The Use of Supercomputers in Stellar Dynamics [E-Book] : Proceedings of a Workshop Held at the Institute for Advanced Study Princeton, USA, June 2–4, 1986 / edited by Piet Hut, Stephen L. W. McMillan.
Saved in:
Full text |
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Personal Name(s): | Hut, Piet, editor |
McMillan, Stephen L. W., editor | |
Imprint: |
Berlin, Heidelberg :
Springer,
1986
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Physical Description: |
VI, 240 p. online resource. |
Note: |
englisch |
ISBN: |
9783540473619 |
DOI: |
10.1007/BFb0116387 |
Series Title: |
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Lecture Notes in Physics ;
267 |
Subject (LOC): |
- Dynamical evolution of globular clusters
- Disc galaxy dynamics on the computer
- Star cluster dynamics: Mathematical models
- Models of hot stellar systems
- Supercomputers and large cosmological N-body simulations
- Modelling stellar dynamical systems on the CRAY-1S and the CDC Cyber 205
- Programming the ETA10 for large problems in stellar dynamics
- The architecture of a homogeneous vector supercomputer
- The BBN multiprocessors: Butterfly and Monarch
- The Connection Machine
- A digital Orrery
- The outer solar system for 200 million years
- Smooth particle hydrodynamics: Theory and application to the origin of the moon
- Multiple mesh techniques for modelling interacting galaxies
- Numerical experiments on galactic halo formation
- Numerical integration using explicit taylor series
- Multiple-mesh-particle scheme for N-body simulation
- Direct N-body simulation on supercomputers
- The vectorization of small-n integrators
- N-body integrations using supercomputers
- A new numerical technique for calculation of phase space evolution of stellar systems
- An efficient N-body algorithm for a fine-grain parallel computer
- A gridless fourier method
- Techniques and tricks for N-body computation
- On toolboxes and telescopes
- A unified N-body method
- Vectorization of N-body codes
- Large scale calculations of core oscillations in globular clusters
- Round-off sensitivity in the N-body problem
- Formation of a bar through cold collapse of a stellar system
- The gravitational interaction between N-body (star clusters) and hydrodynamic (ISM) codes in disk galaxy simulations
- Standardised units and time scales.