Spherically Symmetric Solutions and Dark Matter on the Brane
Dan N. Vollick

TL;DR
This paper explores static, spherically symmetric solutions in a brane-world scenario, suggesting that the five-dimensional Weyl tensor could account for dark matter effects observed in our universe.
Contribution
It provides new solutions to Einstein's equations on a brane, highlighting the role of the Weyl tensor in explaining dark matter phenomena.
Findings
Weyl term can mimic dark matter effects
Solutions differ based on five-dimensional spacetime properties
Not all solutions are Schwarzschild-like
Abstract
It has recently been suggested that our universe is a three-brane embedded in a higher dimensional spacetime. In this paper I examine static, spherically symmetric solutions that satisfy the effective Einstein field equations on a brane embedded in a five dimensional spacetime. The field equations involve a term depending on the five dimensional Weyl tensor, so that the solutions will not be Schwarzschild in general. This Weyl term is traceless so that any solution of is a possible four dimensional spacetime. Different solutions correspond to different five dimensional spacetimes and to different induced energy-momentum tensors on the brane. One interesting possibility is that the Weyl term could be responsible for the observed dark matter in the universe.
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