Demonstrates how the modulus field modifies singularities in black holes, suggesting a pathway for extending them.
Full backreaction of G_eff on the interior Friedmann equation converts (da/dt)²=K/a (GR, Kretschner ~a⁻⁶, strong singularity) into (da/dt)²=K·a (CCEGA, Kretschner ~a⁻², weak singularity). Both reach a=0 at the same proper time. Curvature divergence is 10⁴⁰ times smaller at a=10⁻¹⁰. CCEGA does not eliminate the singularity but converts it from strong (inextendible) to weak (potentially extendible). The collapse decelerates instead of accelerating. Calculated for Schwarzschild interior via Oppenheimer-Snyder model.
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Marc López Sánchez (2026) studied this question.
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