Test Particles and Quasiperiodic Oscillations around Gravitational Aether Black Holes

被引:14
|
作者
Rayimbaev, Javlon [1 ,2 ,3 ,4 ]
Abdulxamidov, Farrux [5 ,6 ,7 ]
Tojiev, Sardor [5 ,6 ]
Abdujabbarov, Ahmadjon [3 ,4 ,6 ]
Holmurodov, Farhod [8 ]
机构
[1] Natl Res Univ TIIAME, Inst Fundamental & Appl Res, Kori Niyoziy 39, Tashkent 100000, Uzbekistan
[2] Cent Asian Univ, Sch Engn, Tashkent 111221, Uzbekistan
[3] Natl Univ Uzbekistan, Fac Phys, Tashkent 100174, Uzbekistan
[4] Tashkent State Tech Univ, Power Engn Fac, Tashkent 100095, Uzbekistan
[5] New Uzbekistan Univ, Sch Math & Nat Sci, Mustaqillik Ave 54, Tashkent 100007, Uzbekistan
[6] Ulugh Beg Astron Inst, Astron St 33, Tashkent 100052, Uzbekistan
[7] Inst Nucl Phys, Ulugbek 1, Tashkent 100214, Uzbekistan
[8] Namangan State Univ, Fac Math, Boburshoh Str 161, Namangan 160107, Uzbekistan
来源
GALAXIES | 2023年 / 11卷 / 05期
关键词
black holes; gravitational aether fields; test particles; particle collisions; 04.50.-h; 04.40.Dg; 97.60.Gb; MAGNETIZED ORBITS; PRECESSION; MODEL; QPOS;
D O I
10.3390/galaxies11050095
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper is devoted to the analysis of the dynamics of test particles in the vicinity of a black hole within the framework of a gravitational aether model. First, we explored the structure of spacetime by analyzing the curvature scalars. Then, we studied particle dynamics around a black hole using the Hamilton-Jacobi equation.The influence of the aether on the effective potential of the radial motion of test particles around the black hole has been investigated. The dependence of the innermost stable circular orbits (ISCO) on the aether parameter has also been investigated. We also considered particle collision near the black hole in the presence of aether, and studied the fundamental frequencies of the orbital motion of the test particles around the black hole in the presence of aether. Further, we applied the obtained results to the analysis of the upper and lower frequencies of twin-peaked quasiperiodic oscillations (QPOs) occurring near black holes. Finally, we use theoretical and numerical results to obtain constraints on model parameters using observation data in QPO.
引用
收藏
页数:18
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