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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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Pubblicazione: | Berlin, Heidelberg : , : Springer Berlin Heidelberg : , : Imprint : Springer, , 1986 |
Edizione: | 1st ed. 1986. |
Descrizione fisica: | 1 online resource (VI, 240 p.) |
Disciplina: | 520 |
Soggetto topico: | 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 | |
Persona (resp. second.): | HutPiet |
McMillianStephen L.W | |
Nota di contenuto: | 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. |
Titolo autorizzato: | The Use of Supercomputers in Stellar Dynamics ![]() |
ISBN: | 3-540-47361-0 |
Formato: | Materiale a stampa ![]() |
Livello bibliografico | Monografia |
Lingua di pubblicazione: | Inglese |
Record Nr.: | 9910257391803321 |
Lo trovi qui: | Univ. Federico II |
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