Brane-World Black Hole Solutions via a Confining Potential
M. Heydari-Fard, H. Razmi, H. R. Sepangi

TL;DR
This paper derives spherically symmetric black hole solutions in a brane-world model using a confining potential, revealing a cosmological constant-like effect and a potential explanation for galaxy rotation curves without dark matter.
Contribution
It introduces new brane-world black hole solutions that incorporate a confining potential, linking extra-dimensional effects to observable cosmological phenomena.
Findings
A Schwarzschild-de Sitter solution mimics a cosmological constant effect.
A potential explanation for galaxy rotation curves without dark matter.
Extra terms in brane-world equations can account for accelerated expansion.
Abstract
Using a confining potential, we consider spherically symmetric vacuum (static black hole) solutions in a brane-world scenario. Working with a constant curvature bulk, two interesting cases/solutions are studied. A Schwarzschild-de Sitter black hole solution similar to the standard solution in the presence of a cosmological constant is obtained which confirms the idea that an extra term in the field equations on the brane can play the role of a positive cosmological constant and may be used to account for the accelerated expansion of the universe. The other solution is one in which we can have a proper potential to explain the galaxy rotation curves without assuming the existence of dark matter and without working with new modified theories (modified Newtonian dynamics).
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