Publication:
Investigating the shadows and strong gravitational lensing of modified Bardeen black holes

Simple item page
dc.citedby2
dc.contributor.authorMolla N.U.en_US
dc.contributor.authorAli A.en_US
dc.contributor.authorDebnath U.en_US
dc.contributor.authorGunasekaran S.S.en_US
dc.contributor.authorid57336530700en_US
dc.contributor.authorid56293288600en_US
dc.contributor.authorid6603948771en_US
dc.contributor.authorid55652730500en_US
dc.date.accessioned2025-03-03T07:42:46Z
dc.date.available2025-03-03T07:42:46Z
dc.date.issued2024
dc.description.abstractThis 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.en_US
dc.description.natureFinalen_US
dc.identifier.ArtNo75019
dc.identifier.doi10.1088/1402-4896/ad52cd
dc.identifier.issue7
dc.identifier.scopus2-s2.0-85196091250
dc.identifier.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85196091250&doi=10.1088%2f1402-4896%2fad52cd&partnerID=40&md5=675c9bdcd82ba14634da89fd44cd1881
dc.identifier.urihttps://irepository.uniten.edu.my/handle/123456789/36505
dc.identifier.volume99
dc.publisherInstitute of Physicsen_US
dc.sourceScopus
dc.sourcetitlePhysica Scripta
dc.subjectAstrophysics
dc.subjectGravitation
dc.subjectRelativity
dc.subjectScattering parameters
dc.subjectStars
dc.subjectBardeen black hole
dc.subjectBlack holes
dc.subjectEvent horizon
dc.subjectGraphical representations
dc.subjectGravitational lensing
dc.subjectMeticulous analysis
dc.subjectNull geodesic
dc.subjectS -parameters
dc.subjectSchwarzschild
dc.subjectShadow
dc.subjectBlack holes
dc.titleInvestigating the shadows and strong gravitational lensing of modified Bardeen black holesen_US
dc.typeArticleen_US
dspace.entity.typePublication
Files
Collections
SCOPUS