Phases of Gravitational Collapse in AdS
APA
Frey, A. (2018). Phases of Gravitational Collapse in AdS. Perimeter Institute. https://pirsa.org/18050063
MLA
Frey, Andrew. Phases of Gravitational Collapse in AdS. Perimeter Institute, May. 23, 2018, https://pirsa.org/18050063
BibTex
@misc{ pirsa_PIRSA:18050063, doi = {10.48660/18050063}, url = {https://pirsa.org/18050063}, author = {Frey, Andrew}, keywords = {Quantum Fields and Strings}, language = {en}, title = {Phases of Gravitational Collapse in AdS}, publisher = {Perimeter Institute}, year = {2018}, month = {may}, note = {PIRSA:18050063 see, \url{https://pirsa.org}} }
Generically, a small amount of matter introduced to anti-de Sitter spacetime leads to formation of a black hole; however, the high degree of symmetry of AdS means that some initial distributions of matter (possibly also technically generic) oscillate indefinitely. Whether a given initial profile leads to a horizon at arbitrarily small amplitudes is of great interest for a number of reasons, not least because horizon formation corresponds holographically to thermalization in CFT. We will present an overview of approaches the question and show a phase diagram of the stability behavior of AdS in the presence of a scalar field, including an analysis of nonperturbative phases at the border of perturbative stability and instability.