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Long-lived quasinormal modes in the Euler-Heisenberg electrodynamics

dc.contributor.authorLütfüoglu, Bekir Can
dc.date.accessioned2026-08-18T06:52:35Z
dc.date.issued2025
dc.description.abstractUsing the precise Leaver method and time-domain integration, we analyze the quasinormal modes and late-time behavior of massive neutral and charged scalar fields in the background of a charged, asymptotically flat black hole in the presence of Euler-Heisenberg nonlinear electrodynamics. We show that as the field mass increases, the damping rate decreases significantly, approaching arbitrarily long-lived states known as quasi-resonances. However, these modes cannot be identified in time-domain profiles due to the dominance of asymptotic tails in this regime, which decay slowly and exhibit oscillations with a power-law envelope. We observe that a larger field charge leads to a significantly higher quality factor, as it increases the oscillation frequency while reducing the damping rate.eng
dc.formatp. "Article number: 140026"
dc.identifier.doi10.1016/j.physletb.2025.140026
dc.identifier.issn0370-2693
dc.identifier.obd43882617
dc.identifier.scopus2-s2.0-105022281836
dc.identifier.urihttps://hdl.handle.net/20.500.12603/3032
dc.identifier.wos001625912500001
dc.language.isoeng
dc.peerreviewedyes
dc.project.IDExcellence Project PrF UHK 2205/2025-2026
dc.publicationstatuspostprint
dc.publisherElsevier
dc.relation.ispartofPhysics letters B, volume 871, issue: Decembereng
dc.relation.publisherversionhttps://doi.org/10.1016/j.physletb.2025.140026
dc.rights.accessOpen Access
dc.rights.licenseCC BY
dc.source.urlhttps://doi.org/10.1016/j.physletb.2025.140026
dc.subjectQuasinormal modeseng
dc.subjectEuler-Heisenberg electrodynamicseng
dc.subjectMassive scalar fieldseng
dc.subjectCharged black holeseng
dc.titleLong-lived quasinormal modes in the Euler-Heisenberg electrodynamicseng
dc.typearticle

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