Particle motion around a static axially symmetric wormhole
Narzilloev B. Malafarina D. Abdujabbarov A. Ahmedov B. Bambi C.
15 September 2021American Physical Society
Physical Review D
2021#104Issue 6
We consider the properties of a static axially symmetric wormhole described by an exact solution of Einsteins field equations and investigate how we can distinguish such a hypothetical object from a black hole. To this aim, we explore the motion of test particles and photons in the equatorial plane of the wormholes space-time and compare it with the particle dynamics in the well-known space-times of Schwarzschild and Kerr black holes. We show that precise simultaneous measurement of test particle motion and photon motion may provide the means to distinguish the wormhole geometry from that of a black hole.
Text of the article Перейти на текст статьи
Center for Field Theory and Particle Physics, Department of Physics, Fudan University, Shanghai, 200438, China
Akfa University, Kichik Halqa Yuli Street 17, Tashkent, 100095, Uzbekistan
Ulugh Beg Astronomical Institute, Astronomy Street 33, Tashkent, 100052, Uzbekistan
Department of Physics, Nazarbayev University, 53 Kabanbay Batyr Avenue, Astana, 010000, Kazakhstan
Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai, 200030, China
Institute of Nuclear Physics, Ulugbek 1, Tashkent, 100214, Uzbekistan
National University of Uzbekistan, Tashkent, 100174, Uzbekistan
Tashkent Institute of Irrigation and Agricultural Mechanization Engineers, Kori Niyoziy 39, Tashkent, 100000, Uzbekistan
Center for Field Theory and Particle Physics
Akfa University
Ulugh Beg Astronomical Institute
Department of Physics
Shanghai Astronomical Observatory
Institute of Nuclear Physics
National University of Uzbekistan
Tashkent Institute of Irrigation and Agricultural Mechanization Engineers
10 лет помогаем публиковать статьи Международный издатель
Книга Публикация научной статьи Волощук 2026 Book Publication of a scientific article 2026