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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
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
Edizione [1st ed. 1986.]
Pubbl/distr/stampa Berlin, Heidelberg : , : Springer Berlin Heidelberg : , : Imprint : Springer, , 1986
Descrizione fisica 1 online resource (VI, 240 p.)
Disciplina 520
Collana Lecture Notes in Physics
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
ISBN 3-540-47361-0
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
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.
Record Nr. UNINA-9910257391803321
Berlin, Heidelberg : , : Springer Berlin Heidelberg : , : Imprint : Springer, , 1986
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui
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
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
Edizione [1st ed. 1986.]
Pubbl/distr/stampa Berlin, Heidelberg : , : Springer Berlin Heidelberg : , : Imprint : Springer, , 1986
Descrizione fisica 1 online resource (VI, 240 p.)
Disciplina 520
Collana Lecture Notes in Physics
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
ISBN 3-540-47361-0
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
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.
Record Nr. UNISA-996466834303316
Berlin, Heidelberg : , : Springer Berlin Heidelberg : , : Imprint : Springer, , 1986
Materiale a stampa
Lo trovi qui: Univ. di Salerno
Opac: Controlla la disponibilità qui