Computation of fluid flows in non-inertial contracting, expanding, and rotating reference frames
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[1] Symmetries of fluid dynamics with polytropic exponent , 2000, hep-th/0009092.
[2] F. S. Sherman,et al. Unsteady motion of continuous media , 1960 .
[3] Michael L. Norman,et al. The Formation of the First Star in the Universe , 2001, Science.
[4] R. LeVeque,et al. Adaptive Mesh Refinement Using Wave-Propagation Algorithms for Hyperbolic Systems , 1998 .
[5] Alexei M. Khokhlov,et al. Fully Threaded Tree Algorithms for Adaptive Refinement Fluid Dynamics Simulations , 1997, astro-ph/9701194.
[6] Ami Harten,et al. Self adjusting grid methods for one-dimensional hyperbolic conservation laws☆ , 1983 .
[7] H. Trac,et al. A moving frame algorithm for high Mach number hydrodynamics , 2003, astro-ph/0309599.
[8] W. Hillebrandt,et al. Full-star type Ia supernova explosion models , 2005 .
[9] A. I. Saichev,et al. The large-scale structure of the Universe in the frame of the model equation of non-linear diffusion , 1989 .
[10] R. LeVeque. Wave Propagation Algorithms for Multidimensional Hyperbolic Systems , 1997 .
[12] A. Frank,et al. AstroBEAR: AMR for Astrophysical Applications - I: Methods , 2005 .
[13] C. W. Hirt,et al. An Arbitrary Lagrangian-Eulerian Computing Method for All Flow Speeds , 1997 .
[14] R. Salmon,et al. Geophysical Fluid Dynamics , 2019, Classical Mechanics in Geophysical Fluid Dynamics.
[15] William H. Press,et al. Numerical recipes in Fortran 77 : the art of scientificcomputing. , 1992 .
[16] Riccardo Fazio. Numerical Applications of the Scaling Concept , 1999 .
[17] M. L. Norman,et al. Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS-MP , 2005, astro-ph/0511545.
[18] Michael L. Norman,et al. Adaptive-mesh radiation hydrodynamics. I - The radiation transport equation in a completely adaptive coordinate system. II - The radiation and fluid equations in relativistic flows , 1984 .
[19] Following multi-dimensional type Ia supernova explosion models to homologous expansion , 2004, astro-ph/0408296.
[20] The Maximal Kinematical Invariance Group of Fluid Dynamics and Explosion–Implosion Duality , 2000, hep-th/0007199.
[21] O. Jahn,et al. Symmetries of discontinuous flows and the dual Rankine–Hugoniot conditions in fluid dynamics , 2004, math-ph/0407061.
[22] R. Anderson,et al. An arbitrary Lagrangian-Eulerian method with adaptive mesh refinement for the solution of the Euler equations , 2004 .
[23] P. Colella,et al. Local adaptive mesh refinement for shock hydrodynamics , 1989 .
[24] R.,et al. Moving-Mesh Methods for One-Dimensional Hyperbolic Problems Using CLAWPACK , 2003 .
[25] P. Rentrop,et al. Generalized Runge-Kutta methods of order four with stepsize control for stiff ordinary differential equations , 1979 .
[26] J. T. Mendonça,et al. Explosion implosion duality and the laboratory simulation of astrophysical systems , 2000, astro-ph/0003385.
[27] P. Woodward,et al. The Piecewise Parabolic Method (PPM) for Gas Dynamical Simulations , 1984 .
[28] The maximal invariance group of Newton’s equations for a free point particle , 2001, math-ph/0102011.
[29] S. Penner. Physics of shock waves and high-temperature hydrodynamic phenomena - Ya.B. Zeldovich and Yu.P. Raizer (translated from the Russian and then edited by Wallace D. Hayes and Ronald F. Probstein); Dover Publications, New York, 2002, 944 pp., $34. , 2003 .