SPHS: Smoothed Particle Hydrodynamics with a higher order dissipation switch
暂无分享,去创建一个
[1] G. Bryan,et al. GAS CONDENSATION IN THE GALACTIC HALO , 2011, 1105.4639.
[2] Riccardo Brunino,et al. Hydrodynamic simulations with the Godunov smoothed particle hydrodynamics , 2011 .
[3] J. Read,et al. N-body simulations of gravitational dynamics , 2011, 1105.1082.
[4] Walter Dehnen,et al. Inviscid smoothed particle hydrodynamics , 2010 .
[5] V. Springel. Smoothed Particle Hydrodynamics in Astrophysics , 2010, 1109.2219.
[6] Evghenii Gaburov,et al. Astrophysical Weighted Particle Magnetohydrodynamics , 2010, 1006.4159.
[7] H. Dejonghe,et al. Kelvin-Helmholtz instabilities in smoothed particle hydrodynamics , 2010, 1006.1767.
[8] Sergei Nayakshin,et al. Kelvin-Helmholtz instabilities with Godunov smoothed particle hydrodynamics , 2010 .
[9] Stephan Rosswog,et al. Conservative, special-relativistic smoothed particle hydrodynamics , 2009, J. Comput. Phys..
[10] V. Springel. E pur si muove: Galilean-invariant cosmological hydrodynamical simulations on a moving mesh , 2009, 0901.4107.
[11] Volker Springel,et al. Particle hydrodynamics with tessellation techniques , 2009, 0912.0629.
[12] O. Agertz,et al. Resolving mixing in smoothed particle hydrodynamics , 2009, 0906.0774.
[13] Stephan Rosswog,et al. Astrophysical smooth particle hydrodynamics , 2009, 0903.5075.
[14] New Jersey Institute of Technology,et al. Redistributing hot gas around galaxies: do cool clouds signal a solution to the overcooling problem? , 2008, 0812.2025.
[15] J. Makino,et al. A NECESSARY CONDITION FOR INDIVIDUAL TIME STEPS IN SPH SIMULATIONS , 2008, 0808.0773.
[16] James Wadsley,et al. On the treatment of entropy mixing in numerical cosmology , 2008 .
[17] Daniel J. Price. Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH , 2007, J. Comput. Phys..
[18] Bertrand Alessandrini,et al. An improved SPH method: Towards higher order convergence , 2007, J. Comput. Phys..
[19] Daniel J. Price,et al. magma: a three-dimensional, Lagrangian magnetohydrodynamics code for merger applications , 2007, 0705.1441.
[20] J. Monaghan,et al. Fundamental differences between SPH and grid methods , 2006, astro-ph/0610051.
[21] V. Springel. The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.
[22] Gasoline: a flexible, parallel implementation of TreeSPH , 2003, astro-ph/0303521.
[23] V. Springel,et al. Cosmological smoothed particle hydrodynamics simulations: the entropy equation , 2001, astro-ph/0111016.
[24] Shu-ichiro Inutsuka. Reformulation of Smoothed Particle Hydrodynamics with Riemann Solver , 2002 .
[25] S. Kitsionas,et al. Smoothed Particle Hydrodynamics with particle splitting, applied to self-gravitating collapse , 2002, astro-ph/0203057.
[26] V. Springel,et al. Cosmological SPH simulations: The entropy equation , 2001, astro-ph/0111016.
[27] Gregory G. Howes,et al. Gradient Particle Magnetohydrodynamics: A Lagrangian Particle Code for Astrophysical Magnetohydrodynamics , 2001, astro-ph/0107454.
[28] P. Thomas,et al. Multiphase smoothed-particle hydrodynamics , 2000, astro-ph/0005357.
[29] Atsunori Yonehara,et al. Publications of the Astronomical Society of Australia , 2000 .
[30] M. Steinmetz,et al. The Santa Barbara Cluster Comparison Project: A Comparison of Cosmological Hydrodynamics Solutions , 1999, astro-ph/9906160.
[31] G. Dilts. MOVING-LEAST-SQUARES-PARTICLE HYDRODYNAMICS-I. CONSISTENCY AND STABILITY , 1999 .
[32] Joseph John Monaghan,et al. SPH and Riemann Solvers , 1997 .
[33] J. Monaghan,et al. A Switch to Reduce SPH Viscosity , 1997 .
[34] Francesco Miniati,et al. The Survival of Interstellar Clouds against Kelvin-Helmholtz Instabilities , 1997, astro-ph/9701058.
[35] Joseph P. Morris,et al. A Study of the Stability Properties of Smooth Particle Hydrodynamics , 1996, Publications of the Astronomical Society of Australia.
[36] F. Pearce,et al. Hydra: An Adaptive--Mesh Implementation of PPPM--SPH , 1994, astro-ph/9409058.
[37] Jianqing Fan,et al. Local polynomial modelling and its applications , 1994 .
[38] Zdzislaw Meglicki,et al. 3D structure of truncated accretion discs in close binaries , 1993 .
[39] J. Monaghan. Smoothed particle hydrodynamics , 2005 .
[40] Joseph John Monaghan,et al. The dynamics of interstellar cloud complexes , 1988 .
[41] M. Rees,et al. Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering , 1978 .
[42] J. Monaghan,et al. Smoothed particle hydrodynamics: Theory and application to non-spherical stars , 1977 .
[43] L. Lucy. A numerical approach to the testing of the fission hypothesis. , 1977 .
[44] S. Chandrasekhar. Hydrodynamic and Hydromagnetic Stability , 1961 .