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/10.1088/0264-9381/29/15/157001Additional details
Identifiers
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