Theories on property loss in Zone ε and causal factors for black hole gravity suggest new insights.
AbstractSupplement VI of fossil gravity theory introduced Zone ε as an independent physical structure and derived its phaseboundary condition t_metric · t_C / t_P² = −1 completely. Three questions remained open: the sequence of propertyloss in Zone ε, the origin of black hole gravity when all matter has entered Zone 0, and the parameter-free derivationof the Hawking temperature without circular reasoning.This supplement answers all three from the existing framework without new assumptions. The sequence of propertyloss follows from characteristic time scales: charge loses localisation first because t_charge < t_C. Mass becomes apoint in time. Spin is the last property because t_spin → ∞. The no-hair theorem is a direct consequence.The neutron star is identified as the only stable Zone-ε site in the universe. The neutron without a spin partner is thecollapse trigger. Black hole gravity follows from the new term Z_S: causal order in Zone 0 produces spacetimecurvature without a mass source term. The Bekenstein-Hawking entropy follows from n_C = ¼ – from the geometry ofthe phase boundary. The Hawking temperature is derived from t_metric^(BH) = 2GM/c³ without circular reasoning. Theinformation paradox resolves through the time-invariance of Zone 0. Four new falsifiable predictions are derived.KeywordsZone ε · Zone 0 · property loss · sequence · neutron star · black hole · causal condensation · Z_S · no-hair theorem · Bekenstein-Hawkingentropy · Hawking temperature · information paradox · unitarity · fossil gravity · LIGO · Einstein TelescopeRelated PublicationsWartenberg, B. (2026): Fossil Gravity. DOI: 10.5281/zenodo.19654996Wartenberg, B. (2026): Supplement V – Zone 4. DOI: 10.5281/zenodo.19683809Wartenberg, B. (2026): Supplement VI – Zone 0 and Zone ε. DOI: 10.5281/zenodo.19765599Bodo Wartenberg · bodo.wartenberg@web.de · May 2026
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