PLUTO: a numerical code for computational astrophysics

Authors
Abstract:
We present a new, versatile numerical code PLUTO, suitable for the solution of high-mach number flow in 1, 2 and 3 spatial dimensions and different systems of coordinates. The code provides a multiphysics (newtonian or relativistic HD or MHD), multialgorithm modular environment particularly oriented toward the treatment of astrophysical flows in th presence of discontinuities. The modular structure exploits a general framework for integrating a system of conservation laws, built on modern Godunov-type shock-capturing schemes. Recently implemented features include Adaptive Mesh Refinement, radiative cooling, resistivity and heat conduction.
Session:
Presentation Type:
Poster
Presenter:
Matsakos Titos
Contact Name:
Matsakos Titos
Email:
matsakos@ph.unito.it
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