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Main Author: Giovannetti, Federico
Format: Recurso digital
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Published: Zenodo 2026
Online Access:https://doi.org/10.5281/zenodo.19202709
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author Giovannetti, Federico
author_facet Giovannetti, Federico
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>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_19202709
institution Zenodo
language
publishDate 2026
publisher Zenodo
record_format zenodo
spellingShingle Emergent Gravitational Pressure from Entanglement Saturation
Giovannetti, Federico
<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>
title Emergent Gravitational Pressure from Entanglement Saturation
url https://doi.org/10.5281/zenodo.19202709