Exploring the shadow of a rotating charged ModMax black hole

dc.contributor.authorKarshiboev, Khurshid
dc.contributor.authorAtamurotov, Farruh
dc.contributor.authorAbdujabbarov, Ahmadjon
dc.contributor.authorOvgun, Ali
dc.contributor.authorReyimberganov, Anvar
dc.date.accessioned2026-02-06T18:48:47Z
dc.date.issued2024
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractThe research presented in this paper discusses the impact that the parameters of charge (Q) and screening factor (gamma) have on properties of the horizon and silhouette of rotating charged ModMax black holes which were reviewed in [Eur. Phys. J. C (2022) 82:1155] recently, building upon previous findings in the field. Furthermore, the study explores the behavior of null geodesics, which can help us better understand the apparent shape of the black hole's silhouette, as well as the distortion parameter and approximate radii of the silhouette that are influenced by the aforementioned parameters, and there are some values of parameter Q which corresponds to data from the Event Horizon Telescope (EHT). Notably, we explore the distortion parameter and approximate radii of the silhouette, revealing that while an increase in gamma leads to a growth in silhouette radius (R s ), it simultaneously reduces the distortion rate (delta s ). Conversely, heightened Q charge results in a reduction of R s accompanied by an increase in delta s . Lastly, the paper analyzes the effects of the black hole's parameters on the effective potential and energy emission: the peak value of the energy emission rate experiences a decrease as the screening factor (gamma) increases, while it increases with higher values of the charge parameter (Q).
dc.description.sponsorshipUzbekistan Ministry for Innovative Development [F-FA-2021-510]; COST Action [CA18108, CA21106]; Scientific and Technological Research Council of Tuerkiye (TUEBIdot;TAK); Abdus Salam International Centre for Theoretical Physics, Trieste, Italy; Sponsoring Consortium for Open Access Publishing in Particle Physics (SCOAP3)
dc.description.sponsorshipThis research is partly supported by Research Grant F-FA-2021-510 of the Uzbekistan Ministry for Innovative Development. A. A thanks Silesian University in Opava for their hospitality during his visit. A. OE would like to acknowledge the contribution of the COST Action CA18108 - Quantum gravity phenomenology in the multi-messenger approach (QG-MM) and the COST Action CA21106 - COSMIC WISPers in the Dark Universe: Theory, astrophysics and experiments (CosmicWISPers). A. OE acknowledges the support received from the Scientific and Technological Research Council of Tuerkiye (TUEB & Idot;TAK), the Abdus Salam International Centre for Theoretical Physics, Trieste, Italy and the Sponsoring Consortium for Open Access Publishing in Particle Physics (SCOAP3).
dc.identifier.doi10.1088/1572-9494/ad1583
dc.identifier.issn0253-6102
dc.identifier.issn1572-9494
dc.identifier.issue2
dc.identifier.orcid0000-0001-7686-1032
dc.identifier.scopus2-s2.0-85184009944
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1088/1572-9494/ad1583
dc.identifier.urihttps://hdl.handle.net/11129/14594
dc.identifier.volume76
dc.identifier.wosWOS:001156770400001
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/openAccess
dc.snmzKA_WoS_20260204
dc.subjectblack hole
dc.subjectModMax gravity
dc.subjectrotating black hole
dc.subjectblack hole shadow
dc.titleExploring the shadow of a rotating charged ModMax black hole
dc.typeArticle

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