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We present our implementation of the soft-sphere discrete element method (SSDEM) in the parallel gravitational N-body code pkdgrav, a well-tested simulation package that has been used to provide many ...
The spectral code for non-equilibrium plasma has been developed based on the updated atomic database. The first application is for winds from super stellar clusters for which a self-consistent physica...
By analysing models of the young massive cluster R136 in 30 Doradus, set-up using the herewith introduced and publicly made available code McLuster, we investigate and compare different methods for de...
We perform high resolution N-body simulations for f(R) gravity based on a self-adaptive particle-mesh code MLAPM. The Chameleon mechanism that recovers General Relativity on small scales is fully take...
We discuss results from simulations of black hole formation in failing core-collapse supernovae performed with the code GR1D, a new open-source Eulerian spherically-symmetric general-relativistic hy...
We present a new numerical code, X-ECHO, for general relativistic magnetohydrodynamics (GRMHD) in dynamical spacetimes. This is aimed at studying astrophysical situations where strong gravity and magn...
We present a new general relativistic (GR) code for hydrodynamic supernova simulations with neutrino transport in spherical and azimuthal symmetry (1D/2D). The code is a combination of the CoCoNuT hyd...
A massively parallel code for polarization calculations     parallel code  polarization calculations       font style='font-size:12px;'> 2009/6/8
A massively parallel code for polarization calculations。
Introducing zeus-mp: a 3d, parallel, multiphysics code for astrophysical fluid dynamics。
Introducing zeus-mp: a 3d, parallel, multiphysics code for astrophysical fluid dynamics。
A NEW ,3D ADAPRIVE GRID CODE FOR ASTROPHYSICAL ANG DEOPHSICAL GASDYNAMICS     shock waves  hydrodynamics       font style='font-size:12px;'> 2009/6/4
A NEW ,3D ADAPRIVE GRID CODE FOR ASTROPHYSICAL ANG DEOPHSICAL GASDYNAMICS。
We describe the TreePM method for carrying out large N-Body simulations to study formation and evolution of the large scale structure in the Universe. This method is a combination of Barnes and Hut ...
We describe the two-dimensional TreePM method in this paper. The 2d TreePM code is an accurate and efficient technique to carry out large two-dimensional N-body simulations in cosmology. This hybri...
In this paper an analysis of the physical properties of the Broad Line Region (BLR) of the active galaxy NGC 5548 is presented. Using the photoion- ization code CLOUDY and the measurements of Peters...

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