Simulation of the interaction of oppositely directed particle flows

DOI10.1134/S0965542520100139zbMath1457.85003OpenAlexW3109969774MaRDI QIDQ2214172

Yanyan Li

Publication date: 6 December 2020

Published in: Computational Mathematics and Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0965542520100139

zbMATH Keywords

impactevolutionplanetary systemcosmogony

Mathematics Subject Classification ID

Numerical methods for initial value problems involving ordinary differential equations (65L05) Galactic and stellar structure (85A15) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) Mathematical modeling or simulation for problems pertaining to astronomy and astrophysics (85-10)

Related Items (1)

Energy-Casimir method for the dynamical systems with modified gravitational potential

Cites Work

• Vlasov-Poisson-Poisson equations, critical mass, and Kordylewski clouds
• Three-Dimensional Rigid-Body Collisions With Multiple Contact Points
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