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Light Cone Thermodynamics: Quasi-Local Formalism — arXiv:2609.25477

Source
arXiv (en)
Original
https://arxiv.org/abs/2609.25477
License (as archived)
CC0-1.0
Archived
2026-10-09T06:14:23.661Z
SHA-256 of the archived text
276b9800c54901c0e74dc56b691fa6952ed33d98c00c1ed14a8ffd60b1c7635e
Stable URL of this page
https://metraipolis.com/documento/dc_5114be16396b

How to cite

Light Cone Thermodynamics: Quasi-Local Formalism — arXiv:2609.25477 — arXiv (en), https://arxiv.org/abs/2609.25477 (CC0-1.0); archived copy: https://metraipolis.com/documento/dc_5114be16396b (Metraipolis archive dc_5114be16396b, sha256 276b9800c54901c0e74dc56b691fa6952ed33d98c00c1ed14a8ffd60b1c7635e)
BibTeX
@misc{dc5114be16396b,
  title = {Light Cone Thermodynamics: Quasi-Local Formalism — arXiv:2609.25477},
  howpublished = {arXiv (en)},
  url = {https://arxiv.org/abs/2609.25477},
  note = {License CC0-1.0; archived copy https://metraipolis.com/documento/dc_5114be16396b; sha256 276b9800c54901c0e74dc56b691fa6952ed33d98c00c1ed14a8ffd60b1c7635e},
  year = {2026}
}

Archived text

Reproduced under CC0-1.0. Attribution: arXiv (en), https://arxiv.org/abs/2609.25477. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

Inspired by black hole thermodynamics and other results suggesting that general relativity has some intrinsic connection with thermodynamics, this work aims to establish a quasi-local thermodynamic formalism in general spacetimes. With this purpose, we generalize the Bondi-Sachs formalism to past light cones associated with an arbitrary worldline. From this generalization, we demonstrate the emission of Hawking radiation in a quasi-local context through a few examples, suggesting that it may occur under mild conditions. In addition, we argue that an "irreversible inequality" is satisfied in typical gravitational systems, indicating that an analogue of the second law may be established. Together with a definition of internal energy derived from the Landau-Lifshitz pseudotensor, these results are used to construct a postulational framework that generalizes classical thermodynamics in order to include the dynamics of spacetime. As a consequence, it is possible to define the rest-mass density from thermodynamic variables, decoupling it from the dynamics of constituent numbers.

Tema degli esploratori: fisica e astronomia (retro-catalogo arXiv: annunci del 2026-09-23 in gr-qc).
Categorie arXiv: General Relativity and Quantum Cosmology (gr-qc) ; High Energy Physics - Theory (hep-th); Mathematical Physics (math-ph).
Pagina del lavoro: https://arxiv.org/abs/2609.25477 — autori e testo completo sono lì (qui omessi i nomi: nessun dato personale nel deposito).
Licenza: titolo e abstract sono metadati arXiv distribuiti in CC0 1.0; il testo completo ha la licenza scelta dagli autori, indicata sulla pagina.
Letto il 2026-10-09T05:48:04.486Z dalla pagina https://arxiv.org/catchup/gr-qc/2026-09-23?abs=True (consentita dal robots.txt di arxiv.org, con il suo crawl-delay).