Gravitational collapse and far from equilibrium dynamics in holographic CFTs
APA
Chesler, P. (2010). Gravitational collapse and far from equilibrium dynamics in holographic CFTs. Perimeter Institute. https://pirsa.org/10100043
MLA
Chesler, Paul. Gravitational collapse and far from equilibrium dynamics in holographic CFTs. Perimeter Institute, Oct. 07, 2010, https://pirsa.org/10100043
BibTex
@misc{ pirsa_PIRSA:10100043, doi = {10.48660/10100043}, url = {https://pirsa.org/10100043}, author = {Chesler, Paul}, keywords = {Quantum Fields and Strings}, language = {en}, title = {Gravitational collapse and far from equilibrium dynamics in holographic CFTs}, publisher = {Perimeter Institute}, year = {2010}, month = {oct}, note = {PIRSA:10100043 see, \url{https://pirsa.org}} }
Massachusetts Institute of Technology (MIT) - Department of Physics
Collection
Talk Type
Subject
Abstract
A remarkable result from heavy ion collisions at the Relativistic Heavy Ion Collider is that shortly after a collision, the medium produced behaves as a nearly ideal liquid. The system is very dynamic and evolves from a state of two colliding nuclei to a liquid in a time roughly equivalent to the time it takes light to cross a proton. Understanding the mechanisms behind the rapid approach to a liquid state is a challenging task. In recent years holography has emerged as a powerful tool to study non-equilibrium phenomena, mapping the (challenging) dynamics of quantum systems onto the dynamics of classical gravitational systems. The creation of a liquid in a quantum theory maps onto the classical process of gravitational collapse and black hole formation. I will describe how one can use holography to study processes which mimic the dynamics of heavy ion collisions.