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Physics of Gravitating Systems I: Equilibrium and Stability (Softcover Reprint of the Original 1st 1984)

Physics of Gravitating Systems I

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"Physics of Gravitating Systems I" by A.M. Fridman, V.L. Polyachenko is a astronomy book and space science reference focused on General Astronomy. Best for students, researchers, and serious astronomy enthusiasts.

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 and lunar 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.

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Best For: Students and researchers in astronomy and astrophysics focusing on gravitational dynamics.
Focus: The equilibrium and stability of gravitating systems, emphasizing collective effects in their dynamics.
Covers: Fundamental concepts in the physics of gravitating systems, including plasma physics analogies and gravitational interactions.
Why It Matters: Provides a detailed examination of how collective effects influence the behavior of systems governed by gravity, a perspective only recently acknowledged in astronomy.

"Physics of Gravitating Systems I" by A.M. Fridman, V.L. Polyachenko is a astronomy book and space science reference focused on General Astronomy. Best for students, researchers, and serious astronomy enthusiasts.

Topic: General Astronomy

Author: A.M. Fridman, V.L. Polyachenko

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

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 and lunar 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.

AuthorA.M. Fridman, V.L. Polyachenko
PublisherSpringer
Published2012-08-03
ISBN-139783642878329
BindingPaperback
LanguageEnglish
SubjectsScience
TopicGeneral Astronomy

Format: Paperback

Language: English

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