Schwarzschild Black Hole in Galaxies Surrounded by a Dark Matter Halo
Ahmad Al-Badawi, Sanjar Shaymatov, Yassine Sekhmani

TL;DR
This paper derives a new Schwarzschild-like black hole solution within Einstein gravity that models a black hole surrounded by a Dehnen-type dark matter halo, analyzing its properties and particle trajectories.
Contribution
It introduces a novel black hole solution incorporating a realistic dark matter halo with a Dehnen profile, extending previous models.
Findings
The solution is static and asymptotically flat.
Curvature and energy conditions are satisfied.
Particle geodesics reveal unique orbital features.
Abstract
In this paper, we derive a novel Schwarzschild-like black hole (BH) solution describing a static and asymptotically flat BH surrounded by a dark matter (DM) halo with a Dehnen-type density distribution in the surrounding environment. We investigate the properties of the obtained BH by studying the curvature properties and energy conditions in Einstein gravity. Furthermore, we explore the features of a novel Schwarzschild-like BH embedded in a DM halo with Dehnen-type density profile by analyzing the timelike geodesics of particles along with BH observable properties.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsRelativity and Gravitational Theory · Astrophysical Phenomena and Observations · Adaptive optics and wavefront sensing
