We present and discuss the characteristics and performance, both in term of computational speed and precision, of a numerical code which integrates the equation of motions of N 'particles' interacting via Newtonian gravitation and move in an external galactic smooth field. The force evaluation on every particle is done by mean of direct summation of the contribution of all the other system's particles, avoiding truncation error. The time integration is done with second-order and sixth-order symplectic schemes. The code, NBSymple, has been parallelized twice, by mean of the Compute Unified Device Architecture (CUDA) to make the all-pair force evaluation as fast as possible on high-performance Graphic Processing Units NVIDIA TESLA C1060, whil...
We describe source code level parallelization for the kira direct gravitational N-body integrator, t...
This report deals with speed up results of our new N-body code for simulating self gravitating codes...
A wide variety of outstanding problems in astrophysics involve the motion of a large number of parti...
NBSymple is a numerical code which numerically integrates the equation of motions of N 'particles' i...
We present a new implementation of the numerical integration of the classical, gravitational, N-body...
We present the results of gravitational direct N-body simulations using the graphics processing unit...
The main target of this work is the discussion of the modern techniques (software and hardware) apt ...
The main performance bottleneck of gravitational N-body codes is the force calculation between two p...
Hybrid computational architectures based on the joint power of Central Processing Units (CPUs) and G...
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...
Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact w...
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable...
The classic N-body problem refers to determining the motion of N particles that interact via a long-...
We describe source code level parallelization for the kira direct gravitational N-body integrator, t...
This report deals with speed up results of our new N-body code for simulating self gravitating codes...
A wide variety of outstanding problems in astrophysics involve the motion of a large number of parti...
NBSymple is a numerical code which numerically integrates the equation of motions of N 'particles' i...
We present a new implementation of the numerical integration of the classical, gravitational, N-body...
We present the results of gravitational direct N-body simulations using the graphics processing unit...
The main target of this work is the discussion of the modern techniques (software and hardware) apt ...
The main performance bottleneck of gravitational N-body codes is the force calculation between two p...
Hybrid computational architectures based on the joint power of Central Processing Units (CPUs) and G...
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...
Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact w...
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable...
The classic N-body problem refers to determining the motion of N particles that interact via a long-...
We describe source code level parallelization for the kira direct gravitational N-body integrator, t...
This report deals with speed up results of our new N-body code for simulating self gravitating codes...
A wide variety of outstanding problems in astrophysics involve the motion of a large number of parti...