pith. sign in

arxiv: hep-th/0402166 · v2 · pith:WEBARVKInew · submitted 2004-02-23 · ✦ hep-th · gr-qc

Energy Conservation and Hawking Radiation

classification ✦ hep-th gr-qc
keywords blackconservationenergyholeapplicableapproximatelycannotconsider
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 4 Pith papers

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

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

    hep-th 2026-03 unverdicted novelty 5.0

    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

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

    gr-qc 2026-02 unverdicted novelty 3.0

    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.

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

    hep-th 2019-07 unverdicted novelty 3.0

    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.