Exact Solution to the Galactic Halo Problem via Madelung Hydrodynamic Formalism.

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Authors: Nuñez Martinez ARMANDO
Cited by: 0

Abstract

This research presents the definitive analytical solution to the density divergence problem in galactic halos, widely known as the "cusp-core" problem. By transitioning from the Schrödinger-Poisson framework to the Euler-Madelung hydrodynamic description, this work demonstrates that the intrinsic quantum pressure of the dark matter fluid acts as a fundamental stabilization mechanism. The author, Armando Núñez Martínez, provides a rigorous step-by-step derivation showing that the Bohm quantum potential generates a localized repulsive barrier that grows faster than classical gravitational attraction as r \to 0. This physical constraint necessitates that the density gradient vanishes at the origin, effectively eliminating the singularity predicted by classical \LambdaCDM models. Key Results: Singularity Elimination: Mathematical proof that the Bohm potential prevents gravitational collapse into an infinite density point. Mathematical Necessity: The existence of a finite central density core (\rho_c) is established as a necessary consequence of the stabilization of self-gravitating quantum fluids. Field Unification: The study confirms that physical infinities are mathematically excluded from the architecture of the universe when wave nature and quantum effects are properly accounted for via the Euler-Madelung formalism. Keywords: Dark Matter, Galactic Halos, Quantum Hydrodynamics, Madelung Transformation, Cusp-Core Problem, Bohm Potential, Mathematical Physics.

Fields of Study & Subjects

Galaxies: Formation Evolution Phenomena Dark Matter and Cosmic Phenomena Cosmology and Gravitation Theories

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
15 January 2026