Pith. sign in

REVIEW 1 cited by

Subtleties in the quasi-classical calculation of Hawking radiation

Not yet reviewed by Pith; the record is open.

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 0805.2653 v2 pith:A6JZBBMQ submitted 2008-05-17 gr-qc hep-th

classification gr-qchep-th
keywords contributionhawkingactioncomingpartquasi-classicalradiationtemperature
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

he quasi-classical method of deriving Hawking radiation is investigated. In order to recover the original Hawking temperature one must take into account a previously ignored contribution coming from the temporal part of the action. This contribution plus a contribution coming from the spatial part of the action gives the correct temperature.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Thermal bath induced suppression of Hawking radiation

    gr-qc 2026-07 reject novelty 5.0 of 10

    A Schwarzschild black hole coupled bilinearly to an environmental scalar field radiates less than Hawking's prediction, according to a semiclassical Keldysh calculation.

Pith tools