Foundation · Paper 5
Paper 5 tests spin dependence, Vaidya compatibility, and early-time completeness, sharpening which early IO structures survive as viable theorem routes.
If the theory is correct, the math will just work.
Paper 5 — Kerr Limit and Radiation Phase
Explores three early structural questions: how black-hole spin affects the temperature prediction, whether the Vaidya radiation phase is compatible with an isotropic CMB bath, and what early-time interior physics is required. The analysis favors the Schwarzschild limit, rules out the naive Vaidya null-dust phase for CMB acoustics, and sharpens the framework's early-radiation picture.
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