Geometric, thermodynamic and perturbative properties of Frolov black holes surrounded by a cloud of strings and a global monopole

dc.contributor.authorAl-Badawi, Ahmad
dc.contributor.authorAhmed, Faizuddin
dc.contributor.authorSakalli, Izzet
dc.date.accessioned2026-02-06T18:48:47Z
dc.date.issued2026
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractIn this study, we present a comprehensive analysis of a modified Frolov black hole (BH) model that incorporates two types of topological defects, a global monopole (GM) and a cloud of strings (CS). This composite BH solution is examined from multiple theoretical perspectives to explore the impact of these modifications on the BH's geometric, thermodynamic and dynamical properties. We begin by studying the geometrical optics of the spacetime, focusing on the motion of null geodesics. Key features, such as the effective potential, photon sphere, the force acting on photons and the stability of circular photon orbits, are analyzed in detail. Our results show that the presence of GM and CS significantly affects the spacetime geometry and photon dynamics. In addition, the thermodynamic behavior of the modified BH is also investigated. We derive essential quantities such as the Hawking temperature and entropy, demonstrating how the inclusion of GM and CS leads to deviations from the standard thermodynamic relations observed in classical BH solutions. These deviations may offer valuable insights into quantum gravity and the role of topological defects in BH physics. Furthermore, we examine the BH shadow as an observational signature of the underlying geometry. Our analysis shows that the Frolov parameter tends to reduce the apparent size of the shadow, while the presence of topological defects, particularly GM and CS, enlarges it. In addition, we investigate the perturbative dynamics of the BH by studying both scalar (spin-0), fermionic (spin-1/2) and electromagnetic (spin-1) fields through the massless Klein-Gordon and Maxwell equations, respectively. Using the Wentzel-Kramers-Brillouin approximation, we compute the quasinormal modes (QNMs) for scalar and electromagnetic field perturbations. The results confirm the stability of the BH under small perturbations and show that the QNM frequencies and damping rates are strongly influenced by the Frolov parameter, electric charge, GM and CS.
dc.description.sponsorshipEMU; TUBITAK; ANKOS; SCOAP3; COST [CA22113, CA21106, CA23130]
dc.description.sponsorshipThe authors thank the editor and anonymous referees for their constructive suggestions and comments. We express our sincere gratitude to Prof. Dr Habib Mazharimousavi for his valuable assistance in deriving the explicit form of the NLED Lagrangian corresponding to the charged Frolov BH. His insightful computations and expertize greatly enriched the theoretical foundation of this study. F.A. expresses gratitude to the Inter University Centre for Astronomy and Astrophysics (IUCAA), Pune, India, for a visiting associateship. I.S. acknowledges academic and/or financial support from EMU, TUBITAK, ANKOS and SCOAP3, along with networking support from COST Actions CA22113, CA21106 and CA23130.
dc.identifier.doi10.1088/1572-9494/adfd3f
dc.identifier.issn0253-6102
dc.identifier.issn1572-9494
dc.identifier.issue2
dc.identifier.orcid0000-0003-2196-9622
dc.identifier.orcid0000-0002-3127-3453
dc.identifier.orcid0000-0001-7827-9476
dc.identifier.scopus2-s2.0-105017411676
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1088/1572-9494/adfd3f
dc.identifier.urihttps://hdl.handle.net/11129/14597
dc.identifier.volume78
dc.identifier.wosWOS:001583380800001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherIop Publishing Ltd
dc.relation.ispartofCommunications in Theoretical Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectblack hole
dc.subjectFrolov
dc.subjectglobal monopole
dc.subjectcosmic string
dc.subjectquasinormal modes
dc.subjectthermodynamics
dc.subjectshadow
dc.titleGeometric, thermodynamic and perturbative properties of Frolov black holes surrounded by a cloud of strings and a global monopole
dc.typeArticle

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