Dynamics of test particles around charged black holes in Einstein-Æther gravity

Author:

Rayimbaev Javlon12345ORCID,Abdujabbarov Ahmadjon34678,Jamil Mubasher91011ORCID,Han Wen-Biao12,Khudoyberdieva Malika46

Affiliation:

1. Institute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, Tashkent 100000, Uzbekistan

2. Akfa University, Milliy Bogh Street 264, Tashkent 111221, Uzbekistan

3. Tashkent State Technical University, Tashkent 100095, Uzbekistan

4. National University of Uzbekistan, Tashkent 100174, Uzbekistan

5. Samarkand State University, University Avenue 15, Samarkand 140104, Uzbekistan

6. Ulugh Beg Astronomical Institute, Astronomy Street 33, Tashkent 100052, Uzbekistan

7. Tashkent Institute of Irrigation and Agricultural Mechanization Engineers, Kori Niyoziy, 39, Tashkent 100000, Uzbekistan

8. Institute of Nuclear Physics, Tashkent 100214, Uzbekistan

9. Institute for Theoretical Physics and Cosmology, Zhejiang University of Technology, Hangzhou 310023, China

10. School of Natural Sciences, National University of Sciences and Technology (NUST), Islamabad 44000, Pakistan

11. Canadian Quantum Research Center, 204-3002, 32 Avenue, Vernon, BC V1T 2L7, Canada

12. Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai 200030, China

Abstract

This paper focuses on the issues of motion of various kinds of charged, magnetized, and neutral test particles in the vicinity of static and spherically symmetric electrically charged black holes in the Einstein-Æther gravitational theory. Our purpose here is to analyze the effects of the free parameters occurring in the Einstein-Æther theory for particle motion in curved spacetime. Specifically, we have studied the stability of circular and radially varying orbits of different kinds of particles by varying the free parameters [Formula: see text] and [Formula: see text], and also varying the particle’s specific energy, specific angular momentum, and electric charge of the black hole. As a special case, we investigate the charged particle motion around the black holes with a uniform magnetic field by checking the characteristics of the particle’s innermost stable circular orbit. Finally, we propose few values of the parameters [Formula: see text] and [Formula: see text] which mimic the behavior of spin of a Kerr black hole to model an astrophysical black hole.

Funder

PIFI fund of Chinese Academy of Sciences

National Key Research and Development Program of China

Zhejiang Provincial Natural Science Foundation of China

Fundamental Research Funds for the Provincial Universities of Zhejiang

National Natural Science Foundation of China

Publisher

World Scientific Pub Co Pte Ltd

Subject

General Physics and Astronomy,Astronomy and Astrophysics,Nuclear and High Energy Physics

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