Smoothed particle hydrodynamics calculations of stellar interactions

DOI10.1016/S0377-0427(99)00159-4zbMath0944.76066arXivastro-ph/9805089WikidataQ57954630 ScholiaQ57954630MaRDI QIDQ1807717

James C. jun. Lombardi, Frederic A. Rasio

Publication date: 20 September 2000

Published in: Journal of Computational and Applied Mathematics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/9805089

zbMATH Keywords

ideal fluidsmoothed particle hydrodynamicsadiabatic evolutioncoalescence of compact binariescollisions between main sequence starsmulti-dimensional Lagrangian methodstellar interactions

Mathematics Subject Classification ID

Particle methods and lattice-gas methods (76M28) Compressible fluids and gas dynamics (76N99) Galactic and stellar dynamics (85A05) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Related Items (5)

Evaluation of weakly compressible SPH variants using derived analytical solutions of Taylor-Couette flows ⋮ Smoothed particle hydrodynamics method for fluid flows, towards industrial applications: motivations, current state, and challenges ⋮ Smoothed particle hydrodynamics (SPH): an overview and recent developments ⋮ The viscous gas ring as an astrophysical test problem for a viscous SPH-code ⋮ Tests of spurious transport in smoothed particle hydrodynamics

Cites Work

• On the problem of penetration in particle methods
• Kernel estimates as a basis for general particle methods in hydrodynamics
• von Neumann stability analysis of smoothed particle hydrodynamics -- suggestions for optimal algorithms
• Beyond N-body: 3D cosmological gas dynamics
• Smoothed particle hydrodynamics: theory and application to non-spherical stars
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