Astrophysical and electromagnetic emissivity properties of black holes surrounded by a quintessence type exotic fluid in the scalar–vector–tensor modified gravity

Haidar Sheikhahmadi; Saheb Soroushfar; S. N. Sajadi; Tiberiu Harko

doi:10.1140/epjc/s10052-023-11980-3

2022 Impact factor 4.4

Particles and Fields

Open Access

Eur. Phys. J. C (2023) 83: 814
https://doi.org/10.1140/epjc/s10052-023-11980-3

Regular Article - Theoretical Physics

Astrophysical and electromagnetic emissivity properties of black holes surrounded by a quintessence type exotic fluid in the scalar–vector–tensor modified gravity

Haidar Sheikhahmadi¹^,2^,3, Saheb Soroushfar⁴^b, S. N. Sajadi⁵ and Tiberiu Harko⁶^,7^,8

¹ School of Astronomy, Institute for Research in Fundamental Sciences (IPM), P. O. Box 19395-5531, Tehran, Iran
² Center for Space Research, North-West University, Potchefstroom, South Africa
³ Canadian Quantum Research Center, 204-3002 32 Avenue, V1T 2L7, Vernon, BC, Canada
⁴ Department of Physics, College of Sciences, Yasouj University, 75918-74934, Yasouj, Iran
⁵ School of Physics, Institute for Research in Fundamental Sciences (IPM), P. O. Box 19395-5531, Tehran, Iran
⁶ Faculty of Physics, Babes-Bolyai University, Kogalniceanu Street, 400084, Cluj-Napoca, Romania
⁷ Department of Theoretical Physics, National Institute of Physics and Nuclear Engineering (IFIN-HH), 077125, Bucharest, Romania
⁸ Astronomical Observatory, 19 Ciresilor Street, 400487, Cluj-Napoca, Romania

^b saheb.soroushfar@gmail.com, soroush@yu.ac.ir

Received: 12 April 2023
Accepted: 28 August 2023
Published online: 12 September 2023

Abstract

The astrophysical consequences of the presence of a quintessence scalar field on the evolution of the horizon and on the accretion disk surrounding a static black hole, in the scalar–vector–tensor version of modified gravity (MOG), are investigated. The positions of the stable circular orbits of the massive test particles, moving around the central object, are obtained from the extremum of the effective potential. Detailed calculations are also presented to investigate the light deflection, shadow and Shapiro effect for such a black hole. The electromagnetic properties of the accretion disks that form around such black holes are considered in detail. The energy flux and efficiency parameter are estimated analytically and numerically. A comparison with the disk properties in Schwarzschild geometry is also performed. The quantum properties of the black hole are also considered, and the Hawking temperature and the mass loss rate due to the Hawking radiation are considered. The obtained results may lead to the possibility of direct astrophysical tests of black hole type objects in modified gravity theories.

© The Author(s) 2023

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