Bulk observables in JT gravity
APA
Mertens, T. (2020). Bulk observables in JT gravity. Perimeter Institute. https://pirsa.org/20050028
MLA
Mertens, Thomas. Bulk observables in JT gravity. Perimeter Institute, May. 21, 2020, https://pirsa.org/20050028
BibTex
@misc{ pirsa_PIRSA:20050028, doi = {10.48660/20050028}, url = {https://pirsa.org/20050028}, author = {Mertens, Thomas}, keywords = {Quantum Gravity}, language = {en}, title = {Bulk observables in JT gravity}, publisher = {Perimeter Institute}, year = {2020}, month = {may}, note = {PIRSA:20050028 see, \url{https://pirsa.org}} }
Using a definition of bulk diff-invariant observables, we go into the bulk of 2d Jackiw-Teitelboim gravity. By mapping the computation to a Schwarzian path integral, we study exact bulk correlation functions and discuss their physical implications. We describe how the black hole thermal atmosphere gets modified by quantum gravitational corrections. Finally, we will discuss how higher topological effects further modify the spectral density and detector response in the Unruh heat bath.