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Journal Article

A new three-dimensional general-relativistic hydrodynamics code

MPS-Authors

Hawk,  Ian
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Rezzolla,  Luciano
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Fulltext (public)

1004.3849
(Preprint), 348KB

210.pdf
(Any fulltext), 465KB

Supplementary Material (public)
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Citation

Baiotti, L., Hawk, I., Montero, P. J., & Rezzolla, L. (2003). A new three-dimensional general-relativistic hydrodynamics code. Memorie della Società Astronomica Italiana, Suppl., 1, 210-219. Retrieved from http://arxiv.org/abs/1004.3849.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000E-F11F-1
Abstract
We present a new three-dimensional general relativistic hydrodynamics code, the Whisky code. This code incorporates the expertise developed over the past years in the numerical solution of Einstein equations and of the hydrodynamics equations in a curved spacetime, and is the result of a collaboration of several European Institutes. We here discuss the ability of the code to carry out long-term accurate evolutions of the linear and nonlinear dynamics of isolated relativistic stars.