Charged quantum Oppenheimer–Snyder model

Abstract In the framework of loop quantum cosmology, particularly within the quantum Oppenheimer–Snyder model, the semiclassical Ashtekar–Pawlowski–Singh (APS) metric is associated with a static, spherically symmetric black hole that incorporates quantum effects derived from the APS metric. This qua...

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Main Author: S. Habib Mazharimousavi
Format: Article
Language:English
Published: SpringerOpen 2025-06-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-025-14410-8
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author S. Habib Mazharimousavi
author_facet S. Habib Mazharimousavi
author_sort S. Habib Mazharimousavi
collection DOAJ
description Abstract In the framework of loop quantum cosmology, particularly within the quantum Oppenheimer–Snyder model, the semiclassical Ashtekar–Pawlowski–Singh (APS) metric is associated with a static, spherically symmetric black hole that incorporates quantum effects derived from the APS metric. This quantum-corrected black hole can be interpreted as a modified Schwarzschild black hole, where the Schwarzschild metric function is adjusted by an additional term proportional to $$\frac{M^{2}}{r^{4}}$$ M 2 r 4 , with r denoting the radial coordinate and M,  the black hole mass. In this study, we show that such a quantum-mechanically modified black hole can arise in the context of nonlinear electrodynamics with either electric or magnetic charge. This charged, quantum-corrected solution is then matched to a dust ball of constant mass $$M_{APS}$$ M APS , governed by the APS metric, at a timelike thin-shell possessing nonzero mass m and electric charge Q or magnetic charge P. Analytically, it is demonstrated that the thin-shell oscillates around an equilibrium radius $$r=R_{eq}$$ r = R eq , which is expressed in terms of $$M_{APS}$$ M APS , m, and Q or P.
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spelling doaj-art-e1f04c06af2b46b687a62c954c44d9c52025-08-20T02:37:35ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-06-018561810.1140/epjc/s10052-025-14410-8Charged quantum Oppenheimer–Snyder modelS. Habib Mazharimousavi0Department of Physics, Faculty of Arts and Sciences, Eastern Mediterranean UniversityAbstract In the framework of loop quantum cosmology, particularly within the quantum Oppenheimer–Snyder model, the semiclassical Ashtekar–Pawlowski–Singh (APS) metric is associated with a static, spherically symmetric black hole that incorporates quantum effects derived from the APS metric. This quantum-corrected black hole can be interpreted as a modified Schwarzschild black hole, where the Schwarzschild metric function is adjusted by an additional term proportional to $$\frac{M^{2}}{r^{4}}$$ M 2 r 4 , with r denoting the radial coordinate and M,  the black hole mass. In this study, we show that such a quantum-mechanically modified black hole can arise in the context of nonlinear electrodynamics with either electric or magnetic charge. This charged, quantum-corrected solution is then matched to a dust ball of constant mass $$M_{APS}$$ M APS , governed by the APS metric, at a timelike thin-shell possessing nonzero mass m and electric charge Q or magnetic charge P. Analytically, it is demonstrated that the thin-shell oscillates around an equilibrium radius $$r=R_{eq}$$ r = R eq , which is expressed in terms of $$M_{APS}$$ M APS , m, and Q or P.https://doi.org/10.1140/epjc/s10052-025-14410-8
spellingShingle S. Habib Mazharimousavi
Charged quantum Oppenheimer–Snyder model
European Physical Journal C: Particles and Fields
title Charged quantum Oppenheimer–Snyder model
title_full Charged quantum Oppenheimer–Snyder model
title_fullStr Charged quantum Oppenheimer–Snyder model
title_full_unstemmed Charged quantum Oppenheimer–Snyder model
title_short Charged quantum Oppenheimer–Snyder model
title_sort charged quantum oppenheimer snyder model
url https://doi.org/10.1140/epjc/s10052-025-14410-8
work_keys_str_mv AT shabibmazharimousavi chargedquantumoppenheimersnydermodel