Enhancing SPH using Moving Least-Squares and Radial Basis Functions
暂无分享,去创建一个
[1] G. Sod. A survey of several finite difference methods for systems of nonlinear hyperbolic conservation laws , 1978 .
[2] K. Salkauskas,et al. Moving least-squares are Backus-Gilbert optimal , 1989 .
[3] Institute of Astronomy, University of Cambridge. Annual report Oct 1990 - Sep 1991. , 1990 .
[4] Steven N. Shore. Magnetic Fields in Astrophysics , 1992 .
[5] Holger Wendland,et al. Piecewise polynomial, positive definite and compactly supported radial functions of minimal degree , 1995, Adv. Comput. Math..
[6] Mark A Fleming,et al. Meshless methods: An overview and recent developments , 1996 .
[7] R. Beatson,et al. Fast evaluation of radial basis functions : methods for two-dimensional polyharmonic splines , 1997 .
[8] J. Monaghan. Smoothed particle hydrodynamics , 2005 .
[9] G. Dilts. MOVING-LEAST-SQUARES-PARTICLE HYDRODYNAMICS-I. CONSISTENCY AND STABILITY , 1999 .
[10] J. Bonet,et al. Variational and momentum preservation aspects of Smooth Particle Hydrodynamic formulations , 1999 .
[11] Gary A. Dilts,et al. Moving least‐squares particle hydrodynamics II: conservation and boundaries , 2000 .
[12] H. Wendland. Local polynomial reproduction and moving least squares approximation , 2001 .
[13] Garching,et al. Smoothed particle hydrodynamics for galaxy‐formation simulations: improved treatments of multiphase gas, of star formation and of supernovae feedback , 2003 .
[14] R. A. Brownlee,et al. Approximation orders for interpolation by surface splines to rough functions , 2004, 0705.4281.
[15] E. Kansa,et al. On Approximate Cardinal Preconditioning Methods for Solving PDEs with Radial Basis Functions , 2005 .