EHT-Constrained Analysis of Shadow Deformation in Quantum-Improved Rotating Non-Singular Magnetic Monopole

Fuente: arXiv
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Main Authors: M, Gowtham Sidharth, Das, Sanjit
Format: Preprint
Published: 2026
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author M, Gowtham Sidharth
Das, Sanjit
author_facet M, Gowtham Sidharth
Das, Sanjit
contents We studied the shadow cast by a rotating Bardeen black hole within the framework of asymptotically safe gravity. The null geodesics were analyzed using the Hamilton Jacobi separation method to derive shadow observables. Our findings show that an increase in both the asymptotic safety parameter and the spin parameter leads to a decrease in the apparent shadow size and an increase in shadow distortion. The monopole charge of the black hole played an important role in the shadow profile. Furthermore, we compute the energy emission rate associated with varying values of the asymptotic safety parameter.
format Preprint
id arxiv_https___arxiv_org_abs_2604_04695
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle EHT-Constrained Analysis of Shadow Deformation in Quantum-Improved Rotating Non-Singular Magnetic Monopole
M, Gowtham Sidharth
Das, Sanjit
General Relativity and Quantum Cosmology
We studied the shadow cast by a rotating Bardeen black hole within the framework of asymptotically safe gravity. The null geodesics were analyzed using the Hamilton Jacobi separation method to derive shadow observables. Our findings show that an increase in both the asymptotic safety parameter and the spin parameter leads to a decrease in the apparent shadow size and an increase in shadow distortion. The monopole charge of the black hole played an important role in the shadow profile. Furthermore, we compute the energy emission rate associated with varying values of the asymptotic safety parameter.
title EHT-Constrained Analysis of Shadow Deformation in Quantum-Improved Rotating Non-Singular Magnetic Monopole
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2604.04695