Partition Functions of Three Dimensional Gravity
APA
Maloney, A. (2007). Partition Functions of Three Dimensional Gravity. Perimeter Institute. https://pirsa.org/07110061
MLA
Maloney, Alexander. Partition Functions of Three Dimensional Gravity. Perimeter Institute, Nov. 12, 2007, https://pirsa.org/07110061
BibTex
@misc{ pirsa_PIRSA:07110061, doi = {10.48660/07110061}, url = {https://pirsa.org/07110061}, author = {Maloney, Alexander}, keywords = {Quantum Fields and Strings}, language = {en}, title = {Partition Functions of Three Dimensional Gravity}, publisher = {Perimeter Institute}, year = {2007}, month = {nov}, note = {PIRSA:07110061 see, \url{https://pirsa.org}} }
McGill University
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Abstract
We consider pure three dimensional quantum gravity with a negative cosmological constant. The torus partition function can be computed exactly as a sum over geometries, including all known quantum corrections. The answer provides important clues about the structure of quantum gravity; in particular, in order for the theory to be a proper quantum mechanical system some extra ingredients are needed beyond the usual real geometries considered in general relativity. One possiblity is that complex geometries need to be included; this leads to holomorphically factorized partition functions. These partition functions provide a wealth of information about black hole microphysics. For example, the Hawking-page phase transition can be studied exactly; it is a phase transition of the type described by Lee and Yang, which is associated with a condensation of zeros in the complex temperature plane.