pith. sign in

arxiv: gr-qc/0302099 · v1 · pith:34MXKXUZnew · submitted 2003-02-25 · 🌀 gr-qc · hep-th

Horizon Entropy

classification 🌀 gr-qc hep-th
keywords horizonlawsasymptoticbeenblackentropyestablishedhole
0
0 comments X
read the original abstract

Although the laws of thermodynamics are well established for black hole horizons, much less has been said in the literature to support the extension of these laws to more general settings such as an asymptotic de Sitter horizon or a Rindler horizon (the event horizon of an asymptotic uniformly accelerated observer). In the present paper we review the results that have been previously established and argue that the laws of black hole thermodynamics, as well as their underlying statistical mechanical content, extend quite generally to what we call here "causal horizons". The root of this generalization is the local notion of horizon entropy density.

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. Jacobson's thermodynamic approach to classical gravity applied to non-Riemannian geometries: remarks on the simplicity of Nature

    gr-qc 2026-01 unverdicted novelty 7.0

    Jacobson's thermodynamic approach applied to non-Riemannian geometries selects the Einstein-Hilbert action plus a quadratic torsion term as Nature's choice when non-metricity is absent and the metric energy-momentum t...

  2. Searching for primordial features with radio surveys: synergy between the power spectrum and bispectrum

    astro-ph.CO 2026-06 unverdicted novelty 5.0

    Joint power spectrum and bispectrum analysis from future HI intensity mapping surveys improves constraints on primordial feature amplitudes by 30-40% and achieves percent-level precision on oscillation frequencies whe...

  3. Modular theory and affine representations on the Rindler horizon

    hep-th 2026-05 unverdicted novelty 5.0

    Affine group symmetries on the light ray, with dilations implementing modular flow, provide the minimal structure for thermality on the Rindler horizon via the Mellin transform bridge between Minkowski and Rindler modes.

  4. Modave lectures on energy conditions in quantum field theory and semi-classical gravity

    hep-th 2026-05 accept novelty 2.0

    Review of classical energy conditions, their quantum violations, and information-theoretic bounds for semi-classical gravity, based on Modave lectures.