Investigating the shadows and strong gravitational lensing of modified Bardeen black holes
This study is dedicated to exploring the distinctive observational features affected by the modified Bardeen black hole through meticulous analysis of its shadow and strong gravitational lensing observations. We thoroughly investigated the impact of the black hole?s parameters q, g and ? on its shad...
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my.uniten.dspace-365052025-03-03T15:42:46Z Investigating the shadows and strong gravitational lensing of modified Bardeen black holes Molla N.U. Ali A. Debnath U. Gunasekaran S.S. 57336530700 56293288600 6603948771 55652730500 Astrophysics Gravitation Relativity Scattering parameters Stars Bardeen black hole Black holes Event horizon Graphical representations Gravitational lensing Meticulous analysis Null geodesic S -parameters Schwarzschild Shadow Black holes This study is dedicated to exploring the distinctive observational features affected by the modified Bardeen black hole through meticulous analysis of its shadow and strong gravitational lensing observations. We thoroughly investigated the impact of the black hole?s parameters q, g and ? on its shadow radius through numerical simulations and graphical representations. Utilizing the Event Horizon Telescope (EHT) data, we constrained the modified Bardeen black hole parameter ? of the modified Bardeen black hole within specific ranges: 0.24 � ? � 1.16 for M87*; and 0.036 � ? � 0.51 for Sgr A *, while maintaining the fixed values g = 0.2 and q = 0.3. This restriction of the modified Bardeen black hole parameter ? by the EHT findings illustrates the viability of modified Bardeen black holes as astrophysical candidates. Additionally, we study strong gravitational lensing and its various observables for the modified Bardeen black hole, comparing its behavior to other astrophysical black holes such as the Schwarzschild (? = 0 = q) and Bardeen (? = 0) black holes. By examining the astrophysical ramifications through strong gravitational lensing, considering supermassive black holes at the center of nearby galaxies, we uncovered that the modified Bardeen black hole exhibits distinct characteristics, offering a quantitative distinction from other black holes such as the Schwarzschild and Bardeen black holes. These findings in astrophysical consequences provide a promising pathway to differentiate the modified black hole from its counterparts in the realm of general relativity. ? 2024 IOP Publishing Ltd. Final 2025-03-03T07:42:46Z 2025-03-03T07:42:46Z 2024 Article 10.1088/1402-4896/ad52cd 2-s2.0-85196091250 https://www.scopus.com/inward/record.uri?eid=2-s2.0-85196091250&doi=10.1088%2f1402-4896%2fad52cd&partnerID=40&md5=675c9bdcd82ba14634da89fd44cd1881 https://irepository.uniten.edu.my/handle/123456789/36505 99 7 75019 Institute of Physics Scopus |
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Astrophysics Gravitation Relativity Scattering parameters Stars Bardeen black hole Black holes Event horizon Graphical representations Gravitational lensing Meticulous analysis Null geodesic S -parameters Schwarzschild Shadow Black holes |
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Astrophysics Gravitation Relativity Scattering parameters Stars Bardeen black hole Black holes Event horizon Graphical representations Gravitational lensing Meticulous analysis Null geodesic S -parameters Schwarzschild Shadow Black holes Molla N.U. Ali A. Debnath U. Gunasekaran S.S. Investigating the shadows and strong gravitational lensing of modified Bardeen black holes |
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This study is dedicated to exploring the distinctive observational features affected by the modified Bardeen black hole through meticulous analysis of its shadow and strong gravitational lensing observations. We thoroughly investigated the impact of the black hole?s parameters q, g and ? on its shadow radius through numerical simulations and graphical representations. Utilizing the Event Horizon Telescope (EHT) data, we constrained the modified Bardeen black hole parameter ? of the modified Bardeen black hole within specific ranges: 0.24 � ? � 1.16 for M87*; and 0.036 � ? � 0.51 for Sgr A *, while maintaining the fixed values g = 0.2 and q = 0.3. This restriction of the modified Bardeen black hole parameter ? by the EHT findings illustrates the viability of modified Bardeen black holes as astrophysical candidates. Additionally, we study strong gravitational lensing and its various observables for the modified Bardeen black hole, comparing its behavior to other astrophysical black holes such as the Schwarzschild (? = 0 = q) and Bardeen (? = 0) black holes. By examining the astrophysical ramifications through strong gravitational lensing, considering supermassive black holes at the center of nearby galaxies, we uncovered that the modified Bardeen black hole exhibits distinct characteristics, offering a quantitative distinction from other black holes such as the Schwarzschild and Bardeen black holes. These findings in astrophysical consequences provide a promising pathway to differentiate the modified black hole from its counterparts in the realm of general relativity. ? 2024 IOP Publishing Ltd. |
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57336530700 |
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57336530700 Molla N.U. Ali A. Debnath U. Gunasekaran S.S. |
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Article |
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Molla N.U. Ali A. Debnath U. Gunasekaran S.S. |
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Molla N.U. |
title |
Investigating the shadows and strong gravitational lensing of modified Bardeen black holes |
title_short |
Investigating the shadows and strong gravitational lensing of modified Bardeen black holes |
title_full |
Investigating the shadows and strong gravitational lensing of modified Bardeen black holes |
title_fullStr |
Investigating the shadows and strong gravitational lensing of modified Bardeen black holes |
title_full_unstemmed |
Investigating the shadows and strong gravitational lensing of modified Bardeen black holes |
title_sort |
investigating the shadows and strong gravitational lensing of modified bardeen black holes |
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Institute of Physics |
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2025 |
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1825816024178491392 |
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