A simple and efficient solver for self-gravity in the DISPATCH astrophysical simulation framework
暂无分享,去创建一个
[1] C. Graziani,et al. AN IMPROVED MULTIPOLE APPROXIMATION FOR SELF-GRAVITY AND ITS IMPORTANCE FOR CORE-COLLAPSE SUPERNOVA SIMULATIONS , 2013, 1307.3135.
[2] R. Klessen,et al. MODELING COLLAPSE AND ACCRETION IN TURBULENT GAS CLOUDS: IMPLEMENTATION AND COMPARISON OF SINK PARTICLES IN AMR AND SPH , 2010, 1001.4456.
[3] Terry Clark,et al. Parallel Computing , 2017, Encyclopedia of GIS.
[4] Wolfgang Straßer,et al. A Parallel Preconditioned Conjugate Gradient Solver for the Poisson Problem on a Multi-GPU Platform , 2010, 2010 18th Euromicro Conference on Parallel, Distributed and Network-based Processing.
[5] J. P. Ramsey,et al. AZEuS: AN ADAPTIVE ZONE EULERIAN SCHEME FOR COMPUTATIONAL MAGNETOHYDRODYNAMICS , 2011, 1112.4390.
[6] F. Hoyle. On the Fragmentation of Gas Clouds Into Galaxies and Stars. , 1953 .
[7] P. Colella,et al. Local adaptive mesh refinement for shock hydrodynamics , 1989 .
[8] Richard I. Klein,et al. Self-gravitational Hydrodynamics with Three-dimensional Adaptive Mesh Refinement: Methodology and Applications to Molecular Cloud Collapse and Fragmentation , 1998 .
[9] James R. Graham,et al. Exploring the formation and evolution of planetary systems : proceedings of the 299th symposium of the International Astronomical Union, held in Victoria, Canada, June 2-7, 2013 , 2013 .
[10] D. A. Clarke. ON THE RELIABILITY OF ZEUS-3D , 2010 .
[11] Paolo Cremonesi,et al. Parallel, distributed and network-based processing , 2006, J. Syst. Archit..
[12] W. Press,et al. Numerical Recipes in Fortran: The Art of Scientific Computing.@@@Numerical Recipes in C: The Art of Scientific Computing. , 1994 .
[13] Michael L. Norman,et al. COSMOLOGICAL ADAPTIVE MESH REFINEMENT MAGNETOHYDRODYNAMICS WITH ENZO , 2010 .
[14] J. Jeans,et al. The Stability of a Spherical Nebula , 1902 .
[15] David Collins,et al. COMPARING NUMERICAL METHODS FOR ISOTHERMAL MAGNETIZED SUPERSONIC TURBULENCE , 2011, 1103.5525.
[16] William H. Press,et al. Numerical recipes in Fortran 77 : the art of scientificcomputing. , 1992 .
[17] Wim Vanroose,et al. Hiding global synchronization latency in the preconditioned Conjugate Gradient algorithm , 2014, Parallel Comput..
[18] R. Teyssier,et al. A high order Godunov scheme with constrained transport and adaptive mesh refinement for astrophysical magnetohydrodynamics , 2006 .
[19] Richard I. Klein,et al. The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-Gravitational Hydrodynamics , 1997 .
[20] R. Teyssier. Cosmological hydrodynamics with adaptive mesh refinement - A new high resolution code called RAMSES , 2001, astro-ph/0111367.
[21] CremonesiPaolo. Parallel, distributed and network-based processing , 2006 .
[22] Hui Li,et al. Cosmological AMR MHD with Enzo , 2009, 0902.2594.
[23] C. Hunter. The Instability of the Collapse of a Self-Gravitating Gas Cloud. , 1962 .
[24] A. Evrard. Beyond N-body: 3D cosmological gas dynamics , 1988 .
[25] M. Bate,et al. Resolution requirements for smoothed particle hydrodynamics calculations with self-gravity , 1997 .
[26] Romain Teyssier,et al. A simple multigrid scheme for solving the Poisson equation with arbitrary domain boundaries , 2011, J. Comput. Phys..
[27] L. H. Howell,et al. CASTRO: A NEW COMPRESSIBLE ASTROPHYSICAL SOLVER. I. HYDRODYNAMICS AND SELF-GRAVITY , 2010, 1005.0114.
[28] P. Bodenheimer,et al. Multiple fragmentation in collapsing protostars , 1993 .
[29] Jacob Trier Frederiksen,et al. photon-plasma: A modern high-order particle-in-cell code , 2012, 1211.4575.