Rotating black hole mimicker surrounded by the string cloud

dc.contributor.authorYang, Yi
dc.contributor.authorLiu, Dong
dc.contributor.authorOvgun, Ali
dc.contributor.authorLambiase, Gaetano
dc.contributor.authorLong, Zheng-Wen
dc.date.accessioned2026-02-06T18:49:01Z
dc.date.issued2024
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractTraversable wormholes and regular black holes usually represent completely different scenarios. But in the black bounce spacetime they can be described by a same line element, which is very attractive. Furthermore, the black hole photos taken by EHT show that black holes have spin, so spin is an indispensable intrinsic property of black holes in the actual Universe. In this work, we derive a rotating black hole mimicker surrounded by the string cloud (SC), which can be interpolated to represent regular black hole spacetime and traversable wormhole spacetime. We investigate the effect of the spin a and SC parameter L on the observables (shadow radius Rs and distortion delta s) and energy emission rate of the black hole mimicker surrounded by the SC. We find that shadow for this spacetime is very sensitive to the L, i.e., the SC parameter can significantly increase the boundary of the shadow.
dc.description.sponsorshipNational Natural Science Foundation of China [12265007, 12261018]; Universities Key Laboratory of System Modeling and Data Mining in Guizhou Province [2023013]; Science and Technology Foundation of Guizhou Province [CA18108]; Italian Istituto Nazionale di Fisica Nucleare (INFN) through the QGSKY project; Ministero dell'Istruzione, Universita e Ricerca (MIUR); COST Action [ZK[2022]YB029]; [CA21106]
dc.description.sponsorshipThis research was funded by the National Natural Science Foundation of China (No. 12265007 and No. 12261018) , Universities Key Laboratory of System Modeling and Data Mining in Guizhou Province (No. 2023013), the Science and Technology Foundation of Guizhou Province (No. ZK[2022]YB029) . The work of G. L. is supported by the Italian Istituto Nazionale di Fisica Nucleare (INFN) through the QGSKY project and by Ministero dell'Istruzione, Universita e Ricerca (MIUR). G. L., and A. OE. would like to acknowledge networking support by the COST Action CA18108 - Quantum gravity phenomenology in the multimessenger approach (QG-MM) . A. OE. would like to acknowledge networking support by the COST Action CA21106 - COSMIC WISPers in the Dark Universe: Theory, astrophysics and experiments (CosmicWISPers) .
dc.identifier.doi10.1103/PhysRevD.109.024002
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.issue2
dc.identifier.orcid0000-0001-7514-4592
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.orcid0000-0001-7574-2330
dc.identifier.orcid0000-0003-1886-8716
dc.identifier.scopus2-s2.0-85181466384
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.109.024002
dc.identifier.urihttps://hdl.handle.net/11129/14692
dc.identifier.volume109
dc.identifier.wosWOS:001174871900007
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Physical Soc
dc.relation.ispartofPhysical Review D
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectDark-Matter
dc.subjectField
dc.subjectMass
dc.titleRotating black hole mimicker surrounded by the string cloud
dc.typeArticle

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