04294nam 22006135 450 99646683430331620200629143522.03-540-47361-010.1007/BFb0116387(CKB)1000000000778475(DE-He213)978-3-540-47361-9(PPN)155194402(EXLCZ)99100000000077847520121227d1986 u| 0engurnn|008mamaatxtrdacontentcrdamediacrrdacarrierThe 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. McMillian1st ed. 1986.Berlin, Heidelberg :Springer Berlin Heidelberg :Imprint: Springer,1986.1 online resource (VI, 240 p.) Lecture Notes in Physics,0075-8450 ;2673-540-17196-7 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.Lecture Notes in Physics,0075-8450 ;267Observations, AstronomicalAstronomy—ObservationsAstrophysicsPhysicsComputational complexityAstronomy, Observations and Techniqueshttps://scigraph.springernature.com/ontologies/product-market-codes/P22014Astrophysics and Astroparticleshttps://scigraph.springernature.com/ontologies/product-market-codes/P22022Mathematical Methods in Physicshttps://scigraph.springernature.com/ontologies/product-market-codes/P19013Numerical and Computational Physics, Simulationhttps://scigraph.springernature.com/ontologies/product-market-codes/P19021Complexityhttps://scigraph.springernature.com/ontologies/product-market-codes/T11022Observations, Astronomical.Astronomy—Observations.Astrophysics.Physics.Computational complexity.Astronomy, Observations and Techniques.Astrophysics and Astroparticles.Mathematical Methods in Physics.Numerical and Computational Physics, Simulation.Complexity.520Hut Pietedthttp://id.loc.gov/vocabulary/relators/edtMcMillian Stephen L.Wedthttp://id.loc.gov/vocabulary/relators/edtBOOK996466834303316The Use of Supercomputers in Stellar Dynamics2505020UNISA