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Euler-Heisenberg Black Hole Surrounded by Quintessence in the Background of Perfect Fluid Dark Matter: Thermodynamics, Shadows, and Quasinormal Modes

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dc.contributor.authorHamil, Bilel
dc.contributor.authorLütfüoglu, Bekir Can
dc.date.accessioned2025-12-05T15:24:44Z
dc.date.available2025-12-05T15:24:44Z
dc.date.issued2025
dc.description.abstractCurrent observations show that a significant fraction of the Universe is composed of dark energy and dark matter. In this paper, the simultaneous effects of these dark sectors on the Euler-Heisenberg black hole are investigated, using the quintessence matter field and perfect fluid to model them. In particular, the black hole's thermodynamics, shadows, and quasinormal modes are studied, and detailed discussions are provided on how these properties change with relatively large or small dark sector components.eng
dc.formatp. &quot; Article number: 2400105&quot;
dc.identifier.doi10.1002/prop.202400105
dc.identifier.issn0015-8208
dc.identifier.obd43881720
dc.identifier.urihttp://hdl.handle.net/20.500.12603/2289
dc.identifier.wos001386246000001
dc.language.isoeng
dc.peerreviewedyes
dc.publicationstatuspostprint
dc.publisherJ. Wiley
dc.relation.ispartofProgress of Physics, volume 73, issue: 3eng
dc.relation.publisherversionhttps://doi.org/10.1002/prop.202400105
dc.rights.accessOpen Access
dc.rights.licenseCC BY
dc.source.urlhttps://doi.org/10.1002/prop.202400105
dc.subjectblack hole thermodynamicseng
dc.subjectdark matter and dark energyeng
dc.subjectEuler-Heisenberg black holeeng
dc.subjectquasinormal modeseng
dc.subjectshadowseng
dc.titleEuler-Heisenberg Black Hole Surrounded by Quintessence in the Background of Perfect Fluid Dark Matter: Thermodynamics, Shadows, and Quasinormal Modeseng
dc.typearticle

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