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
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Abstract
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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View paper (DOI)Open access versionOpenAlexZenodo (CERN European Organization for Nuclear Research)Published 2026-09-16
Authors: Sangwha Yi
Institutions: Daejeon University