Numerical verification shows the exponential effective gravity predicts neutron star mass, suggesting strong alignment with observations.
First numerical verification of the maximum neutron star mass predicted by the CCEGA framework. TOV equations with G_eff(ρ) = G_N·exp(−ρ/ρ_c) and APR4 EOS yield M_max = 2.330 M☉ and R(1.4 M☉) = 12.63 km, consistent with PSR J0952-0607 and NICER. The exponential functional form is uniquely selected among power-law alternatives. ρ_c = 7.4 ρ_nuc derived independently from QCD transition physics (P18) — not fitted to stellar data. CCEGA Program Paper 34.
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Marc López Sánchez (2026) studied this question.
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