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[null,"1.","Record Nr.",null,"UNINA9910146559403321"]
[null,null,"Titolo",null,"The Cambridge n-body lectures / / Sverre Aarseth, Christopher Tout, Rosemary Mardling, editor"]
[null,null,"Pubbl/distr/stampa",null,"Berlin, Heidelberg : , : Springer, , [2008]"]
[{"$nulls":4},"©2008"]
[null,null,"ISBN",null,"1-4020-8431-5"]
[null,null,"Edizione",null,"[1st ed. 2008.]"]
[null,null,"Descrizione fisica",null,"1 online resource (X, 402 p.)"]
[null,null,"Collana",null,"Lecture Notes in Physics"]
[null,null,"Disciplina",null,"530.144"]
[null,null,"Soggetti",null,"Many-body problem"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,null,"Note generali","Bibliographic Level Mode of Issuance: Monograph"]
[null,null,null,"Nota di bibliografia","Includes bibliographical references and index."]
[null,null,"Nota di contenuto",null,"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."]
[null,null,null,"Sommario/riassunto","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."]