Numerical modeling of the collisions of spheroidal galaxies: mass loss efficiency by baryon components

DOI10.1134/S1063454122010149OpenAlexW4281898175MaRDI QIDQ2674740

A. V. Titov, A. V. Khoperskov

Publication date: 14 September 2022

Published in: Vestnik St. Petersburg University. Mathematics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s1063454122010149

zbMATH Keywords

smoothed particle hydrodynamics methodgravitational potential\(N\) body modelgas dynamics modelglobal shock wave

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Particle methods and lattice-gas methods (76M28) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) (n)-body problems (70F10)

Uses Software

• gooPhi

Cites Work

• To the problem of modeling gas flows behind the strong shock wave front using an effective adiabatic index
• New Features of Parallel Implementation of N-Body Problems on GPU
• Numerical Modelling of the Dynamics of the Galactic Halos in the Colliding Galaxies
• Theory and Applications of Smoothed Particle Hydrodynamics

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