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May 26, 20260 citationsOpen Access

P69: Information Capacity of the ρc Surface in CCEGA — Sρc = e · SBekenstein and the Four Information Channels

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MSMarc López Sánchez

Key Points

  • This research aims to compute the information capacity of the ρc surface in CCEGA black stars.
  • Calculated the information capacity using S_ρc = e · S_Bekenstein(R_final) formula.
  • Analyzed four information channels: GW, infalling matter, Hawking radiation, and GW echoes.
  • Investigated the absence of an AMPS firewall for black stars.
  • For M ≲ 6 M☉, the ρc surface has greater information capacity than a Schwarzschild BH of the same mass.
  • The Page time correction from the e-factor is calculated to be approximately 1.7%.
  • The only currently observable channel for information is GW echoes.

Abstract

We compute the information capacity of the ρc surface of CCEGA black stars. The key result is exact: S_ρc = e · SBekenstein (Rfinal), where e = 2. 718. . . is Euler's number, arising directly from Gₑff (ρc) = GN 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, Rₑff = 1), infalling matter (encoded on surface), Hawking radiation (negligible, TH ~ 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.

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Cite This Study

Marc López Sánchez (2026) studied this question.

synapsesocial.com/papers/6a153a88b5d9c58d83e8d250https://doi.org/10.5281/zenodo.20364279
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