Numerical Hydrodynamics in General Relativity.
Ontology highlight
ABSTRACT: The current status of numerical solutions for the equations of ideal general relativistic hydrodynamics is reviewed. With respect to an earlier version of the article, the present update provides additional information on numerical schemes, and extends the discussion of astrophysical simulations in general relativistic hydrodynamics. Different formulations of the equations are presented, with special mention of conservative and hyperbolic formulations well-adapted to advanced numerical methods. A large sample of available numerical schemes is discussed, paying particular attention to solution procedures based on schemes exploiting the characteristic structure of the equations through linearized Riemann solvers. A comprehensive summary of astrophysical simulations in strong gravitational fi
SUBMITTER: Font JA
PROVIDER: S-EPMC5660627 | biostudies-literature | 2003
REPOSITORIES: biostudies-literature
ACCESS DATA