Fractional-Dimension Gravity reproduces Milky Way rotation curves via a variable dimension D(R) fitted to Gaia data without dark matter.
Fourier and Gegenbauer expansions for a fundamental solution of the Laplacian in the hyperboloid model of hyperbolic geometry
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abstract
Due to the isotropy $d$-dimensional hyperbolic space, there exist a spherically symmetric fundamental solution for its corresponding Laplace-Beltrami operator. On the $R$-radius hyperboloid model of $d$-dimensional hyperbolic geometry with $R>0$ and $d\ge 2$, we compute azimuthal Fourier expansions for a fundamental solution of Laplace's equation. For $d\ge 2$, we compute a Gegenbauer polynomial expansion in geodesic polar coordinates for a fundamental solution of Laplace's equation on this negative-constant sectional curvature Riemannian manifold. In three-dimensions, an addition theorem for the azimuthal Fourier coefficients of a fundamental solution for Laplace's equation is obtained through comparison with its corresponding Gegenbauer expansion.
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2026 1verdicts
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Fractional-Dimension Gravity and the Milky Way Galaxy
Fractional-Dimension Gravity reproduces Milky Way rotation curves via a variable dimension D(R) fitted to Gaia data without dark matter.