Spectral methods in general relativistic astrophysics
arXiv:gr-qc/9811089
Abstract
We present spectral methods developed in our group to solve three-dimensional partial differential equations. The emphasis is put on equations arising from astrophysical problems in the framework of general relativity.
51 pages, elsart (Elsevier Preprint), 19 PostScript figures, submitted to Journal of Computational & Applied Mathematics
References in corpus (10)
- Numerical approach for high precision 3-D relativistic star models
- A Turbulent Model for the Interstellar Medium. II. Magnetic Fields and Rotation
- Numerical models of irrotational binary neutron stars in general relativity
- A relativistic formalism to compute quasi-equilibrium configurations of non-synchronized neutron star binaries
- Gravitational waves from pulsars: emission by the magnetic field induced distortion
- Spontaneous Symmetry Breaking of Rapidly Rotating Stars in General Relativity
- Rapid uniform rotation of protoneutron stars
- Rapid differential rotation of protoneutron stars and constraints on radio pulsars periods
- Spectral methods in general relativity -- toward the simulation of 3D-gravitational collapse of neutron stars
- 3+1 General Relativity in Hyperbolic Form