Stationary scalar clouds around maximally rotating linear dilaton black holes

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dc.contributor.authorTokgoz, G.
dc.contributor.authorSakalli, I.
dc.date.accessioned2026-02-06T18:47:44Z
dc.date.issued2017
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractWe investigate the wave dynamics of a charged massive scalar field propagating in a maximally rotating (extremal) linear dilaton black hole geometry. We prove the existence of a discrete and infinite family of resonances describing non-decaying stationary scalar configurations (clouds) enclosing these rapidly rotating black holes. The results obtained signal the potential stationary scalar field distributions (dark matter) around the extremal linear dilaton black holes. In particular, we analytically compute the effective heights of those clouds above the center of the black hole.
dc.identifier.doi10.1088/1361-6382/aa6858
dc.identifier.issn0264-9381
dc.identifier.issn1361-6382
dc.identifier.issue12
dc.identifier.orcid0000-0001-7270-4355
dc.identifier.orcid0000-0001-7827-9476
dc.identifier.scopus2-s2.0-85020383231
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1088/1361-6382/aa6858
dc.identifier.urihttps://hdl.handle.net/11129/14529
dc.identifier.volume34
dc.identifier.wosWOS:000402400500007
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherIop Publishing Ltd
dc.relation.ispartofClassical and Quantum Gravity
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectscalar clouds
dc.subjecteffective height
dc.subjectstationary resonance
dc.subjectconfluent hypergeometric function
dc.subjectLaguerre polynomials
dc.subjectlinear dilaton
dc.subjectdark matter
dc.titleStationary scalar clouds around maximally rotating linear dilaton black holes
dc.typeArticle

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