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N-body Problem
Details
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online.To understand the motion of celestial bodies, the sun, planets and the visible stars has been the main motivation for the n-body problem. The first complete mathematical formulation of this problem appeared in Newton''s Principia. Since gravity was responsible for the motion of planets and stars, Newton had to express gravitational interactions in terms of differential equations. An important fact, which Newton proved in the Principia, is that celestial bodies can be modelled as point masses.
Klappentext
To understand the motion of celestial bodies, the sun, planets and the visible stars has been the main motivation for the n-body problem. The first complete mathematical formulation of this problem appeared in Newton's Principia. Since gravity was responsible for the motion of planets and stars, Newton had to express gravitational interactions in terms of differential equations. An important fact, which Newton proved in the Principia, is that celestial bodies can be modelled as point masses.
Weitere Informationen
- Allgemeine Informationen
- GTIN 09786130303686
- Editor Lambert M. Surhone, Miriam T. Timpledon, Susan F. Marseken
- Sprache Englisch
- Genre Physik & Astronomie
- Größe H4mm x B220mm x T150mm
- Jahr 2009
- EAN 9786130303686
- Format Fachbuch
- ISBN 978-613-0-30368-6
- Titel N-body Problem
- Untertitel Many-body Problem, Euler's Three-body Problem, Virial Theorem, Few-body Systems, Natural Units, N-body Simulation
- Gewicht 128g
- Herausgeber Betascript Publishers
- Anzahl Seiten 84