Full list of author information is available at the end of the article ChaNGa is an N-body cosmology simulation application implemented using Charm++. In this paper, we present the parallel design of ChaNGa and address many challenges arising due to the high dynamic ranges of clustered datasets. We focus on optimizations based on adaptive techniques for scaling to more than 128K cores. We demonstrate strong scaling on up to 512K cores of Blue Waters evolving 12 and 24 billion particles. We also show strong scaling of highly clustered dataset on up to 128K cores
Modeling large-scale sky survey observations is a key driver for the continuing development of high ...
Fundamental physical considerations and past tests suggest that there may be a problem with discrete...
Tormen and Bertschinger have presented an algorithm which allows the dynamic range of N-body simulat...
We report on improvements made over the past two decades to our adaptive treecode N-body method (HOT...
We report on improvements made over the past two decades to our adaptive treecode N-body method (HOT...
Cosmological simulators are currently an important component in the study of the formation of galaxi...
International audienceThe Quijote simulations are a set of 44,100 full N-body simulations spanning m...
The Quijote simulations are a set of 44,100 full N-body simulations spanning more than 7000 cosmolog...
N-Body simulations are a common method of modeling the interacting behavior between objects from the...
The Quijote simulations are a set of 44,100 full N-body simulations spanning more than 7000 cosmolog...
We present benchmarks on high precision direct astrophysical N-body simulations using up to several ...
In this paper, we describe the performance of an $N$-body simulation of star cluster with 64k stars ...
We present our new parallel GPU clusters in Beijing and Heidelberg and demonstrate the nearly optima...
Modern cosmology and plasma physics codes are now capable of simulating trillions of particles on pe...
In cosmological N-body simulations, the representation of dark matter as discrete 'macroparticles' s...
Modeling large-scale sky survey observations is a key driver for the continuing development of high ...
Fundamental physical considerations and past tests suggest that there may be a problem with discrete...
Tormen and Bertschinger have presented an algorithm which allows the dynamic range of N-body simulat...
We report on improvements made over the past two decades to our adaptive treecode N-body method (HOT...
We report on improvements made over the past two decades to our adaptive treecode N-body method (HOT...
Cosmological simulators are currently an important component in the study of the formation of galaxi...
International audienceThe Quijote simulations are a set of 44,100 full N-body simulations spanning m...
The Quijote simulations are a set of 44,100 full N-body simulations spanning more than 7000 cosmolog...
N-Body simulations are a common method of modeling the interacting behavior between objects from the...
The Quijote simulations are a set of 44,100 full N-body simulations spanning more than 7000 cosmolog...
We present benchmarks on high precision direct astrophysical N-body simulations using up to several ...
In this paper, we describe the performance of an $N$-body simulation of star cluster with 64k stars ...
We present our new parallel GPU clusters in Beijing and Heidelberg and demonstrate the nearly optima...
Modern cosmology and plasma physics codes are now capable of simulating trillions of particles on pe...
In cosmological N-body simulations, the representation of dark matter as discrete 'macroparticles' s...
Modeling large-scale sky survey observations is a key driver for the continuing development of high ...
Fundamental physical considerations and past tests suggest that there may be a problem with discrete...
Tormen and Bertschinger have presented an algorithm which allows the dynamic range of N-body simulat...