R-layer Mode Theory (RLMT) XLVI: Unified Gravitational Temperature — Correction and Observational Applications

This volume develops the unified gravitational temperature correction derived from the time‑density formalism of R-layer Mode Theory.The correction is applied to white dwarfs, neutron stars, the solar photosphere and corona, accretion disks, and the CUP‑limit interior of black holes.The framework provides consistent explanations for several long-standing observational puzzles, including neutron‑star cooling discrepancies and high‑energy suppression in accretion disks.A method for stellar mass estimation using R-layer distortions is also proposed.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-06-27
DOI
https://doi.org/10.5281/zenodo.20948270
Primary Topic
Pulsars and Gravitational Waves Research
Type
preprint
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preprint

R-layer Mode Theory (RLMT) XLVI: Unified Gravitational Temperature — Correction and Observational Applications

Tsuyoshi Tohi
Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
preprint

R-layer Mode Theory (RLMT) XLVI: Unified Gravitational Temperature — Correction and Observational Applications

Tsuyoshi Tohi
preprint en

Abstract

This volume develops the unified gravitational temperature correction derived from the time‑density formalism of R-layer Mode Theory.The correction is applied to white dwarfs, neutron stars, the solar photosphere and corona, accretion disks, and the CUP‑limit interior of black holes.The framework provides consistent explanations for several long-standing observational puzzles, including neutron‑star cooling discrepancies and high‑energy suppression in accretion disks.A method for stellar mass estimation using R-layer distortions is also proposed.

Zenodo (CERN European Organization for Nuclear Research)
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