Emergent Spiral Galactic Morphologies via Navier-Stokes Equations and Shear Stress Tension

Luçardo Olivaes, Bruno

doi:10.5281/zenodo.21725187

Published July 31, 2026 | Version v1

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Emergent Spiral Galactic Morphologies via Navier-Stokes Equations and Shear Stress Tension

Luçardo Olivaes, Bruno¹

1. Ouroboros Deep Tech Research Program

This paper investigates a hydrodynamic approach to galaxy formation, modeling galactic mergers via viscous fluid dynamics and shear stress without classical Newtonian or Einsteinian gravitational potentials. Results suggest spiral arms can emerge purely from fluid mechanics.

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Zenodo

License: Creative Commons Attribution 4.0 International

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Created: July 31, 2026
Modified: July 31, 2026

Emergent Spiral Galactic Morphologies via Navier-Stokes Equations and Shear Stress Tension

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