Non-Linear Electrodynamics in Blandford-Znajek Energy Extraction

dc.contributor.authorCarleo, Amodio
dc.contributor.authorLambiase, Gaetano
dc.contributor.authorOvgun, Ali
dc.date.accessioned2026-02-06T18:29:10Z
dc.date.issued2023
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractNon-linear electrodynamics (NLED) is a generalization of Maxwell's electrodynamics for strong fields. It has significant implications for the study of black holes and cosmology and has been extensively studied in the literature, extending from quantum to cosmological contexts. In this work, two new ways to investigate these non-linear theories are investigated. First, the Blandford-Znajek mechanism is analyzed in light of this promising theoretical context, providing the general form of the extracted power up to second order in the black hole spin parameter a. It is found that, depending on the NLED model, the emitted power can be extremely increased or decreased, and that the magnetic field lines around the black hole seem to become vertical quickly. Considering only separated solutions, it is found that no monopole solutions exist and this could have interesting astrophysical consequences (not considered here). Last but not least, it is attempted to confine the NLED parameters by inducing the amplification of primordial magnetic fields (seeds), thus admitting non-linear theories already during the early stages of the Universe. However, the latter approach proves to be useful for NLED research only in certain models. These (analytical) results emphasize that the behavior of non-linear electromagnetic phenomena strongly depends on the physical context and that only a power-law model seems to have any chance to compete with Maxwell.
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN) Iniziativa Specifica QGSKY; COST Action [CA18108]; Universita degli Studi di Salerno within the CRUI-CARE Agreement
dc.description.sponsorshipThe authors are very grateful to the anonymous reviewers for valuable suggestions that significantly improved the quality of this paper. G.L. and A.C. acknowledge the support by the Istituto Nazionale di Fisica Nucleare (INFN) Iniziativa Specifica QGSKY. G.L. and A.OE. would like to acknowledge networking support by the COST Action CA18108- Quantum gravity phenomenology in the multi-messenger approach (QG-MM). Open Access Funding provided by Universita degli Studi di Salerno within the CRUI-CARE Agreement.
dc.identifier.doi10.1002/andp.202200635
dc.identifier.issn0003-3804
dc.identifier.issn1521-3889
dc.identifier.issue5
dc.identifier.orcid0000-0001-9929-2370
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.orcid0000-0001-7574-2330
dc.identifier.scopus2-s2.0-85151647098
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1002/andp.202200635
dc.identifier.urihttps://hdl.handle.net/11129/11309
dc.identifier.volume535
dc.identifier.wosWOS:000962712400001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWiley-V C H Verlag Gmbh
dc.relation.ispartofAnnalen Der Physik
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectblack holes
dc.subjectBlandford-Znajek
dc.subjectenergy extraction
dc.subjectnon-linear electrodynamics
dc.titleNon-Linear Electrodynamics in Blandford-Znajek Energy Extraction
dc.typeArticle

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