We demonstrate the acceleration obtained from using GPU/CPU hybrid clusters and supercomputers for N-body simulations of gravity based in part on the author's new code development. Validation tests are shown for cosmological simulations and for galaxy simulations, along with their respective speedups compared to traditional simulations. Potential new applications for science enabled by this advance are highlighted.Department of Physics and AstronomyCollege of Arts and Scienc
Most recent progress in understanding the dynamical evolution of star clusters relies on direct N-bo...
AbstractWe have implemented a fast collisionless N-body code which runs on GPU, the peak performance...
In this short review we present the developments over the last 5 decades that have led to the use of...
N-Body simulations are a common method of modeling the interacting behavior between objects from the...
N-Body simulations are a common method of modeling the interacting behavior between objects from the...
We present the results of gravitational direct $N$-body simulations using the commercial graphics pr...
Fig. 1. Rendering (left) and computer representation (tree-code in green) of a collision between two...
We present benchmarks on high precision direct astrophysical N-body simulations using up to several ...
The main target of this work is the discussion of the modern techniques (software and hardware) apt ...
We report on resent N-body simulations of galaxy formation performed on the GRAPE-4 (GRAvity PipE) s...
We present an algorithm named "Chamomile Scheme". The scheme is fully optimized for calculating grav...
Most recent progress in understanding the dynamical evolution of star clusters relies on direct N-bo...
Graphics Processing Units (GPUs) are quickly becoming viable alternatives for certain simulations cu...
A wide variety of outstanding problems in astrophysics involve the motion of a large number of parti...
Owing to mankind's constant pursuit of knowledge, we have been seeking to understand the vast univer...
Most recent progress in understanding the dynamical evolution of star clusters relies on direct N-bo...
AbstractWe have implemented a fast collisionless N-body code which runs on GPU, the peak performance...
In this short review we present the developments over the last 5 decades that have led to the use of...
N-Body simulations are a common method of modeling the interacting behavior between objects from the...
N-Body simulations are a common method of modeling the interacting behavior between objects from the...
We present the results of gravitational direct $N$-body simulations using the commercial graphics pr...
Fig. 1. Rendering (left) and computer representation (tree-code in green) of a collision between two...
We present benchmarks on high precision direct astrophysical N-body simulations using up to several ...
The main target of this work is the discussion of the modern techniques (software and hardware) apt ...
We report on resent N-body simulations of galaxy formation performed on the GRAPE-4 (GRAvity PipE) s...
We present an algorithm named "Chamomile Scheme". The scheme is fully optimized for calculating grav...
Most recent progress in understanding the dynamical evolution of star clusters relies on direct N-bo...
Graphics Processing Units (GPUs) are quickly becoming viable alternatives for certain simulations cu...
A wide variety of outstanding problems in astrophysics involve the motion of a large number of parti...
Owing to mankind's constant pursuit of knowledge, we have been seeking to understand the vast univer...
Most recent progress in understanding the dynamical evolution of star clusters relies on direct N-bo...
AbstractWe have implemented a fast collisionless N-body code which runs on GPU, the peak performance...
In this short review we present the developments over the last 5 decades that have led to the use of...