Astrophysics Source Code Library

Making codes discoverable since 1999

Searching for codes credited to 'Maindl, Thomas'

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[ascl:1911.023] miluphcuda: Smooth particle hydrodynamics code

miluphcuda is the CUDA port of the original miluph code; it runs on single Nvidia GPUs with compute capability 5.0 and higher and provides fast and efficient computation. The code can be used for hydrodynamical simulations and collision and impact physics, and features self-gravity via Barnes-Hut trees and porosity models such as P-alpha and epsilon-alpha. It can model solid bodies, including ductile and brittle materials, as well as non-viscous fluids, granular media, and porous continua.

[submitted] DYnamics, Age and Metallicity Indicators Tracing Evolution (DYNAMITE)

DYNAMITE (DYnamics, Age and Metallicity Indicators Tracing Evolution) is a triaxial dynamical modelling code for stellar systems, which is developed at the University of Vienna. It is based on existing codes for Schwarzschild modelling in triaxial systems. The power and innovation of DYNAMITE lies in the easy-to-use object oriented Python wrapper. This makes it simple to extend the scope of pre-existing triaxial Schwarzschild codes with a number of new features, including (i) discrete kinematics, (ii) more flexible descriptions of line-of-sight velocity distributions, (iii) modelling of stellar population information, (iv) more efficient steps through parameter space, and (v) using GPU acceleration.