GRAPE-5: A Special-Purpose Computer for N-body Simulation
arXiv:astro-ph/9909116 · doi:10.1093/pasj/52.4.659
Abstract
We have developed a special-purpose computer for gravitational many-body simulations, GRAPE-5. GRAPE-5 is the successor of GRAPE-3. Both consist of eight custom pipeline chips (G5 chip and GRAPE chip). The difference between GRAPE-5 and GRAPE-3 are: (1) The G5 chip contains two pipelines operating at 80 MHz, while the GRAPE chip had one at 20 MHz. Thus, the calculation speed of the G5 chip and that of GRAPE-5 board are 8 times faster than that of GRAPE chip and GRAPE-3 board. (2) The GRAPE-5 board adopted PCI bus as the interface to the host computer instead of VME of GRAPE-3, resulting in the communication speed one order of magnitude faster. (3) In addition to the pure 1/r potential, the G5 chip can calculate forces with arbitrary cutoff functions, so that it can be applied to Ewald or P^3M methods. (4) The pairwise force calculated on GRAPE-5 is about 10 times more accurate than that on GRAPE-3. On one GRAPE-5 board, one timestep of 128k-body simulation with direct summation algorithm takes 14 seconds. With Barnes-Hut tree algorithm (theta = 0.75), one timestep of 10^6-body simulation can be done in 16 seconds.
19 pages, 24 Postscript figures, 3 tables, Latex, submitted to Publications of the Astronomical Society of Japan
Cited by in corpus (46)
- GADGET: A code for collisionless and gasdynamical cosmological simulations
- What determines the strength and the slowdown rate of bars ?
- Morphology, photometry and kinematics of N-body bars. I Three models with different halo central concentrations
- Statistical Properties of Collisionless Equal- and Unequal-Mass Merger Remnants of Disk Galaxies
- Properties of Early-Type, Dry Galaxy Mergers and the Origin of Massive Elliptical Galaxies
- A Hierarchical O(N) Force Calculation Algorithm
- Structure of Dark Matter Halos From Hierarchical Clustering
- Bar-driven dark halo evolution: a resolution of the cusp--core controversy
- The dynamical evolution of fractal star clusters: the survival of substructure
- GRAPE-6: The massively-parallel special-purpose computer for astrophysical particle simulation
- Surface density profiles of collisionless disc merger remnants
- GreeM : Massively Parallel TreePM Code for Large Cosmological N-body Simulations
- GRAPE-6A: A single-card GRAPE-6 for parallel PC-GRAPE cluster system
- Structure of Dark Matter Halos From Hierarchical Clustering. III. Shallowing of The Inner Cusp
- Simulation techniques for cosmological simulations
- Orbital Structure of Collisionless Merger Remnants: On the Origin of Photometric and Kinematic Properties of Elliptical and S0 Galaxies
- Thermodynamics of the self-gravitating ring model
- VINE -- A numerical code for simulating astrophysical systems using particles I: Description of the physics and the numerical methods
- The Formation of Disks in Elliptical Galaxies
- Phantom-GRAPE: numerical software library to accelerate collisionless -body simulation with SIMD instruction set on x86 architecture
- The Validity of the Adiabatic Contraction Approximation for Dark Matter Halos
- Tidal disruption of dark matter halos around proto-globular clusters
- FAST: A Fully Asynchronous Split Time-Integrator for Self-Gravitating Fluid
- A bar in the inner halo of barred galaxies I. Structure and kinematics of a representative model
- PPPM and TreePM Methods on GRAPE Systems for Cosmological N-body Simulations
- VINE -- A numerical code for simulating astrophysical systems using particles II: Implementation and performance characteristics
- On the equilibrium morphology of systems drawn from spherical collapse experiments
- GOTHIC: Gravitational oct-tree code accelerated by hierarchical time step controlling
- Pseudoparticle Multipole Method: A Simple Method to Implement High-Accuracy Treecode
- Universal Non-Gaussian Velocity Distribution in Violent Gravitational Processes
- Coevolution of the galactic cores and spiral galaxies
- Mass Loss Timescale of Star Clusters in External Tidal Field
- Vectorization and Parallelization of the Adaptive Mesh Refinement N-body Code
- Dynamical evolution driven by bars and interactions : Input from numerical simulations
- Mass-Loss Timescale of Star Clusters in an External Tidal Field. II. Effect of Mass Profile of Parent Galaxy
- A Natural Symmetrization for the Plummer Potential
- Relaxation times calculated from angular deflections
- Local virial relation for self-gravitating system
- Mean-pairwise peculiar velocity in cosmological N-body simulations: time-variation, scale-dependence and stable condition
- PGPG: An Automatic Generator of Pipeline Design for Programmable GRAPE Systems
- Gravitational Fugacity as the seed of self-organized violent relaxaton process toward Local Virial relation
- Hierarchical Tree Algorithm for Collisional N-body Simulations on GRAPE
- Acceleration of the tree method with SIMD instruction set
- Acceleration Method of Neighbor Search with GRAPE and Morton-ordering
- A 400 Trillion-Grid Vlasov Simulation on Fugaku Supercomputer: Large-Scale Distribution of Cosmic Relic Neutrinos in a Six-dimensional Phase Space
- Investigating the long-term evolution of galaxies: Noise,cuspy halos and bars