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Energy Conservation and Hawking Radiation

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arxiv hep-th/0402166 v2 pith:WEBARVKI submitted 2004-02-23 hep-th gr-qc

Maulik K. Parikh This is my paper · ORCID
classification hep-thgr-qc
keywords blackconservationenergyholeapplicableapproximatelycannotconsider
verification ladder T0 review T1 audit T2 compute T3 formal
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The conservation of energy implies that an isolated radiating black hole cannot have an emission spectrum that is precisely thermal. Moreover, the no-hair theorem is only approximately applicable. We consider the implications for the black hole information puzzle.

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Cited by 6 Pith papers

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

  1. New Construction of Black Hole Solution in Non-Commutative Geometry and Their Thermodynamic Properties

    hep-th 2026-03 unverdicted novelty 5.0 of 10

    Non-commutative black hole solutions derived via Seiberg-Witten map on potentials exhibit eliminated temperature divergence, phase transitions, and stable Planck-mass remnants proposed as gravitational dark matter.

  2. Spin effects on particle creation and evaporation in $f(R,T)$ gravity

    gr-qc 2025-10 unverdicted novelty 5.0 of 10

    Spin-dependent particle creation densities, greybody factors, absorption cross sections, and evaporation lifetimes are computed for scalar, vector, tensor, and spinorial modes around black holes in f(R,T) gravity.

  3. Comment on "Quantum tunneling from Schwarzschild black hole in non-commutative gauge theory of gravity"

    gr-qc 2025-07 conditional novelty 4.0 of 10

    A comment claiming that the horizon in a 2024 non-commutative black hole tunneling paper is complex rather than real, and recomputing the tunneling rate under a different twist.

  4. Particle production, absorption, scattering, and geodesics in a Schwarzschild-Hernquist black hole

    gr-qc 2026-02 unverdicted novelty 3.0 of 10

    Embedding a Schwarzschild black hole in a Hernquist dark matter halo suppresses particle creation rates, changes scattering cross sections, and alters null and timelike geodesics relative to the vacuum case.

  5. Modified Fermions Tunneling Radiation from Non-stationary, Axially Symmetric Kerr Black Hole

    hep-th 2019-07 unverdicted novelty 3.0 of 10

    Using a deformed dispersion relation, the Hawking temperature and tunneling rate for fermions from non-stationary Kerr black holes receive corrections dependent on the horizon's angular parameters.

  6. Alternative Derivations of Hawking Radiation

    gr-qc 2025-05 unverdicted novelty 2.0 of 10

    A review chapter that reproduces and compares the tunneling, anomaly, and Green's function derivations of Hawking radiation, recovering the Hawking temperature and noting open justifications.

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