA
(2024). Black hole evaporation in random matrix theory (RMT) and statistical CFTs. Perimeter Institute. https://pirsa.org/24110077
MLA
Black hole evaporation in random matrix theory (RMT) and statistical CFTs. Perimeter Institute, Nov. 20, 2024, https://pirsa.org/24110077
BibTex
@misc{ pirsa_PIRSA:24110077, doi = {10.48660/24110077}, url = {https://pirsa.org/24110077}, author = {}, keywords = {Quantum Information}, language = {en}, title = {Black hole evaporation in random matrix theory (RMT) and statistical CFTs}, publisher = {Perimeter Institute}, year = {2024}, month = {nov}, note = {PIRSA:24110077 see, \url{https://pirsa.org}} }
Andrew Rolph
Collection
Talk Type
Subject
Abstract
In this talk, with two parts, I will first show how to capture both Hawking's non-unitary entropy curve and density matrix-connecting contributions that restore unitarity, in a toy RMT quantum system modelling black hole evaporation. The motivation is to find the simplest possible dynamical model that captures this aspect of gravitational physics. In the model, there is a dynamical phase transition in the averaging that connects the density matrices in a replica wormhole-like manner and restores unitarity in the entropy curve. In the second half of the talk, I will discuss ongoing follow-up work describing black hole evaporation and unitarity restoration in statistical descriptions of holographic CFTs.