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Periodic orbits and observational accretion disk around a Schwarzschild-like black hole surrounded by dark matter halo

Javokhir Sharipov, Institute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, Tashkent 100000, Uzbekistan, Tashkent, 100000, UzbekistanTursunali XamidovTIIAME NRU, Institute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, Tashkent 100000, Tashkent, Tashkent Province, 700000, UzbekistanQiang WuInstitute for Theoretical Physics and Cosmology, Zhejiang University of Technology, 288 Liuhe Road, Hangzhou, Zhejiang, 310023, ChinaSanjar ShaymatovZhejiang University of Technology, Institute for Theoretical Physics and Cosmology, Zheijiang University of Technology, Hangzhou 310023, China, Hangzhou, Zhejiang, 310014, ChinaTao ZhuInstitute for Theoretical Physics and Cosmology, Zhejiang University of Technology, 288 Liuhe Road, Xihu Qu, Hangzhou, Zhejiang, 310014, China
Chinese Physics Cjournal2026
ABI

Аннотация

Abstract In this work, we investigate the dynamics of periodic orbits and the properties of accretion disks around a Schwarzschild-like black hole (BH) immersed in a King-type dark matter (DM) halo. Our analysis focuses on how the presence of the King DM halo influences both the behavior of periodic orbits and the radiative characteristics of the accretion disk. We begin by examining time-like periodic geodesic orbits for various configurations characterized by different energy and angular momentum values, represented by the integers $(z, w, v)$. Furthermore, we explore the effects of the King DM halo on time-like periodic geodesics, marginally bound orbits, and innermost stable circular orbits, thereby providing a deeper understanding of how the DM halo environment modifies the behavior of these stable orbits and timelike particle geodesics. Finally, we analyze the null geodesics and the accretion disk properties by studying their direct and secondary images, redshift distributions, and radiation fluxes as observed at infinity for a range of inclination angles. This approach allows us to gain valuable insights into the spacetime geometry of a Schwarzschild-like BH within the King-type DM halo, its physical and radiative properties in the accretion disk, and the corresponding observational implications.

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