Charged fuzzy dark matter black holes

被引:5
作者
Yousaf, Z. [1 ]
Almutairi, Bander [2 ]
Khan, S. [3 ]
Bamba, Kazuharu [4 ]
机构
[1] Univ Punjab, Dept Math, Lahore 54590, Pakistan
[2] King Saud Univ, Dept Math, Coll Sci, POB 2455, Riyadh 11451, Saudi Arabia
[3] Univ Agr Faisalabad, Sub Campus Toba Tek Singh, Faisalabad 36050, Pakistan
[4] Fukushima Univ, Fac Symbiot Syst Sci, Fukushima 9601296, Japan
来源
PHYSICS OF THE DARK UNIVERSE | 2024年 / 46卷
关键词
Self-gravitating system; Dark matter; Black holes; Modified theories of gravity; EQUATION-OF-STATE; ELLIPTIC GALAXIES; MASS DENSITY; SUBHALOES; WORMHOLES; MODELS; HALOES; DWARF;
D O I
10.1016/j.dark.2024.101727
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the impact of fuzzy dark matter (FDM) on supermassive black holes (SMBHs) characterized by a spherical charge distribution. This work introduces anew class of spherically symmetric, self-gravitational relativistic charged models for FDM haloes, using the Einasto density model. This study enables the dark matter (DM) to appear as the matter ingredient, which constructs the black hole and extends the non- commutative mini black hole stellar solutions. By considering the charged anisotropic energy-momentum tensor with an equation of state (EoS) pr = - rho, we explore various black hole solutions for different values of the Einasto index and mass parameter. Our approach suggests that the central density of the resulting black hole model mimics the usual de Sitter core. Furthermore, we discuss the possibility of constructing a charged self-gravitational droplet by replacing the above-mentioned EoS with a non-local one. However, under these circumstances, the radial pressure is observed to be negative. Ultimately, we consider various possibilities of constructing DM black holes, featuring intermediate masses that could evolve into galaxies. Consequently, some of these theoretical models have the potential to replace the usual black hole solutions of the galactic core. Simultaneously, these models are physically beneficial for being comprised of the fundamental matter component of the cosmos. Due to the outcomes of this paper, we would be able to study the connection between BH and DM by formulating stable stellar structures featuring fuzzy mass distributions derived from the Einasto distribution of DM halos.
引用
收藏
页数:13
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