A Hybrid Cosmological Hydrodynamic/N-Body Code Based on a Weighted Essentially Nonoscillatory Scheme
暂无分享,去创建一个
Technology of China | Chi-Wang Shu | Long-Long Feng | Chi-Wang Shu | U. O. Science | Long-Long Feng | Meng-Ping Zhang Center for Astrophysics | Technology of China Division of Applied Mathematics | Brown Univ. Dept. of Mathematics | Univ. of Science
[1] Philippe Montarnal,et al. Real Gas Computation Using an Energy Relaxation Method and High-Order WENO Schemes , 1999 .
[2] Richard Liska,et al. Two-dimensional shallow water equations by composite schemes , 1999 .
[3] S. Noelle. The MoT-ICE: a new high-resolution wave-propagation algorithm for multidimensional systems of conservation laws based on Fey's method of transport , 2000 .
[4] Sergio Pirozzoli,et al. Shock wave–thermal inhomogeneity interactions: Analysis and numerical simulations of sound generation , 2000 .
[5] Richard Liska Burton Wendroff. Composite Schemes For Conservation Laws , 1998 .
[6] R. Giacconi,et al. Evidence for x Rays From Sources Outside the Solar System , 1962 .
[7] Matthias Steinmetz. Grapesph: cosmological smoothed particle hydrodynamics simulations with the special-purpose hardware GRAPE , 1996 .
[8] COSMOS: A Hybrid N-Body/Hydrodynamics Code for Cosmological Problems , 1999, astro-ph/9912339.
[9] Wayne Hu,et al. Power Spectra for Cold Dark Matter and Its Variants , 1997, astro-ph/9710252.
[10] Timothy J. Barth,et al. High-order methods for computational physics , 1999 .
[11] V. Springel,et al. GADGET: a code for collisionless and gasdynamical cosmological simulations , 2000, astro-ph/0003162.
[12] Jeremiah P. Ostriker,et al. A piecewise parabolic method for cosmological hydrodynamics , 1995 .
[13] Chi-Wang Shu,et al. Efficient Implementation of Weighted ENO Schemes , 1995 .
[14] Jeremiah P. Ostriker,et al. Generation of microwave background fluctuations from nonlinear perturbations at the era of galaxy formation , 1986 .
[15] G. Efstathiou,et al. Numerical techniques for large cosmological N-body simulations , 1985 .
[16] Guang-Shan Jiang,et al. A High-Order WENO Finite Difference Scheme for the Equations of Ideal Magnetohydrodynamics , 1999 .
[17] T. N. Stevenson,et al. Fluid Mechanics , 2021, Nature.
[18] S. White,et al. Simulations of dissipative galaxy formation in hierarchically clustering universes – I: Tests of the code , 1993 .
[19] Chi-Wang Shu. Total-variation-diminishing time discretizations , 1988 .
[20] Chi-Wang Shu,et al. Strong Stability-Preserving High-Order Time Discretization Methods , 2001, SIAM Rev..
[21] S. Liang,et al. Numerical simulation of underwater blast-wave focusing using a high-order scheme , 1999 .
[22] Danping Peng,et al. Weighted ENO Schemes for Hamilton-Jacobi Equations , 1999, SIAM J. Sci. Comput..
[23] Yong-Tao Zhang,et al. Resolution of high order WENO schemes for complicated flow structures , 2003 .
[24] K. Olive,et al. Primordial nucleosynthesis redux , 1991 .
[25] Chi-Wang Shu,et al. High Order ENO and WENO Schemes for Computational Fluid Dynamics , 1999 .
[26] Centro internazionale matematico estivo. Session,et al. Advanced Numerical Approximation of Nonlinear Hyperbolic Equations , 1998 .
[27] L. Hernquist,et al. TREESPH: A Unification of SPH with the Hierarchical Tree Method , 1989 .
[28] Chi-Wang Shu,et al. Total variation diminishing Runge-Kutta schemes , 1998, Math. Comput..
[29] L. Sedov. Similarity and Dimensional Methods in Mechanics , 1960 .
[30] Y. Zeldovich,et al. The interaction of matter and radiation in a hot-model universe , 1969 .
[31] G. Bryan,et al. Cosmological Adaptive Mesh Refinement , 1998, astro-ph/9807121.
[32] J. Owen,et al. Adaptive Smoothed Particle Hydrodynamics: Methodology. II. , 1995, astro-ph/9512078.
[33] X-RAY PROPERTIES OF GROUPS OF GALAXIES , 2000, astro-ph/0009379.
[34] A. Evrard. Beyond N-body: 3D cosmological gas dynamics , 1988 .
[35] Nickolay Y. Gnedin,et al. Softened Lagrangian Hydrodynamics for Cosmology , 1995 .
[36] Chi-Wang Shu,et al. High order finite difference and finite volume WENO schemes and discontinuous Galerkin methods for CFD , 2001 .
[37] L. Lucy. A numerical approach to the testing of the fission hypothesis. , 1977 .
[38] Chi-Wang Shu. Essentially non-oscillatory and weighted essentially non-oscillatory schemes for hyperbolic conservation laws , 1998 .
[39] Ue-Li Pen,et al. A High-Resolution Adaptive Moving Mesh Hydrodynamic Algorithm , 1997, astro-ph/9704258.
[40] R. Cen. A hydrodynamic approach to cosmology - Methodology , 1992 .
[41] P. Woodward,et al. The Piecewise Parabolic Method (PPM) for Gas Dynamical Simulations , 1984 .
[42] Jeremiah P. Ostriker,et al. A Cosmological Hydrodynamic Code Based on the Total Variation Diminishing Scheme , 1993 .
[43] R. Teyssier. Cosmological hydrodynamics with adaptive mesh refinement - A new high resolution code called RAMSES , 2001, astro-ph/0111367.
[44] Jaw-Yen Yang,et al. Implicit Weighted ENO Schemes for the Three-Dimensional Incompressible Navier-Stokes Equations , 1998 .
[45] G. Sod. A survey of several finite difference methods for systems of nonlinear hyperbolic conservation laws , 1978 .
[46] M. Norman,et al. ZEUS-2D: A radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. I - The hydrodynamic algorithms and tests. II - The magnetohydrodynamic algorithms and tests , 1992 .
[47] R W Hockney,et al. Computer Simulation Using Particles , 1966 .
[48] Chi-Wang Shu,et al. Monotonicity Preserving Weighted Essentially Non-oscillatory Schemes with Increasingly High Order of Accuracy , 2000 .
[49] F. Pearce,et al. Hydra: An Adaptive--Mesh Implementation of PPPM--SPH , 1994 .
[50] J. Monaghan,et al. Smoothed particle hydrodynamics: Theory and application to non-spherical stars , 1977 .
[51] S. Osher,et al. Uniformly high order accurate essentially non-oscillatory schemes, 111 , 1987 .
[52] E. Bertschinger. SIMULATIONS OF STRUCTURE FORMATION IN THE UNIVERSE , 1998 .
[53] Sergio Pirozzoli,et al. Shock-Wave–Vortex Interactions: Shock and Vortex Deformations, and Sound Production , 2000 .
[54] S. Osher,et al. Weighted essentially non-oscillatory schemes , 1994 .