Published August 7, 2012 | Version v1
Journal article

On numerical relativistic hydrodynamics and barotropic equations of state

  • 1. Department of Astronomy and Astrophysics, University of Valencia, E-46100, Burjassot (Spain)
  • 2. Max-Planck-Institute for Astrophysics, Garching, Karl-Schwarzschild-Str. 1, D-85741, Garching (Germany)
  • 3. Department of Applied Physics, University of Alicante, Campus de Sant Vicent del Raspeig, E-03080, Alicante (Spain)

Description

The characteristic formulation of the relativistic hydrodynamic equations (Donat et al 1998 J. Comput. Phys. 146 58), which have been implemented in many relativistic hydro-codes that make use of Godunov-type methods, has to be slightly modified in the case of evolving barotropic flows. For a barotropic equation of state, a removable singularity appears in one of the eigenvectors. The singularity can be avoided by means of a simple renormalization which makes the system of eigenvectors well defined and complete. An alternative strategy for the particular case of barotropic flows is discussed. Communicated by L Rezzolla (note)

Availability note (English)

Available from http://dx.doi.org/10.1088/0264-9381/29/15/157001

Additional details

Publishing Information

Journal Title
Classical and Quantum Gravity
Journal Volume
29
Journal Issue
15
Journal Page Range
[6 p.]
ISSN
0264-9381
CODEN
CQGRDG

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43107879
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CALCULATION METHODS; COSMOLOGICAL MODELS; COSMOLOGY; EIGENVECTORS; EQUATIONS OF STATE; HYDRODYNAMICS; RELATIVISTIC RANGE; RENORMALIZATION; SINGULARITY
Descriptors DEC
ENERGY RANGE; EQUATIONS; FLUID MECHANICS; MATHEMATICAL MODELS; MECHANICS