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Analytical models of supermassive black holes in galaxies surrounded by dark matter halos

Zibo ShenDepartment of Astronomy, School of Astronomy and Space Science, University of Science and Technology of China, Hefei, Anhui 230026, ChinaAnzhong WangGCAP-CASPER, Physics Department, Baylor University, Waco, TX 76798-7316, USAYungui GongDepartment of Physics, School of Physical Science and Technology, Ningbo University, Ningbo, Zhejiang 315211, ChinaShaoyu YinInstitute for Theoretical Physics and Cosmology, Zhejiang University of Technology, Hangzhou 310023, China

2024en

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Annotatsiya

In this Letter, we present five analytical models in closed forms, each representing a supermassive black hole (SMBH) located at the center of a galaxy surrounded by dark matter (DM) halo. The density profile of the halo vanishes inside twice the Schwarzschild radius of the hole and satisfies the weak, strong, and dominant energy conditions. The spacetime are asymptotically flat, and the difference among the models lies in the slopes of the density profiles in the spike and regions far from the center of the galaxy. Three of them represent cusp models, whereas the other two represent core models. With the well-known (generalized) Newman-Janis algorithm, rotating SMBHs with DM halos can be easily constructed from these models.

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Identifikatorlar

DOI: 10.1016/j.physletb.2024.138797

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