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A new three-dimensional general-relativistic hydrodynamics code

MPG-Autoren

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons20670

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

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Volltexte (frei zugänglich)

1004.3849
(Preprint), 348KB

210.pdf
(beliebiger Volltext), 465KB

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Zitation

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.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000E-F11F-1
Zusammenfassung
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.