Advanced numerical methods in astrophysical fluid dynamics

Details Advanced numerical methods in astrophysical fluid dynamics Advanced numerical methods in astrophysical fluid dynamics

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sfa..book..110h&link_type=abstract

Structure Formation in Astrophysics, edited by Gilles Chabrier. Part of the Cambridge Contemporary Astrophysics. ISBN-13: 978-0-

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Computational gas dynamics has become a prominent research field in both astrophysics and cosmology. In the first part of this chapter, we intend to briefly describe several of the numerical methods used in this field, discuss their range of application and present strategies for converting conditionally stable numerical methods into unconditionally stable solution procedures. The underlying aim of the conversion is to enhance the robustness and unification of numerical methods and subsequently enlarge their range of applications considerably. In the second part, Heitsch presents and discusses the implementation of a time-explicit magneto hydrodynamic (MHD) Boltzmann solver.

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