Study computes information capacity in black stars, suggesting new insights into black hole physics.
We compute the information capacity of the ρc surface of CCEGA black stars. The key result is exact: S_ρc = e · S_Bekenstein(R_final), where e = 2.718... is Euler's number, arising directly from G_eff(ρc) = G_N e⁻¹. For M ≲ 6 M☉, the ρc surface stores more information than a Schwarzschild BH of the same mass. The four information channels are analyzed: GW (perfectly reflected, R_eff = 1), infalling matter (encoded on surface), Hawking radiation (negligible, T_H ~ 10⁻⁸ K), and GW echoes (only currently observable channel). There is no AMPS firewall for black stars — the surface is accessible, no simultaneous inside/outside encoding is required. The Page time correction from the e-factor is ~1.7%, exactly calculable.
No takes yet. Share an insight, caveat, or question.
Marc López Sánchez (2026) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: