Supercomputer Simulation of an Astrophysical Object Collapse by the Fluids-in-Cell Method
暂无分享,去创建一个
Igor M. Kulikov | Vitalii A. Vshivkov | Galina G. Lazareva | Alexei V. Snytnikov | I. Kulikov | V. Vshivkov | G. Lazareva | A. Snytnikov
[1] A. Whitworth,et al. Adaptive smoothing lengths in SPH , 2007, astro-ph/0701909.
[2] V. Springel,et al. GADGET: a code for collisionless and gasdynamical cosmological simulations , 2000, astro-ph/0003162.
[3] Y. Grigoryev,et al. Numerical "Particle-in-Cell" Methods: Theory and Applications , 2002 .
[4] P. Woodward,et al. The Piecewise Parabolic Method (PPM) for Gas Dynamical Simulations , 1984 .
[5] Nikolay Snytnikov,et al. Strategies for Development of a Parallel Program for Protoplanetary Disc Simulation , 2007, PaCT.
[6] Nikolay Snytnikov,et al. Study of 3D Dynamics of Gravitating Systems Using Supercomputers: Methods and Applications , 2007, PaCT.
[7] O. Kuznetsov,et al. The structure of cool accretion disks in semidetached binaries , 2004 .
[8] A. Whitworth,et al. Resolution requirements for simulating gravitational fragmentation using SPH , 2006 .
[9] A modified fluids-in-cell method for problems of gravitational gas dynamics , 2007 .
[10] N. N. Yanenko,et al. The first differential approximation to finite-difference schemes for hyperbolic systems of equations , 1969 .
[11] P V Kaigorodov,et al. Adaptation of Roe-Osher Scheme for the Computers with Massive-Parallel Architecture. , 2002 .
[12] Vitalii A. Vshivkov,et al. A Multigrid Parallel Program for Protoplanetary Disc Simulation , 2005, PaCT.
[13] J. Monaghan,et al. Shock simulation by the particle method SPH , 1983 .