Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact way and have a computational complexity of O(N^2). Performance can be greatly enhanced via the use of special-purpose accelerator boards like the GRAPE-6A. However the memory of the GRAPE boards is limited. Here, we present a performance analysis of direct N-body codes on two parallel supercomputers that incorporate special-purpose boards, allowing as many as four million particles to be integrated. Both computers employ high-speed, Infiniband interconnects to minimize communication overhead, which can otherwise become significant due to the small number of "active" particles at each time step. We find that the computation time scales well wit...
The gravitational N-body algorithm of Barnes and Hut [1] has been successfully implemented on a hype...
We describe source code level parallelization for the kira direct gravitational N-body integrator, t...
We describe a new parallel N-body code for astrophysical simulations of systems of point masses inte...
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...
Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact w...
We present a performance analysis of different parallelization schemes for direct codes used in the ...
We discuss the performance of direct summation codes used in the simulation of astrophysical stellar...
We discuss the performance of direct summation codes used in the simulation of astrophysical stellar...
The main performance bottleneck of gravitational N-body codes is the force calculation between two p...
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 present a new implementation of the numerical integration of the classical, gravitational, N-body...
Performance analysis of direct N-body algorithms on special-purpose supercomputer
The gravitational N-body algorithm of Barnes and Hut [1] has been successfully implemented on a hype...
The gravitational N-body algorithm of Barnes and Hut [1] has been successfully implemented on a hype...
We describe source code level parallelization for the kira direct gravitational N-body integrator, t...
We describe a new parallel N-body code for astrophysical simulations of systems of point masses inte...
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...
Direct-summation N-body algorithms compute the gravitational interaction between stars in an exact w...
We present a performance analysis of different parallelization schemes for direct codes used in the ...
We discuss the performance of direct summation codes used in the simulation of astrophysical stellar...
We discuss the performance of direct summation codes used in the simulation of astrophysical stellar...
The main performance bottleneck of gravitational N-body codes is the force calculation between two p...
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 present a new implementation of the numerical integration of the classical, gravitational, N-body...
Performance analysis of direct N-body algorithms on special-purpose supercomputer
The gravitational N-body algorithm of Barnes and Hut [1] has been successfully implemented on a hype...
The gravitational N-body algorithm of Barnes and Hut [1] has been successfully implemented on a hype...
We describe source code level parallelization for the kira direct gravitational N-body integrator, t...
We describe a new parallel N-body code for astrophysical simulations of systems of point masses inte...