Smoothed particle hydrodynamics and magnetohydrodynamics
暂无分享,去创建一个
[1] Peter A. Thomas,et al. Multiphase smoothed-particle hydrodynamics , 2001 .
[2] Daniel J. Price,et al. Smoothed particle magnetohydrodynamics - III. Multidimensional tests and the B = 0 constraint , 2005, astro-ph/0509083.
[3] Daniel J. Price. Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH , 2007, J. Comput. Phys..
[4] J. Monaghan,et al. Smoothed particle hydrodynamics: Theory and application to non-spherical stars , 1977 .
[5] Daniel J. Price,et al. Variational principles for relativistic smoothed particle hydrodynamics , 2001 .
[6] R W Hockney,et al. Computer Simulation Using Particles , 1966 .
[7] P. Janhunen,et al. A Positive Conservative Method for Magnetohydrodynamics Based on HLL and Roe Methods , 2000 .
[8] Richard P. Nelson,et al. Variable smoothing lengths and energy conservation in smoothed particle hydrodynamics , 1994 .
[9] J. Monaghan,et al. A Switch to Reduce SPH Viscosity , 1997 .
[10] L. Lucy. A numerical approach to the testing of the fission hypothesis. , 1977 .
[11] J. Stone,et al. An unsplit Godunov method for ideal MHD via constrained transport , 2005, astro-ph/0501557.
[12] Michael L. Norman,et al. A test suite for magnetohydrodynamical simulations , 1992 .
[13] Daniel J. Price,et al. An energy‐conserving formalism for adaptive gravitational force softening in smoothed particle hydrodynamics and N‐body codes , 2006, astro-ph/0610872.
[14] C. Munz,et al. Hyperbolic divergence cleaning for the MHD equations , 2002 .
[15] S. Cummins,et al. An SPH Projection Method , 1999 .
[16] Carl Eckart,et al. Variation Principles of Hydrodynamics , 1960 .
[17] Andrea Mignone,et al. A second-order unsplit Godunov scheme for cell-centered MHD: The CTU-GLM scheme , 2009, J. Comput. Phys..
[18] Daniel J. Price,et al. magma: a three-dimensional, Lagrangian magnetohydrodynamics code for merger applications , 2007, 0705.1441.
[19] Pep Español,et al. Smoothed dissipative particle dynamics. , 2003, Physical review. E, Statistical, nonlinear, and soft matter physics.
[20] G. Tóth. The ∇·B=0 Constraint in Shock-Capturing Magnetohydrodynamics Codes , 2000 .
[21] G. Dilts. The moving-least-squares-particle hydrodynamics method (MLSPH) , 1997 .
[22] V. Springel,et al. Thermal conduction in cosmological SPH simulations , 2004, astro-ph/0401456.
[23] V. Springel. The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.
[24] Volker Springel,et al. Particle hydrodynamics with tessellation techniques , 2009, 0912.0629.
[25] Jan Trulsen,et al. Multidimensional MHD Shock Tests of Regularized Smoothed Particle Hydrodynamics , 2006 .
[26] M. Brio,et al. An upwind differencing scheme for the equations of ideal magnetohydrodynamics , 1988 .
[27] Adriano H. CerqueiraElisabete M. de Gouveia Dal Pino,et al. Three-dimensional Magnetohydrodynamic Simulations of Radiatively Cooling, Pulsed Jets , 2001, astro-ph/0103399.
[28] L. Hernquist,et al. TREESPH: A Unification of SPH with the Hierarchical Tree Method , 1989 .
[29] H. Ruder,et al. Smoothed Particle Hydrodynamics: Physical Viscosity and the Simulation of Accretion Disks , 1994 .
[30] David P. Stern,et al. Representation of magnetic fields in space , 1976 .
[31] Garching,et al. Smoothed particle hydrodynamics for galaxy‐formation simulations: improved treatments of multiphase gas, of star formation and of supernovae feedback , 2003 .
[32] J. Hawley,et al. Simulation of magnetohydrodynamic flows: A Constrained transport method , 1988 .
[33] Matthew R. Bate,et al. Smoothed particle hydrodynamics with radiative transfer in the flux-limited diffusion approximation , 2004 .
[34] Dinshaw S. Balsara,et al. Total Variation Diminishing Scheme for Adiabatic and Isothermal Magnetohydrodynamics , 1998 .
[35] Daniel J. Price,et al. The effect of magnetic fields on star cluster formation , 2008, 0801.3293.
[36] J. Monaghan,et al. SPH elastic dynamics , 2001 .
[37] J. Monaghan. SPH without a Tensile Instability , 2000 .
[38] Joseph John Monaghan,et al. Ultrarelativistic SPH , 1997 .
[39] Shu-ichiro Inutsuka. Reformulation of Smoothed Particle Hydrodynamics with Riemann Solver , 2002 .
[40] Daniel J. Price. Smoothed Particle Magnetohydrodynamics – IV. Using the vector potential , 2009, 0909.2469.
[41] Zdzislaw Meglicki. Analysis and Applications of Smoothed Particle Magnetohydrodynamics , 1995 .
[42] Jan Trulsen,et al. Two-dimensional MHD Smoothed Particle Hydrodynamics Stability Analysis , 2004 .
[43] J. Monaghan. Smoothed particle hydrodynamics , 2005 .
[44] Axel Brandenburg,et al. Magnetic field evolution in simulations with Euler potentials , 2009, 0907.1906.
[45] J. Trulsen,et al. Regularized Smoothed Particle Hydrodynamics: A New Approach to Simulating Magnetohydrodynamic Shocks , 2001 .
[46] Daniel J. Price,et al. A comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulence , 2010, 1004.1446.
[47] University of Exeter,et al. On the diffusive propagation of warps in thin accretion discs , 2010, 1002.2973.
[48] A. V Kats. Variational principle and canonical variables in hydrodynamics with discontinuities , 2001 .
[49] Dongsu Ryu,et al. Numerical magnetohydrodynamics in astrophysics: Algorithm and tests for multidimensional flow , 1995 .
[50] J. Robert Buchler,et al. The Numerical Modelling of Nonlinear Stellar Pulsations , 1990 .
[51] Nikolaus A. Adams,et al. A multi-phase SPH method for macroscopic and mesoscopic flows , 2006, J. Comput. Phys..
[52] Paul C. Clark,et al. Protostellar collapse and fragmentation using an MHD gadget , 2010, 1008.3790.
[53] P. Roe,et al. A Solution-Adaptive Upwind Scheme for Ideal Magnetohydrodynamics , 1999 .
[54] Walter Dehnen. Towards optimal softening in three-dimensional N-body codes - I. Minimizing the force error , 2000 .
[55] James R. Murray,et al. SPH simulations of tidally unstable accretion discs in cataclysmic variables , 1995, astro-ph/9511031.
[56] J. Monaghan,et al. A refined particle method for astrophysical problems , 1985 .
[57] Daniel J. Price. SPLASH: An Interactive Visualisation Tool for Smoothed Particle Hydrodynamics Simulations , 2007, Publications of the Astronomical Society of Australia.
[58] H. Pongracic,et al. The Influence of Magnetic Fields on Star Formation , 1996, Publications of the Astronomical Society of Australia.
[59] Paul J. Dellar,et al. A note on magnetic monopoles and the one-dimensional MHD Riemann problem , 2001 .
[60] Daniel J. Price. Magnetic fields in astrophysics , 2004 .
[61] W. Benz. Smooth Particle Hydrodynamics: A Review , 1990 .
[62] R. Salmon. HAMILTONIAN FLUID MECHANICS , 1988 .
[63] George Field. Magnetic helicity in astrophysics , 1986 .
[64] K. Dolag,et al. Magnetic field structure due to the global velocity field in spiral galaxies , 2009, 0905.0351.
[65] P. Español,et al. Voronoi Fluid Particle Model for Euler Equations , 2005 .
[66] G. Dilts. MOVING-LEAST-SQUARES-PARTICLE HYDRODYNAMICS-I. CONSISTENCY AND STABILITY , 1999 .
[67] H. M. P. Couchman,et al. Simulating the formation of a cluster of galaxies , 1992 .
[68] Tom Abel,et al. rpSPH: a novel smoothed particle hydrodynamics algorithm , 2010, 1003.0937.
[69] R. van de Weygaert,et al. Density estimators in particle hydrodynamics DTFE versus regular SPH , 2003, astro-ph/0303071.
[70] Joseph P. Morris,et al. A Study of the Stability Properties of Smooth Particle Hydrodynamics , 1996, Publications of the Astronomical Society of Australia.
[71] Daniel J. Price,et al. Smoothed Particle Magnetohydrodynamics – II. Variational principles and variable smoothing-length terms , 2003, astro-ph/0310790.
[72] H. Couchman,et al. Mesh-refined P3M - A fast adaptive N-body algorithm , 1991 .
[73] Anthony Peter Whitworth,et al. Implementations and tests of Godunov-type particle hydrodynamics , 2003 .
[74] J. Monaghan,et al. Extrapolating B splines for interpolation , 1985 .
[75] James Wadsley,et al. On the treatment of entropy mixing in numerical cosmology , 2008 .
[76] Anthony Peter Whitworth,et al. Modelling ambipolar diffusion with two‐fluid smoothed particle hydrodynamics , 2004 .
[77] K. Dolag,et al. SIMULATING MAGNETIC FIELDS IN THE ANTENNAE GALAXIES , 2009, 0911.3327.
[78] Daniel J. Price,et al. Smoothed Particle Magnetohydrodynamics – I. Algorithm and tests in one dimension , 2003, astro-ph/0310789.
[79] Gregory G. Howes,et al. Gradient Particle Magnetohydrodynamics: A Lagrangian Particle Code for Astrophysical Magnetohydrodynamics , 2001, astro-ph/0107454.
[80] Klaus Dolag,et al. SPH simulations of magnetic fields in galaxy clusters (proceedings) , 1999 .
[81] Roland W. Lewis,et al. A variational formulation based contact algorithm for rigid boundaries in two-dimensional SPH applications , 2004 .
[82] Anthony Peter Whitworth,et al. A new prescription for viscosity in smoothed particle hydrodynamics. , 1996 .
[83] V. Springel,et al. Cosmological smoothed particle hydrodynamics simulations: the entropy equation , 2001, astro-ph/0111016.
[84] L. Brookshaw,et al. A Method of Calculating Radiative Heat Diffusion in Particle Simulations , 1985, Publications of the Astronomical Society of Australia.
[85] Dongsu Ryu,et al. Numerical magetohydrodynamics in astronphysics: Algorithm and tests for one-dimensional flow` , 1995 .
[86] Paul R. Woodward,et al. Extension of the Piecewise Parabolic Method to Multidimensional Ideal Magnetohydrodynamics , 1994 .
[87] J. Monaghan,et al. Fundamental differences between SPH and grid methods , 2006, astro-ph/0610051.
[88] Gabor Toth,et al. Conservative and orthogonal discretization for the Lorentz force , 2002 .
[89] P. Morrison,et al. Hamiltonian description of the ideal fluid , 1998 .
[90] J. Monaghan,et al. Solidification using smoothed particle hydrodynamics , 2005 .
[91] David P. Stern,et al. The motion of magnetic field lines , 1966 .
[92] K. Dolag,et al. An MHD gadget for cosmological simulations , 2008, 0807.3553.
[93] P. Cleary,et al. Conduction Modelling Using Smoothed Particle Hydrodynamics , 1999 .
[94] I. J. Schoenberg. Contributions to the Problem of Approximation of Equidistant Data by Analytic Functions , 1988 .
[95] Stephan Rosswog,et al. Astrophysical smooth particle hydrodynamics , 2009, 0903.5075.
[96] S. Lubow,et al. Dynamics of binary-disk interaction. 1: Resonances and disk gap sizes , 1994 .
[97] F. Harlow,et al. Numerical Calculation of Time‐Dependent Viscous Incompressible Flow of Fluid with Free Surface , 1965 .
[98] Paul W. Cleary,et al. Flow modelling in casting processes , 2002 .
[99] I. J. Schoenberg. Contributions to the problem of approximation of equidistant data by analytic functions. Part A. On the problem of smoothing or graduation. A first class of analytic approximation formulae , 1946 .
[100] Daniel J. Price,et al. The impact of magnetic fields on single and binary star formation , 2007, astro-ph/0702410.
[101] Walter Dehnen,et al. Inviscid smoothed particle hydrodynamics , 2010 .
[102] Joseph John Monaghan,et al. SPH and Riemann Solvers , 1997 .
[103] Dennis W. Quinn,et al. An Analysis of 1-D Smoothed Particle Hydrodynamics Kernels , 1996 .
[104] Tom Abel. rpSPH: a much improved Smoothed Particle Hydrodynamics Algorithm , 2010 .
[105] Daniel J. Price,et al. Magnetic fields and the dynamics of spiral galaxies , 2007, 0710.3558.
[106] Joseph John Monaghan,et al. Energy transfer in a particle α model , 2004 .
[107] G. J. Phillips,et al. A numerical method for three-dimensional simulations of collapsing, isothermal, magnetic gas clouds , 1985 .
[108] Volker Springel,et al. Cosmological SPH simulations: The entropy equation , 2001 .
[109] S Rosswog,et al. Producing Ultrastrong Magnetic Fields in Neutron Star Mergers , 2006, Science.
[110] J. Monaghan. SPH compressible turbulence , 2002, astro-ph/0204118.
[111] Matthew R. Bate,et al. A faster algorithm for smoothed particle hydrodynamics with radiative transfer in the flux‐limited diffusion approximation , 2005 .
[112] Daniel J. Price,et al. Inefficient star formation: the combined effects of magnetic fields and radiative feedback , 2009, 0904.4071.