arXiv · 1903.10485
Towards Black Hole Evaporation in Jackiw-Teitelboim Gravity
Abstract
Using a definition of the bulk frame within 2d Jackiw-Teitelboim gravity, we go into the bulk from the Schwarzian boundary. Including the path integral over the Schwarzian degrees of freedom, we discuss the quantum gravitational Unruh effect and the Planckian black-body spectrum of the thermal atmosphere. We analyze matter entanglement entropy and how the entangling surface should be defined in quantum gravity. Finally, we reanalyze a semi-classical model for black hole evaporation studied in JHEP 1607, 139 (2016) and compute the entanglement between early and late Hawking radiation, illustrating information loss in the semi-classical framework.
Explore related subjects
Keep this discovery
Thomas G. Mertens. 2019-03-25. Towards Black Hole Evaporation in Jackiw-Teitelboim Gravity. https://doi.org/10.1007/jhep07(2019)097
Cite the original work for its findings. Save a collection to share your selection of sources.