Implicit integrations for SPH in semi-Lagrangian approach: application to the accretion disc modeling in a microquasar

DOI10.1016/j.cpc.2012.11.001zbMath1305.76083arXiv1104.1284OpenAlexW2963419855MaRDI QIDQ483856

G. Lanzafame

Publication date: 17 December 2014

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1104.1284

zbMATH Keywords

convection\(N\)-body simulationsaccretionaccretion discsbinaries: closecataclysmic variableshydrodynamics: methods: numericalstars: novas

Mathematics Subject Classification ID

Finite difference methods applied to problems in fluid mechanics (76M20) Particle methods and lattice-gas methods (76M28) Finite difference methods for initial value and initial-boundary value problems involving PDEs (65M06) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05)

Uses Software

• PDE2D

Cites Work

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