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001			978-3-540-47361-9
003			DE-He213
005			20190213151621.0
007			cr nn 008mamaa
008			121227s1986 gw | s |||| 0|eng d
020			_a9783540473619 _9978-3-540-47361-9
024	7		_a10.1007/BFb0116387 _2doi
050		4	_aQB4
072		7	_aPG _2bicssc
072		7	_aSCI004000 _2bisacsh
072		7	_aPG _2thema
082	0	4	_a520 _223
245	1	4	_aThe Use of Supercomputers in Stellar Dynamics _h[electronic resource] : _bProceedings of a Workshop Held at the Institute for Advanced Study Princeton, USA, June 2–4, 1986 / _cedited by Piet Hut, Stephen L. W. McMillan.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1986.
300			_aVI, 240 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aLecture Notes in Physics, _x0075-8450 ; _v267
505	0		_aDynamical 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.
650		0	_aMathematical physics.
650		0	_aEngineering.
650	1	4	_aAstronomy, Observations and Techniques. _0http://scigraph.springernature.com/things/product-market-codes/P22014
650	2	4	_aAstrophysics and Astroparticles. _0http://scigraph.springernature.com/things/product-market-codes/P22022
650	2	4	_aMathematical Methods in Physics. _0http://scigraph.springernature.com/things/product-market-codes/P19013
650	2	4	_aNumerical and Computational Physics, Simulation. _0http://scigraph.springernature.com/things/product-market-codes/P19021
650	2	4	_aComplexity. _0http://scigraph.springernature.com/things/product-market-codes/T11022
700	1		_aHut, Piet. _eeditor. _4edt _4http://id.loc.gov/vocabulary/relators/edt
700	1		_aMcMillan, Stephen L. W. _eeditor. _4edt _4http://id.loc.gov/vocabulary/relators/edt
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9783662135815
776	0	8	_iPrinted edition: _z9783540171966
776	0	8	_iPrinted edition: _z9783662135808
830		0	_aLecture Notes in Physics, _x0075-8450 ; _v267
856	4	0	_uhttps://doi.org/10.1007/BFb0116387
912			_aZDB-2-PHA
912			_aZDB-2-LNP
912			_aZDB-2-BAE
999			_c11291 _d11291