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
Year: 2026
Type: preprint
Abstract: We present the complete dynamical embedding of Kerr (Q=0) and Kerr-Newman black holes in Cosmological General Relativity (CGR) defined by.
Author: Yi, Sangwha
Institution: Daejeon University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W7212361868
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