Fluid Implicit Particles on Coadjoint Orbits

Fuente: arXiv
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Autori principali: Nabizadeh, Mohammad Sina, Roy-Chowdhury, Ritoban, Yin, Hang, Ramamoorthi, Ravi, Chern, Albert
Natura: Preprint
Pubblicazione: 2024
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author Nabizadeh, Mohammad Sina
Roy-Chowdhury, Ritoban
Yin, Hang
Ramamoorthi, Ravi
Chern, Albert
author_facet Nabizadeh, Mohammad Sina
Roy-Chowdhury, Ritoban
Yin, Hang
Ramamoorthi, Ravi
Chern, Albert
contents We propose Coadjoint Orbit FLIP (CO-FLIP), a high order accurate, structure preserving fluid simulation method in the hybrid Eulerian-Lagrangian framework. We start with a Hamiltonian formulation of the incompressible Euler Equations, and then, using a local, explicit, and high order divergence free interpolation, construct a modified Hamiltonian system that governs our discrete Euler flow. The resulting discretization, when paired with a geometric time integration scheme, is energy and circulation preserving (formally the flow evolves on a coadjoint orbit) and is similar to the Fluid Implicit Particle (FLIP) method. CO-FLIP enjoys multiple additional properties including that the pressure projection is exact in the weak sense, and the particle-to-grid transfer is an exact inverse of the grid-to-particle interpolation. The method is demonstrated numerically with outstanding stability, energy, and Casimir preservation. We show that the method produces benchmarks and turbulent visual effects even at low grid resolutions.
format Preprint
id arxiv_https___arxiv_org_abs_2406_01936
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Fluid Implicit Particles on Coadjoint Orbits
Nabizadeh, Mohammad Sina
Roy-Chowdhury, Ritoban
Yin, Hang
Ramamoorthi, Ravi
Chern, Albert
Graphics
Fluid Dynamics
We propose Coadjoint Orbit FLIP (CO-FLIP), a high order accurate, structure preserving fluid simulation method in the hybrid Eulerian-Lagrangian framework. We start with a Hamiltonian formulation of the incompressible Euler Equations, and then, using a local, explicit, and high order divergence free interpolation, construct a modified Hamiltonian system that governs our discrete Euler flow. The resulting discretization, when paired with a geometric time integration scheme, is energy and circulation preserving (formally the flow evolves on a coadjoint orbit) and is similar to the Fluid Implicit Particle (FLIP) method. CO-FLIP enjoys multiple additional properties including that the pressure projection is exact in the weak sense, and the particle-to-grid transfer is an exact inverse of the grid-to-particle interpolation. The method is demonstrated numerically with outstanding stability, energy, and Casimir preservation. We show that the method produces benchmarks and turbulent visual effects even at low grid resolutions.
title Fluid Implicit Particles on Coadjoint Orbits
topic Graphics
Fluid Dynamics
url https://arxiv.org/abs/2406.01936