Towards black hole evaporation in Jackiw-Teitelboim gravity

From MaRDI portal
Publication:2317767

DOI10.1007/JHEP07(2019)097zbMATH Open1418.83040arXiv1903.10485WikidataQ112153836 ScholiaQ112153836MaRDI QIDQ2317767

Author name not available (Why is that?)

Publication date: 12 August 2019

Published in: (Search for Journal in Brave)

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.


Full work available at URL: https://arxiv.org/abs/1903.10485



No records found.


No records found.








This page was built for publication: Towards black hole evaporation in Jackiw-Teitelboim gravity

Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q2317767)