

] is based on such an approach. It can be interpreted as a
Lax-Wendroff scheme with a conservative TVD (total variation
diminishing) dissipation term. The numerical dissipation term is
local, free of problem dependent parameters and does not require
any characteristic information. This last fact makes the
algorithm extremely simple when applied to any hyperbolic system
of conservation laws.
A relativistic version of Davis' method has been used by Koide
et al. [82
,
81
,
129
] in 2D and 3D simulations of relativistic magneto-hydrodynamic
jets with moderate Lorentz factors. Although the results obtained
are encouraging, the coarse grid zoning used in these simulations
and the relative smallness of the beam flow Lorentz factor (4.56,
beam speed
) does not allow for a comparison with Riemann-solver-based HRSC
methods in the ultra-relativistic limit.


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Numerical Hydrodynamics in Special Relativity
Jose Maria Martí and Ewald Müller http://www.livingreviews.org/lrr-1999-3 © Max-Planck-Gesellschaft. ISSN 1433-8351 Problems/Comments to livrev@aei-potsdam.mpg.de |