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Record Nr. |
UNISA996466834303316 |
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Titolo |
The Use of Supercomputers in Stellar Dynamics [[electronic resource] ] : Proceedings of a Workshop Held at the Institute for Advanced Study, Princeton, USA, June 2-4, 1986 / / edited by Piet Hut, Stephen L.W. McMillian |
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Pubbl/distr/stampa |
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Berlin, Heidelberg : , : Springer Berlin Heidelberg : , : Imprint : Springer, , 1986 |
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ISBN |
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Edizione |
[1st ed. 1986.] |
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Descrizione fisica |
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1 online resource (VI, 240 p.) |
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Collana |
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Lecture Notes in Physics, , 0075-8450 ; ; 267 |
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Disciplina |
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Soggetti |
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Observations, Astronomical |
Astronomy—Observations |
Astrophysics |
Physics |
Computational complexity |
Astronomy, Observations and Techniques |
Astrophysics and Astroparticles |
Mathematical Methods in Physics |
Numerical and Computational Physics, Simulation |
Complexity |
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Lingua di pubblicazione |
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Formato |
Materiale a stampa |
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Livello bibliografico |
Monografia |
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Nota di contenuto |
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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 |
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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. |
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