CASTRO: A NEW COMPRESSIBLE ASTROPHYSICAL SOLVER. I. HYDRODYNAMICS AND SELF-GRAVITY

By A. Almgren, V. Beckner, John B. Bell, Marcus S. Day, L. Howell, C. Joggerst, M. Lijewski, A. Nonaka, M. Singer, Michael Zingale. 2010

252 citations recorded by the source corpus.

We present a new code, CASTRO, that solves the multicomponent compressible hydrodynamic equations for astrophysical flows including self-gravity, nuclear reactions, and radiation. CASTRO uses an Eulerian grid and incorporates adaptive mesh refinement (AMR). Our approach to AMR uses a nested hierarchy of logically rectangular grids with simultaneous refinement in both space and time. The radiation component of CASTRO will be described in detail in the next paper, Part II, of this series.

Subfields: Applied Mathematics, Astronomy and Astrophysics, Computational Mechanics

View Paper: https://www.semanticscholar.org/paper/8940b68abe289b85b08061216ae083f2e18d9a50

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In Applied Mathematics

  1. Andreas Marek
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  4. Rüdiger Pakmor

In Astronomy and Astrophysics

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In Computational Mechanics

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