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|a 9781402084317
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| 100 |
1 |
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|a Aarseth, Sverre
|e [editor]
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| 245 |
0 |
0 |
|a The Cambridge N-Body Lectures
|h Elektronische Ressource
|c edited by Sverre Aarseth, Christopher Tout, Rosemary Mardling
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| 250 |
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|a 1st ed. 2008
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| 260 |
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|a Dordrecht
|b Springer Netherlands
|c 2008, 2008
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| 300 |
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|a X, 402 p
|b online resource
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| 505 |
0 |
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|a Direct N-Body Codes -- Regular Algorithms for the Few-Body Problem -- Resonance, Chaos and Stability: The Three-Body Problem in Astrophysics -- Fokker–planck Treatment of Collisional Stellar Dynamics -- Monte-Carlo Models of Collisional Stellar Systems -- Particle-Mesh Technique and Superbox -- Dynamical Friction -- Initial Conditions for Star Clusters -- Stellar Evolution -- N-Body Stellar Evolution -- Binary Stars -- N - Body Binary Evolution -- The Workings of a Stellar Evolution Code -- Realistic N - Body Simulations of Globular Clusters -- Parallelization, Special Hardware and Post-Newtonian Dynamics in Direct N - Body Simulations -- Educational N - Body Websites
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| 653 |
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|a Atoms
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| 653 |
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|a Atomic, Molecular and Chemical Physics
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| 653 |
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|a Classical Mechanics
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| 653 |
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|a Mathematical physics
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| 653 |
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|a Astrophysics
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| 653 |
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|a Mechanics
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| 653 |
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|a Theoretical, Mathematical and Computational Physics
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| 653 |
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|a Molecules
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| 700 |
1 |
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|a Tout, Christopher
|e [editor]
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| 700 |
1 |
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|a Mardling, Rosemary
|e [editor]
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| 041 |
0 |
7 |
|a eng
|2 ISO 639-2
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| 989 |
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|b Springer
|a Springer eBooks 2005-
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| 490 |
0 |
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|a Lecture Notes in Physics
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| 028 |
5 |
0 |
|a 10.1007/978-1-4020-8431-7
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| 856 |
4 |
0 |
|u https://doi.org/10.1007/978-1-4020-8431-7?nosfx=y
|x Verlag
|3 Volltext
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| 082 |
0 |
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|a 523.01
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| 520 |
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|a Published under the auspices of the Royal Astronomical Society, this volume contains a set of extensive school tested lectures, with the aim to give a coherent and thorough background knowledge of the subject and to introduce the latest developments in N-body computational astrophysics. The topics cover a wide range from the classical few-body problem with discussions of resonance, chaos and stability to realistic modelling of star clusters as well as descriptions of codes, algorithms and special hardware for N-body simulations. This collection of topics, related to the gravitational N-body problem, will prove useful to both students and researchers in years to come
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