Maqola

Simulated image of the shadow of the Kerr–Newman–NUT–Kiselev black hole in the Rastall gravity with a thin accretion disk

Temurbek MirzaevDepartment of Physics, Center for Field Theory and Particle Physics, Fudan University, Shanghai, 200438, ChinaSong LiSchool of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing, 100049, ChinaBakhtiyor NarzilloevAkfa University, Milliy Bog’ Street 264, Tashkent, 111221, UzbekistanIbrar HussainSchool of Electrical Engineering and Computer Science, National University of Sciences and Technology, H-12, Islamabad, PakistanAhmadjon AbdujabbarovInstitute of Nuclear Physics, Ulugbek 1, Tashkent, 100214, UzbekistanBobomurat AhmedovNational University of Uzbekistan, Tashkent, 100174, Uzbekistan

The European Physical Journal Plusjournal2023en

ABI

Annotatsiya

Annotatsiya mavjud emas.

Mavzular

Astrophysical Phenomena and Observations Pulsars and Gravitational Waves Research Astrophysics and Cosmic Phenomena

Identifikatorlar

DOI: 10.1140/epjp/s13360-022-03632-4

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