Physics gravitating systems (13 Ergebnisse)

Hardcover. Zustand: Très bon. Ancien livre de bibliothèque avec équipements. Couverture différente. Edition 1984. Ammareal reverse jusqu'à 15% du prix net de cet article à des organisations caritatives. ENGLISH DESCRIPTION Book Condition: Used, Very good. Former library book. Different cover. Edition 1984. Ammareal gives back up to 15% of this item's net price to charity organizations. …

Hardcover. Zustand: Bon. Ancien livre de bibliothèque avec équipements. Couverture différente. Edition 1984. Tome 2. Ammareal reverse jusqu'à 15% du prix net de cet article à des organisations caritatives. ENGLISH DESCRIPTION Book Condition: Used, Good. Former library book. Different cover. Edition 1984. Volume 2. Ammareal gives back up to 15% of this item's net price to charity organizations.…

Zustand: New. In English.

Zustand: New. In English.

PAPERBACK. Zustand: Fine. 3642878350 Like New; Softcover; Close to new condition; Covers are still glossy with straight" edge-corners; Unblemished textblock edges; The endpapers and all text pages are bright and unmarked; Binding is tight with a straight spine; This book will be stored and delivered in a sturdy cardboard box with foam padding; Medium Format (8.5" - 9.75" tall); Dark brown covers with title in orange letteringp; 1984, Springer-Verlag Publishing; 358 pages; "Physics of Gravitating Systems II: Nonlinear Collective Processes: Nonlinear Waves, Solitons, Collisionless Shocks, Turbulence. Astrophysical Applications," by A.M. Fridman & V.L. Polyachenko.…

Paperback. Zustand: Brand New. reprint edition. 376 pages. 9.25x6.10x0.94 inches. In Stock.

Paperback. Zustand: Brand New. reprint edition. 488 pages. 9.25x6.10x1.18 inches. In Stock.

Zustand: New.

Zustand: New.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - (Volume II).- Non-Jeans Instabilities of Gravitating Systems.- VI Non-Jeans Instabilities of Gravitating Systems.- VII Problems of Nonlinear Theory.- II Astrophysical Applications.- VIII General Remarks.- IX Spherical Systems.- X Ellipsoidal Systems.- XI Disk-like Systems. Spiral Structure.- XII Other Applications.- 1. Collisionless Kinetic Equation and Poisson Equation in Different Coordinate Systems.- 2. Separation of Angular Variables in the Problem of Small Perturbations of Spherically Symmetrical Collisionless Systems.- 3. Statistical Simulation of Stellar Systems.- 3.1. Simulation of Stellar Spheres of the First Camm Series.- 3.2. Simulation of Homogeneous Nonrotating Ellipsoids.- 4. The Matrix Formulation of the Problem of Eigenoscillations of a Spherically-Symmetrical Collisionless System.- 5. The Matrix Formulation of the Problem of Eigenoscillations of Collisionless Disk Systems.- 5.1. The Main Ideas of the Derivation of the Matrix Equation.- 5.2. 'Lagrange' Derivation of the Matrix Equation.- 6. Derivation of the Dispersion Equation for Perturbations of the Three-Axial Freeman Ellipsoid.- 7. WKB Solutions of the Poisson Equation Taking into Account the Preexponential Terms and Solution of the Kinetic Equation in the Postepicyclic Approximation.- 7.1. The Relation Between the Potential and the Surface Density.- 7.2. Calculations of the Response of a Stellar Disk to an Imposed Perturbation of the Potential.- 8. On the Derivation of the Nonlinear Dispersion Equation for Collisionless Disk.- 9. Calculation of the Matrix Elements for the Three-Waves Interaction.- 10. Derivation of the Formulas for the Boundaries of Wave Numbers Range Which May Take Part in a Decay.- 11. Derivation of the Kinetic Equation for Waves.- 12. Table of Non-Jeans Instabilities (with a Short Summary).- References.- Additional References.…

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - It would seem that any specialist in plasma physics studying a medium in which the interaction between particles is as distance-dependent as the inter action between stars and other gravitating masses would assert that the role of collective effects in the dynamics of gravitating systems must be decisive. However, among astronomers this point of view has been recog nized only very recently. So, comparatively recently, serious consideration has been devoted to theories of galactic spiral structure in which the dominant role is played by the orbital properties of individual stars rather than collec tive effects. In this connection we would like to draw the reader's attention to a difference in the scientific traditions of plasma physicists and astrono mers, whereby the former have explained the delay of the onset of controlled thermonuclear fusion by the 'intrigues' of collective processes in the plasma, while many a generation of astronomers were calculating star motions, solar andlunar eclipses, and a number of other fine effects for many years ahead by making excellent use of only the laws of Newtonian mechanics. Therefore, for an astronomer, it is perhaps not easy to agree with the fact that the evolution of stellar systems is controlled mainly by collective effects, and the habitual methods of theoretical mechanics III astronomy must make way for the method of self-consistent fields.…

Hardcover. Zustand: gut. 1984. Physics of Gravitating Systems: Equilibrium and Stability of Gravitating Systems In englischer Sprache. pages.

Hardcover. Zustand: gut. 1984. Physics of Gravitating Systems II. Nonlinear Collective Processes: Nonlinear Waves, Solitons, Collisionless Shocks, Turbulence. Astrophysica In englischer Sprache. pages.