DYNAMICS AROUND SCHWARZSCHILD BLACK HOLE EMBEDDED IN THE DARK MATTER HALO
In this paper, we construct a static, spherically symmetric black hole immersed in a Dehnen- (1,4, ) type dark matter halo. To
explore the effect of the central core dark matter density on the dynamics around the black hole, we selected 2 the density
near the centre remains significantly lower than other cases, confirming that dark matter has minimal presence in the central region.
1. Z. Xu, X. Hou, X. Gong, and J. Wang, JCAP 09, 038 (2018),arXiv:1803.00767 [gr-qc].
2. R. C. Pantig and A. O¨ vgu¨n, JCAP 08, 056 (2022),
3. C. Zhang, T. Zhu, X. Fang, and A.Wang, Phys. Dark Univ. 37, 101078 (2022), arXiv:2201.11352 [gr-qc].
4. A. Al-Badawi and S. Shaymatov, Communications in Theoretical Physics 77, 035402 (2025).
5. K. Boshkayev and D. Malafarina, Mon. Not. Roy. Astron. Soc. 484, 3325 (2019), arXiv:1811.04061 [gr-qc].
6. D. Liu, (2025), arXiv:2501.12213 [gr-qc].
7. D. Shadykul, H. Chakrabarty, and D. Malafarina, (2024), arXiv:2410.18657 [gr-qc].
8. T. Matos and D. Nunez, Rev. Mex. Fis. 51, 71 (2005),arXiv:astro-ph/0303594
9. B. Toshmatov and A. Abdukarimov, Annals Phys. 440, 168845 (2022).
10. C. W. F. Everitt et al., Phys. Rev. Lett. 106, 221101 (2011), arXiv:1105.3456 [gr-qc].
11. C. W. Misner, K. S. Thorne, and J. A. Wheeler, Gravitation
12. W. H. Freeman and Company, San Francisco, 1973.
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