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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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フルテキスト (公開)

1004.3849
(プレプリント), 348KB

210.pdf
(全文テキスト(全般)), 465KB

付随資料 (公開)
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引用

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.


引用: https://hdl.handle.net/11858/00-001M-0000-000E-F11F-1
要旨
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.