Entanglement-Induced Curvature in Neutron Stars: A Preliminary Phenomenological Model for Emergent Spacetime

Entanglement-Induced Curvature in Neutron Stars: A Preliminary Phenomenological Model for Emergent Spacetime | Authorea try { document.documentElement.classList.add('js'); } catch (e) { } var _gaq = _gaq || []; _gaq.push(['_setAccount', 'G-8VDV14Y67G']); _gaq.push(['_trackPageview']); (function() { var ga = document.createElement('script'); ga.type = 'text/javascript'; ga.async = true; ga.src = ('https:' == document.location.protocol ? 'https://ssl' : 'http://www') + '.google-analytics.com/ga.js'; var s = document.getElementsByTagName('script')[0]; s.parentNode.insertBefore(ga, s); })(); Skip to main content Preprints Collections Wiley Open Research IET Open Research Ecological Society of Japan All Collections About About Authorea FAQs Contact Us Quick Search anywhere Search for preprint articles, keywords, etc. Search Search ADVANCED SEARCH SCROLL This is a preprint and has not been peer reviewed. Data may be preliminary. 1 April 2026 V2 Latest version Share on Entanglement-Induced Curvature in Neutron Stars: A Preliminary Phenomenological Model for Emergent Spacetime Authors : Mohammed Hajji 0009-0009-5955-8854 [email protected] and Mohamemd Hajji Authors Info & Affiliations https://doi.org/10.22541/au.177187670.07056120/v2 189 views 83 downloads Contents Abstract Supplementary Material Information & Authors Metrics & Citations View Options References Figures Tables Media Share Abstract We present a preliminary framework where quantum entanglement entropy is a fundamental constituent of spacetime geometry in high-density regimes. We hypothesize that in neutron star cores, entanglement transitions from an area-law to a volume-law scaling, inducing an emergent curvature Λent. This curvature reduces effective inter-particle distances d ef f toward the Planck scale. We derive a modified Tolman-Oppenheimer-Volkoff (TOV) equation incorporating "Entanglement Pressure" Pent. Our model provides insights into the singularity problem, satisfies causality conditions, and suggests testable signatures in gravitational wave observations. For any Question, message me on [email protected] . Supplementary Material File (entanglement_induced_curvature_in_neutron_stars__a_phenomenological_model_for_emergent_spacetime (1).pdf) Download 228.85 KB Information & Authors Information Version history V1 Version 1 23 February 2026 V2 Version 2 01 April 2026 Copyright This work is licensed under a Non Exclusive No Reuse License. Keywords compact objects degeneracy pressure emergent spacetime equation of state holographic principle Authors Affiliations Mohammed Hajji 0009-0009-5955-8854 [email protected] View all articles by this author Mohamemd Hajji Independent Researcher View all articles by this author Metrics & Citations Metrics Article Usage 189 views 83 downloads .FvxKWukQNSOunydq8rnd { width: 100px; } Citations Download citation Mohammed Hajji, Mohamemd Hajji. Entanglement-Induced Curvature in Neutron Stars: A Preliminary Phenomenological Model for Emergent Spacetime. Authorea . 01 April 2026. DOI: https://doi.org/10.22541/au.177187670.07056120/v2 If you have the appropriate software installed, you can download article citation data to the citation manager of your choice. Simply select your manager software from the list below and click Download. For more information or tips please see 'Downloading to a citation manager' in the Help menu . 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