Pith. sign in

REVIEW 5 cited by

On 4D-Hawing Radiation from Effective Action

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 hep-th/9403018 v1 pith:IBJZD43S submitted 1994-03-03 hep-th

V. Mukhanov , A. Wipf , A. Zelnikov This is my paper · ORCID
classification hep-th
keywords actioneffectiveenergymomentumradiationtensorappliedarbitrary
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
abstract

We determine the $s$-waves contribution of a scalar field to the four dimensional effective action for arbitrary spherically symmetric external gravitational fields. The result is applied to $4d$-black holes and it is shown that the energy momentum tensor derived from the (nonlocal) effective action contains the Hawking radiation. The luminosity is close to the expected one in the $s$-channel. The energy momentum tensor may be used as starting point to study the backreaction problem.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 5 Pith papers

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

  1. Quantum fate of the Choptuik naked singularity

    gr-qc 2026-06 unverdicted novelty 6.0 of 10

    Quantum backreaction generates horizons that cloak the Choptuik naked singularity, reducing its predictability violation to the standard black hole evaporation problem.

  2. The Fate of Nucleated Black Holes in de Sitter Quantum Gravity

    hep-th 2026-05 unverdicted novelty 6.0 of 10

    Nucleated maximal-mass black holes in de Sitter space undergo thermal Hawking evaporation in smooth quantum states and return fully to the empty de Sitter vacuum.

  3. Test of quantum atmosphere in the dimensionally reduced Schwarzschild black hole

    gr-qc 2019-08 conditional novelty 5.0 of 10

    In a dimensionally reduced Schwarzschild black hole, the temperature carried by outgoing Hawking modes vanishes at the horizon, peaks near 1.43 to 1.5 r_h, and approaches the Hawking temperature at infinity.

  4. Wald-like entropy and Islands in Dimensionally Reduced Einstein-Hilbert Gravity

    hep-th 2026-07 conditional novelty 4.0 of 10

    Wald-like Noether charge of the DREH plus Polyakov-Liouville action yields the island generalized entropy and unitary Page curves for eternal and quasi-stationary evaporating black holes.

  5. Anomaly-driven evaporation endpoints of a two-dimensional regular black hole

    hep-th 2026-06 unverdicted novelty 4.0 of 10

    The FFN dilaton-coupled anomaly model applied to the 2D Bardeen-like black hole enforces r_∞=√2 ℓ for quiescent finite-radius branches and excludes most null branches except the borderline p=2 power-law case under str...

Pith tools