Screened Simpson-Visser Black Holes with Asymptotically de-Sitter Core

Fuente: arXiv
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Main Authors: Ahmed, Faizuddin, Al-Badawi, Ahmad, Silva, Edilberto O.
Format: Preprint
Published: 2026
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author Ahmed, Faizuddin
Al-Badawi, Ahmad
Silva, Edilberto O.
author_facet Ahmed, Faizuddin
Al-Badawi, Ahmad
Silva, Edilberto O.
contents In this work, we introduce a screened Simpson-Visser regular solution and perform a comprehensive study of its physical and observational properties. We begin by analyzing the thermodynamic behavior of the black hole, including detailed investigations of the Hawking temperature, Gibbs free energy, and specific heat, which provide insights into its stability and phase structure. Next, we examine the geodesic structure of the spacetime, considering both massless (photon) and massive (timelike) particles. In particular, we study the photon sphere, the corresponding black hole shadow, and the innermost stable circular orbits (ISCO), which are crucial for understanding the motion of matter and light around the black hole. Furthermore, we explore the black hole's energy-emission rate radiation, highlighting the effects of the modified geometry on observational signatures. Finally, we investigate the topological aspects of the black hole, analyzing both the thermodynamic topology and the photon sphere's topological properties. Our analysis demonstrates the intricate interplay between the spacetime geometry, geodesic motion, and black hole thermodynamics, offering a deeper understanding of this class of regular black holes and their potential observational consequences.
format Preprint
id arxiv_https___arxiv_org_abs_2603_11921
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Screened Simpson-Visser Black Holes with Asymptotically de-Sitter Core
Ahmed, Faizuddin
Al-Badawi, Ahmad
Silva, Edilberto O.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this work, we introduce a screened Simpson-Visser regular solution and perform a comprehensive study of its physical and observational properties. We begin by analyzing the thermodynamic behavior of the black hole, including detailed investigations of the Hawking temperature, Gibbs free energy, and specific heat, which provide insights into its stability and phase structure. Next, we examine the geodesic structure of the spacetime, considering both massless (photon) and massive (timelike) particles. In particular, we study the photon sphere, the corresponding black hole shadow, and the innermost stable circular orbits (ISCO), which are crucial for understanding the motion of matter and light around the black hole. Furthermore, we explore the black hole's energy-emission rate radiation, highlighting the effects of the modified geometry on observational signatures. Finally, we investigate the topological aspects of the black hole, analyzing both the thermodynamic topology and the photon sphere's topological properties. Our analysis demonstrates the intricate interplay between the spacetime geometry, geodesic motion, and black hole thermodynamics, offering a deeper understanding of this class of regular black holes and their potential observational consequences.
title Screened Simpson-Visser Black Holes with Asymptotically de-Sitter Core
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2603.11921