Gianluigi Bodo

TL;DR: PLUTO as mentioned in this paper is a multiphysics, multialgorithm modular environment particularly oriented toward the treatment of astrophysical flows in presence of discontinuities, and it exploits a general framework for integrating a system of conservation laws, built on modern Godunov-type shockcapturing schemes.

TL;DR: The adaptive mesh refinement (AMR) as mentioned in this paper implementation of the PLUTO code for solving the equations of classical and relativistic magnetohydrodynamics (MHD and RMHD) exploits, in addition to the static grid version of the code, the distributed infrastructure of the CHOMBO library for multidimensional parallel computations over block-structured, adaptively refined grids.

TL;DR: An extension of the adaptive mesh refinement (AMR) implementation of the PLUTO code to include non-ideal dissipative processes such as viscosity, resistivity and anisotropic thermal conduction without operator splitting is described.

TL;DR: In this article, the authors present self-consistent, time-dependent simulations of supersonic jets launched from magnetized accretion disks, using high-resolution numerical techniques.

TL;DR: In this article, an extension of the piecewise parabolic method to special relativistic fluid dynamics in multidimensions is presented, which can be used for computations in non-Cartesian geometries.