We present SUPERBOX, a particle-mesh code with high resolution sub-grids and an NGP (nearest grid point) force-calculation scheme based on the second derivatives of the potential. SUPERBOX implements a fast low-storage FFT-algorithm, giving the possibility to work with millions of particles on desk-top computers. Test calculations show energy and angular momentum conservation to one part in 10(5) per crossing-time. The effects of grid and numerical relaxation remain negligible, even when these calculations cover a Hubble-time of evolution. As the sub-grids follow the trajectories of individual galaxies, the code allows a highly resolved treatment of interactions in clusters of galaxies, such as high-velocity encounters between elliptical ga...
We describe a novel N-body code designed for simulations of the central regions of galaxies containi...
Modelling the formation of super-km-sized planetesimals by gravitational collapse of regions overden...
Modelling the formation of super-km-sized planetesimals by gravitational collapse of regions overden...
This paper presents a fast, economical particle-multiple-mesh N-body code optimized for large-N mode...
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable...
Fig. 1. Rendering (left) and computer representation (tree-code in green) of a collision between two...
This paper presents a fast, economical particle-multiple-mesh N-body code optimized for large-N mode...
We describe a nested-grid particle-mesh (NGPM) code designed to study gravitational instability in t...
Context.N-body simulations are widely used for galactic dynamics studies. Several different algorith...
International audienceContext.N-body simulations are widely used for galactic dynamics studies. Seve...
REBOUND is a new multi-purpose N-body code which is freely available under an open-source license. I...
We present and discuss the characteristics and performance, both in term of computational speed and ...
An improved implementation of an N-body code for simulating collisionless cosmological dynamics is p...
We provide a novel and efficient algorithm for computing accelerations in theperiodic large-N-body p...
. I compare various popular and unpopular techniques for simulating large collisionless stellar syst...
We describe a novel N-body code designed for simulations of the central regions of galaxies containi...
Modelling the formation of super-km-sized planetesimals by gravitational collapse of regions overden...
Modelling the formation of super-km-sized planetesimals by gravitational collapse of regions overden...
This paper presents a fast, economical particle-multiple-mesh N-body code optimized for large-N mode...
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable...
Fig. 1. Rendering (left) and computer representation (tree-code in green) of a collision between two...
This paper presents a fast, economical particle-multiple-mesh N-body code optimized for large-N mode...
We describe a nested-grid particle-mesh (NGPM) code designed to study gravitational instability in t...
Context.N-body simulations are widely used for galactic dynamics studies. Several different algorith...
International audienceContext.N-body simulations are widely used for galactic dynamics studies. Seve...
REBOUND is a new multi-purpose N-body code which is freely available under an open-source license. I...
We present and discuss the characteristics and performance, both in term of computational speed and ...
An improved implementation of an N-body code for simulating collisionless cosmological dynamics is p...
We provide a novel and efficient algorithm for computing accelerations in theperiodic large-N-body p...
. I compare various popular and unpopular techniques for simulating large collisionless stellar syst...
We describe a novel N-body code designed for simulations of the central regions of galaxies containi...
Modelling the formation of super-km-sized planetesimals by gravitational collapse of regions overden...
Modelling the formation of super-km-sized planetesimals by gravitational collapse of regions overden...