Epicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs

Abstract The study of the quasi-periodic oscillations (QPOs) of X-ray flux observed in the stellar-mass black hole (BH) binaries or quasars can provide a powerful tool for testing the phenomena occurring in strong gravity regime. We thus fit the data of QPOs observed in the well known microquasars a...

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Autores principales:	Misbah Shahzadi, Martin Kološ, Zdeněk Stuchlík, Yousaf Habib
Formato:	article
Lenguaje:	EN
Publicado:	SpringerOpen 2021
Materias:	Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798
Acceso en línea:	https://doaj.org/article/07dbd0c0250a4ce1912831ab2d634929
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spelling	oai:doaj.org-article:07dbd0c0250a4ce1912831ab2d6349292021-12-05T12:09:04ZEpicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs10.1140/epjc/s10052-021-09868-11434-60441434-6052https://doaj.org/article/07dbd0c0250a4ce1912831ab2d6349292021-12-01T00:00:00Zhttps://doi.org/10.1140/epjc/s10052-021-09868-1https://doaj.org/toc/1434-6044https://doaj.org/toc/1434-6052Abstract The study of the quasi-periodic oscillations (QPOs) of X-ray flux observed in the stellar-mass black hole (BH) binaries or quasars can provide a powerful tool for testing the phenomena occurring in strong gravity regime. We thus fit the data of QPOs observed in the well known microquasars as well as active galactic nuclei (AGNs) in the framework of the model of geodesic oscillations of Keplerian disks modified for the epicyclic oscillations of spinning test particles orbiting Kerr BHs. We show that the modified geodesic models of QPOs can explain the observational fixed data from the microquasars and AGNs but not for all sources. We perform a successful fitting of the high frequency QPOs models of epicyclic resonance and its variants, relativistic precession and its variants, tidal disruption, as well as warped disc models, and discuss the corresponding constraints of parameters of the model, which are the spin of the test particle, mass and rotation of the BH.Misbah ShahzadiMartin KološZdeněk StuchlíkYousaf HabibSpringerOpenarticleAstrophysicsQB460-466Nuclear and particle physics. Atomic energy. RadioactivityQC770-798ENEuropean Physical Journal C: Particles and Fields, Vol 81, Iss 12, Pp 1-14 (2021)
institution	DOAJ
collection	DOAJ
language	EN
topic	Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798
spellingShingle	Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 Misbah Shahzadi Martin Kološ Zdeněk Stuchlík Yousaf Habib Epicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs
description	Abstract The study of the quasi-periodic oscillations (QPOs) of X-ray flux observed in the stellar-mass black hole (BH) binaries or quasars can provide a powerful tool for testing the phenomena occurring in strong gravity regime. We thus fit the data of QPOs observed in the well known microquasars as well as active galactic nuclei (AGNs) in the framework of the model of geodesic oscillations of Keplerian disks modified for the epicyclic oscillations of spinning test particles orbiting Kerr BHs. We show that the modified geodesic models of QPOs can explain the observational fixed data from the microquasars and AGNs but not for all sources. We perform a successful fitting of the high frequency QPOs models of epicyclic resonance and its variants, relativistic precession and its variants, tidal disruption, as well as warped disc models, and discuss the corresponding constraints of parameters of the model, which are the spin of the test particle, mass and rotation of the BH.
format	article
author	Misbah Shahzadi Martin Kološ Zdeněk Stuchlík Yousaf Habib
author_facet	Misbah Shahzadi Martin Kološ Zdeněk Stuchlík Yousaf Habib
author_sort	Misbah Shahzadi
title	Epicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs
title_short	Epicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs
title_full	Epicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs
title_fullStr	Epicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs
title_full_unstemmed	Epicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs
title_sort	epicyclic oscillations in spinning particle motion around kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and agns
publisher	SpringerOpen
publishDate	2021
url	https://doaj.org/article/07dbd0c0250a4ce1912831ab2d634929
work_keys_str_mv	AT misbahshahzadi epicyclicoscillationsinspinningparticlemotionaroundkerrblackholeappliedinmodelsfittingthequasiperiodicoscillationsobservedinmicroquasarsandagns AT martinkolos epicyclicoscillationsinspinningparticlemotionaroundkerrblackholeappliedinmodelsfittingthequasiperiodicoscillationsobservedinmicroquasarsandagns AT zdenekstuchlik epicyclicoscillationsinspinningparticlemotionaroundkerrblackholeappliedinmodelsfittingthequasiperiodicoscillationsobservedinmicroquasarsandagns AT yousafhabib epicyclicoscillationsinspinningparticlemotionaroundkerrblackholeappliedinmodelsfittingthequasiperiodicoscillationsobservedinmicroquasarsandagns
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Epicyclic oscillations in spinning particle motion around Kerr black hole applied in models fitting the quasi-periodic oscillations observed in microquasars and AGNs

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