Pith. sign in

REVIEW 4 cited by

Towards Black Hole Evaporation in Jackiw-Teitelboim Gravity

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1903.10485 v3 pith:5YBGKLR7 submitted 2019-03-25 hep-th

Thomas G. Mertens This is my paper · ORCID
classification hep-th
keywords gravityblackbulkentanglementevaporationholejackiw-teitelboimquantum
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original 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.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The evaporation of black holes in supergravity

    hep-th 2025-04 conditional novelty 8.0 of 10

    Near-BPS black holes in N=2 supergravity emit a discrete spectral line when transitioning to BPS states, and their radiation and absorption spectra deviate strongly from semiclassical black-body predictions.

  2. Falling through the horizon of a quantum black hole

    hep-th 2026-07 conditional novelty 6.5 of 10

    Gravitational dressing in JT gravity lets an infalling Unruh-DeWitt detector detect the horizon location and temperature locally, violating the equivalence principle without a firewall.

  3. Gravitational dynamics of near-extreme Kerr (Anti-)de Sitter black holes

    hep-th 2025-05 conditional novelty 6.0 of 10

    Near-extremal Kerr-dS4 and Kerr-AdS4 black holes admit a sector of metric perturbations whose linearized dynamics is the JT equation, with a Schwarzian effective action for the AdS case.

  4. Jackiw-Teitelboim Model Coupled to Conformal Matter in the Semi-Classical Limit

    hep-th 2019-08 conditional novelty 6.0 of 10

    For JT gravity with conformal matter, the generalized entropy defined from the horizon dilaton plus matter entanglement is monotonic along the event horizon and along future Q-screens under the null energy condition, ...

Pith tools