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Gravitational N-body simulations /

Aarseth, Sverre J. (1934-)

Gravitational N-body simulations /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	521
書名/作者:	Gravitational N-body simulations // Sverre J. Aarseth.
作者:	Aarseth, Sverre J.
面頁冊數:	1 online resource (xv, 413 pages) : : digital, PDF file(s).
附註:	Title from publisher's bibliographic system (viewed on 05 Oct 2015).
標題:	Many-body problem.
ISBN:	9780511535246 (ebook)
摘要、提要註:	This book discusses in detail all the relevant numerical methods for the classical N-body problem. It demonstrates how to develop clear and elegant algorithms for models of gravitational systems, and explains the fundamental mathematical tools needed to describe the dynamics of a large number of mutually attractive particles. Particular attention is given to the techniques needed to model astrophysical phenomena such as close encounters and the dynamics of black hole binaries. The author reviews relevant work in the field and covers applications to the problems of planetary formation and star cluster dynamics, both of Pleiades type and globular clusters. Self-contained and pedagogical, this book is suitable for graduate students and researchers in theoretical physics, astronomy and cosmology.
電子資源:	http://dx.doi.org/10.1017/CBO9780511535246

Gravitational N-body simulations /
Aarseth, Sverre J.1934-

Gravitational N-body simulations /Sverre J. Aarseth. - 1 online resource (xv, 413 pages) :digital, PDF file(s). - Cambridge monographs on mathematical physics. - Cambridge monographs on mathematical physics..

Title from publisher's bibliographic system (viewed on 05 Oct 2015).

The N-body problem --1.

This book discusses in detail all the relevant numerical methods for the classical N-body problem. It demonstrates how to develop clear and elegant algorithms for models of gravitational systems, and explains the fundamental mathematical tools needed to describe the dynamics of a large number of mutually attractive particles. Particular attention is given to the techniques needed to model astrophysical phenomena such as close encounters and the dynamics of black hole binaries. The author reviews relevant work in the field and covers applications to the problems of planetary formation and star cluster dynamics, both of Pleiades type and globular clusters. Self-contained and pedagogical, this book is suitable for graduate students and researchers in theoretical physics, astronomy and cosmology.

ISBN: 9780511535246 (ebook)Subjects--Topical Terms:

394358
Many-body problem.

LC Class. No.: QB362.M3 / A27 2003

Dewey Class. No.: 521

Gravitational N-body simulations /
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505 0 0 $g 1. $t The N-body problem -- $g 2. $t Predictor-corrector methods -- $g 3. $t Neighbour treatments -- $g 4. $t Two-body regularization -- $g 5. $t Multiple regularization -- $g 6. $t Tree codes -- $g 7. $t Program organization -- $g 8. $t Initial setup -- $g 9. $t Decision-making -- $g 10. $t Neighbour schemes -- $g 11. $t Two-body algorithms -- $g 12. $t Chain procedures -- $g 13. $t Accuracy and performance -- $g 14. $t Practical aspects -- $g 15. $t Star clusters -- $g 16. $t Galaxies -- $g 17. $t Planetary systems -- $g 18. $t Small-N experiments -- $g App. A. $t Global regularization algorithms -- $g App. B. $t Chain algorithms -- $g App. C. $t Higher-order systems -- $g App. D. $t Practical algorithms -- $g App. E. $t KS procedures with GRAPE -- $g App. F. $t Alternative simulation method -- $g App. G. $t Table of symbols -- $g App. H. $t Hermite integration method.
520 $a This book discusses in detail all the relevant numerical methods for the classical N-body problem. It demonstrates how to develop clear and elegant algorithms for models of gravitational systems, and explains the fundamental mathematical tools needed to describe the dynamics of a large number of mutually attractive particles. Particular attention is given to the techniques needed to model astrophysical phenomena such as close encounters and the dynamics of black hole binaries. The author reviews relevant work in the field and covers applications to the problems of planetary formation and star cluster dynamics, both of Pleiades type and globular clusters. Self-contained and pedagogical, this book is suitable for graduate students and researchers in theoretical physics, astronomy and cosmology.
650 0 $a Many-body problem. $3 394358
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856 4 0 $u http://dx.doi.org/10.1017/CBO9780511535246

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