Cosmological General Relativity Black Holes:Kerr vs Kerr-Newman Dynamical Embedding, Conformal Structure, Heat Flux, Anisotropic Stress, Self-Consistent dM/dt=H(t)M(t) and Linear Coupling k=1 versus k=3 Vacuum Coupling and JWST Overmassive SMBHs

We present the complete dynamical embedding of Kerr (Q=0) and Kerr-Newman black holes in Cosmological General Relativity (CGR) defined by.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-09-16
DOI
https://doi.org/10.5281/zenodo.22796239
Primary Topic
Noncommutative and Quantum Gravity Theories
Type
preprint
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preprint

Cosmological General Relativity Black Holes:Kerr vs Kerr-Newman Dynamical Embedding, Conformal Structure, Heat Flux, Anisotropic Stress, Self-Consistent dM/dt=H(t)M(t) and Linear Coupling k=1 versus k=3 Vacuum Coupling and JWST Overmassive SMBHs

Sangwha Yi
Zenodo (CERN European Organization for Nuclear Research)
Noncommutative and Quantum Gravity Theories
preprint

Cosmological General Relativity Black Holes:Kerr vs Kerr-Newman Dynamical Embedding, Conformal Structure, Heat Flux, Anisotropic Stress, Self-Consistent dM/dt=H(t)M(t) and Linear Coupling k=1 versus k=3 Vacuum Coupling and JWST Overmassive SMBHs

Sangwha Yi
preprint en

Abstract

We present the complete dynamical embedding of Kerr (Q=0) and Kerr-Newman black holes in Cosmological General Relativity (CGR) defined by.

Zenodo (CERN European Organization for Nuclear Research)
Daejeon University (KR)
Noncommutative and Quantum Gravity Theories
DOIOpen Access PDFOpenAlex
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Cosmological General Relativity Black Holes:Kerr vs Kerr-Newman Dynamical Embedding, Conformal Structure, Heat Flux, Anisotropic Stress, Self-Consistent dM/dt=H(t)M(t) and Linear Coupling k=1 versus k=3 Vacuum Coupling and JWST Overmassive SMBHs — Sangwha Yi · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS