Quasinormal modes of magnetized black hole

dc.contributor.author	Bobir Toshmatov
dc.contributor.author	Zdeněk Stuchlík
dc.contributor.author	Bobomurat Ahmedov
dc.date.accessioned	2025-08-19T04:27:36Z
dc.date.available	2025-08-19T04:27:36Z
dc.date.issued	2018-12-01
dc.description.abstract	We investigate the quasinormal modes (QNMs) of scalar, electromagnetic, and gravitational perturbations in the spacetime of a magnetized black hole. The analysis demonstrates how external magnetic fields modify the QNM spectrum, with implications for the stability of black holes and possible observational signatures. Results show significant differences compared to non-magnetized black holes, offering new insights into astrophysical processes involving strong magnetic fields.	en
dc.identifier.citation	Toshmatov, B.; Stuchlík, Z.; Ahmedov, B. (2018). Quasinormal modes of magnetized black hole. Phys. Rev. D 98, 085021. DOI: 10.1103/PhysRevD.98.085021	en
dc.identifier.doi	10.1103/PhysRevD.98.085021
dc.identifier.other	Filename:85074339234_Quasinormal modes of magnetized black hole.pdf
dc.identifier.uri	https://doi.org/10.1103/PhysRevD.98.085021
dc.identifier.uri	https://nur.nu.edu.kz/handle/123456789/9422
dc.language.iso	en
dc.publisher	American Physical Society (APS)
dc.relation.ispartof	Physical Review D, 98(8), 085021	en
dc.source	Physical Review D, 98(8), 085021 (2018)	en
dc.subject	Black holes Quasinormal modes Magnetized black hole General relativity Astrophysics Perturbation theory	en
dc.title	Quasinormal modes of magnetized black hole	en
dc.type	Journal Article	en

Files

Now showing 1 - 1 of 1