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

Hamil, Bilel; Lütfüoglu, Bekir Can

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dc.rights.license	CC BY	eng
dc.contributor.author	Hamil, Bilel	cze
dc.contributor.author	Lütfüoglu, Bekir Can	cze
dc.date.accessioned	2025-12-05T15:24:44Z
dc.date.available	2025-12-05T15:24:44Z
dc.date.issued	2025	eng
dc.identifier.issn	0015-8208	eng
dc.identifier.uri	http://hdl.handle.net/20.500.12603/2289
dc.description.abstract	Current 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.format	p. " Article number: 2400105"	eng
dc.language.iso	eng	eng
dc.publisher	J. Wiley	eng
dc.relation.ispartof	Progress of Physics, volume 73, issue: 3	eng
dc.subject	black hole thermodynamics	eng
dc.subject	dark matter and dark energy	eng
dc.subject	Euler-Heisenberg black hole	eng
dc.subject	quasinormal modes	eng
dc.subject	shadows	eng
dc.title	Euler-Heisenberg Black Hole Surrounded by Quintessence in the Background of Perfect Fluid Dark Matter: Thermodynamics, Shadows, and Quasinormal Modes	eng
dc.type	article	eng
dc.identifier.obd	43881720	eng
dc.identifier.wos	001386246000001	eng
dc.identifier.doi	10.1002/prop.202400105	eng
dc.publicationstatus	postprint	eng
dc.peerreviewed	yes	eng
dc.source.url	https://doi.org/10.1002/prop.202400105	cze
dc.relation.publisherversion	https://doi.org/10.1002/prop.202400105	eng
dc.rights.access	Open Access	eng