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| Format: | Recurso digital |
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Zenodo
2026
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| Online Access: | https://doi.org/10.5281/zenodo.19202709 |
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Table of Contents:
- <p>We propose a phenomenological extension of relativistic stellar structure in which an additional pressure term of informational origin emerges from an underlying entanglement network. The saturation parameter χ(r) — the ratio of local entanglement entropy to its Bekenstein-bound maximum — is derived without free parameters and yields a non-arbitrary functional form that modifies the Tolman–Oppenheimer–Volkoff (TOV) equation. In the strong-gravity regime this emergent pressure counteracts gravitational collapse, predicting stable compact configurations beyond the standard TOV mass limit and suppressing singular behavior at small radii.</p>