Motti Intermediate Physics — HAL: Black Hole Thermodynamics — Hawking Temperature, Bekenstein Entropy, and the Second Law

Black hole thermodynamics in HAL: Hawking temperature identical to GR (ADM normalisation cancels G_eff). Bekenstein entropy enhanced by C0: S^HAL = C0 x S^GR, a +0.73% correction. Evaporation rate faster by C0^2 (time shorter by 1.44%). Second law satisfied via coherential entropy flux of alpha_em x S_BH per evaporation event.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-06-26
DOI
https://doi.org/10.5281/zenodo.20933507
Primary Topic
Black Holes and Theoretical Physics
Type
preprint
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preprint

Motti Intermediate Physics — HAL: Black Hole Thermodynamics — Hawking Temperature, Bekenstein Entropy, and the Second Law

Mordecai Gavila Alvarez
Zenodo (CERN European Organization for Nuclear Research)
Black Holes and Theoretical Physics
preprint

Motti Intermediate Physics — HAL: Black Hole Thermodynamics — Hawking Temperature, Bekenstein Entropy, and the Second Law

Mordecai Gavila Alvarez
preprint en

Abstract

Black hole thermodynamics in HAL: Hawking temperature identical to GR (ADM normalisation cancels G_eff). Bekenstein entropy enhanced by C0: S^HAL = C0 x S^GR, a +0.73% correction. Evaporation rate faster by C0^2 (time shorter by 1.44%). Second law satisfied via coherential entropy flux of alpha_em x S_BH per evaporation event.

Zenodo (CERN European Organization for Nuclear Research)
Valencia Catholic University Saint Vincent Martyr (ES)
Black Holes and Theoretical Physics
DOIOpen Access PDFOpenAlex
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Motti Intermediate Physics — HAL: Black Hole Thermodynamics — Hawking Temperature, Bekenstein Entropy, and the Second Law — Mordecai Gavila Alvarez · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS