Emergence of ER=EPR from non-local gravitational energy

Fuente: arXiv
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Main Authors: Jusufi, Kimet, Lobo, Francisco S. N., Saridakis, Emmanuel N., Singleton, Douglas
Format: Preprint
Published: 2025
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author Jusufi, Kimet
Lobo, Francisco S. N.
Saridakis, Emmanuel N.
Singleton, Douglas
author_facet Jusufi, Kimet
Lobo, Francisco S. N.
Saridakis, Emmanuel N.
Singleton, Douglas
contents We construct a class of wormhole geometries supported by the non-local gravitational self-energy that regularizes the particle and black-hole sectors of spacetime. Using this framework, inspired by T-duality, we show that two entangled particles (or particle-black-hole pairs) naturally source an Einstein-Rosen-type geometry in which the required violation of the strong energy condition arises from intrinsic quantum-gravity effects rather than from ad hoc exotic matter, which is matter that violates the null energy condition. We classify the resulting wormholes, analyze their horizons, throat structure and embedding properties, and we identify the exotic energy needed at the minimal surface. Imposing the ER=EPR requirement of non-traversability and the absence of a macroscopic throat, we find that only the zero-throat geometry is compatible with an entanglement-induced Einstein-Rosen bridge, providing a concrete realization of ER=EPR within a fully regular spacetime. Finally, we briefly discuss possible implications for microscopic ER networks from vacuum fluctuations, replica-wormhole interpretations of Hawking radiation, and possible links to entanglement-driven dark-energy scenarios.
format Preprint
id arxiv_https___arxiv_org_abs_2512_05022
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Emergence of ER=EPR from non-local gravitational energy
Jusufi, Kimet
Lobo, Francisco S. N.
Saridakis, Emmanuel N.
Singleton, Douglas
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Quantum Physics
We construct a class of wormhole geometries supported by the non-local gravitational self-energy that regularizes the particle and black-hole sectors of spacetime. Using this framework, inspired by T-duality, we show that two entangled particles (or particle-black-hole pairs) naturally source an Einstein-Rosen-type geometry in which the required violation of the strong energy condition arises from intrinsic quantum-gravity effects rather than from ad hoc exotic matter, which is matter that violates the null energy condition. We classify the resulting wormholes, analyze their horizons, throat structure and embedding properties, and we identify the exotic energy needed at the minimal surface. Imposing the ER=EPR requirement of non-traversability and the absence of a macroscopic throat, we find that only the zero-throat geometry is compatible with an entanglement-induced Einstein-Rosen bridge, providing a concrete realization of ER=EPR within a fully regular spacetime. Finally, we briefly discuss possible implications for microscopic ER networks from vacuum fluctuations, replica-wormhole interpretations of Hawking radiation, and possible links to entanglement-driven dark-energy scenarios.
title Emergence of ER=EPR from non-local gravitational energy
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
Quantum Physics
url https://arxiv.org/abs/2512.05022