The space-time CE/SE method for solving ultra-relativistic Euler equations
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Publication:634087
DOI10.1016/J.CPC.2010.12.044zbMath1333.76096OpenAlexW2093899040MaRDI QIDQ634087
Publication date: 2 August 2011
Published in: Computer Physics Communications (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/j.cpc.2010.12.044
Black holes (83C57) Finite difference methods for initial value and initial-boundary value problems involving PDEs (65M06) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)
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Cites Work
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- Non-oscillatory central differencing for hyperbolic conservation laws
- On the application of a variant CE/SE method for solving two-dimensional ideal MHD equations
- New algorithms for ultra-relativistic numerical hydrodynamics
- A kinetic beam scheme for relativistic gas dynamics
- Kinetic schemes for the relativistic gas dynamics
- Kinetic schemes for the ultra-relativistic Euler equations.
- The method of space-time conservation element and solution element -- a new approach for solving the Navier-Stokes and Euler equations
- Extension of the piecewise parabolic method to one-dimensional relativistic hydrodynamics
- Capturing shock reflections: An improved flux formula
- The space-time conservation element and solution element method: A new high-resolution and genuinely multidimensional paradigm for solving conservation laws
- Relativistic gasdynamics in two dimensions
- Nonoscillatory Central Schemes for Multidimensional Hyperbolic Conservation Laws
- A BGK-Type Flux-Vector Splitting Scheme for the Ultrarelativistic Euler Equations
- An efficient shock-capturing central-type scheme for multidimensional relativistic flows
- Numerical hydrodynamics in special relativity
- Application of the space-time conservation element and solution element method to one-dimensional convection-diffusion problems
- A space-time conservation element and solution element method for solving the two- and three-dimensional unsteady Euler equations using quadilateral and hexahedral meshes.
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