We present a new implementation of the numerical integration of the classical, gravitational, N-body problem based on a high order Hermite's integration scheme with block time steps, with a direct evaluation of the particle-particle forces. The main innovation of this code (called HiGPUs) is its full parallelization, exploiting both OpenMP and MPI in the use of the multicore Central Processing Units as well as either Compute Unified Device Architecture (CUDA) or OpenCL for the hosted Graphic Processing Units. We tested both performance and accuracy of the code using up to 256 GPUs in the supercomputer IBM iDataPlex DX360M3 Linux Infiniband Cluster provided by the Italian supercomputing consortium CINECA, for values of N <= 8 millions. We we...
NBSymple is a numerical code which numerically integrates the equation of motions of N 'particles' i...
The direct-summation of N gravitational forces is a complex problem for which there is no analytical...
The direct-summation of N gravitational forces is a complex problem for which there is no analytical...
HiGPUs is an implementation of the numerical integration of the classical, gravitational, N-body pro...
The main target of this work is the discussion of the modern techniques (software and hardware) apt ...
Hybrid computational architectures based on the joint power of Central Processing Units (CPUs) and G...
A wide variety of outstanding problems in astrophysics involve the motion of a large number of parti...
We present and discuss the characteristics and performance, both in term of computational speed and ...
We present the results of gravitational direct N-body simulations using the graphics processing unit...
Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact w...
Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact w...
We describe source code level parallelization for the {\tt kira} direct gravitational $N$-body integ...
We describe source code level parallelization for the {____tt kira} direct gravitational $N$-body in...
We describe source code level parallelization for the kira direct gravitational N-body integrator, t...
Fig. 1. Rendering (left) and computer representation (tree-code in green) of a collision between two...
NBSymple is a numerical code which numerically integrates the equation of motions of N 'particles' i...
The direct-summation of N gravitational forces is a complex problem for which there is no analytical...
The direct-summation of N gravitational forces is a complex problem for which there is no analytical...
HiGPUs is an implementation of the numerical integration of the classical, gravitational, N-body pro...
The main target of this work is the discussion of the modern techniques (software and hardware) apt ...
Hybrid computational architectures based on the joint power of Central Processing Units (CPUs) and G...
A wide variety of outstanding problems in astrophysics involve the motion of a large number of parti...
We present and discuss the characteristics and performance, both in term of computational speed and ...
We present the results of gravitational direct N-body simulations using the graphics processing unit...
Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact w...
Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact w...
We describe source code level parallelization for the {\tt kira} direct gravitational $N$-body integ...
We describe source code level parallelization for the {____tt kira} direct gravitational $N$-body in...
We describe source code level parallelization for the kira direct gravitational N-body integrator, t...
Fig. 1. Rendering (left) and computer representation (tree-code in green) of a collision between two...
NBSymple is a numerical code which numerically integrates the equation of motions of N 'particles' i...
The direct-summation of N gravitational forces is a complex problem for which there is no analytical...
The direct-summation of N gravitational forces is a complex problem for which there is no analytical...