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2026
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| Online Access: | https://doi.org/10.5281/zenodo.19202709 |
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| _version_ | 1866901076984201216 |
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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 |