Book contents
- Frontmatter
- Contents
- Preface
- Introduction
- Part I Idealized homogeneous systems – basic ideas and gentle relaxation
- 1 The average and fluctuating gravitational fields
- 2 Gentle relaxation: timescales
- 3 The dynamics of random impulsive forces
- 4 General properties of Fokker–Planck evolution
- 5 Fokker–Planck description of gravitating systems
- 6 Dynamics with a memory: non-Markovian evolution
- 7 The Boltzmann equation
- 8 Some properties of the Boltzmann equation
- 9 The virial theorem
- 10 The grand description – Liouville's equation and entropy
- 11 Extracting knowledge: the BBGKY hierarchy
- 12 Extracting knowledge: the Fourier development
- 13 Collective effects – grexons
- 14 Collective scattering
- 15 Linear response and dispersion relations
- 16 Damping and decay
- 17 Star-gas interactions
- 18 Problems and extensions
- 19 Bibliography
- Part II Infinite inhomogeneous systems – galaxy clustering
- Part III Finite spherical systems – clusters of galaxies, galactic nuclei, globular clusters
- Part IV Finite flattened systems – galaxies
- Index
- Frontmatter
- Contents
- Preface
- Introduction
- Part I Idealized homogeneous systems – basic ideas and gentle relaxation
- 1 The average and fluctuating gravitational fields
- 2 Gentle relaxation: timescales
- 3 The dynamics of random impulsive forces
- 4 General properties of Fokker–Planck evolution
- 5 Fokker–Planck description of gravitating systems
- 6 Dynamics with a memory: non-Markovian evolution
- 7 The Boltzmann equation
- 8 Some properties of the Boltzmann equation
- 9 The virial theorem
- 10 The grand description – Liouville's equation and entropy
- 11 Extracting knowledge: the BBGKY hierarchy
- 12 Extracting knowledge: the Fourier development
- 13 Collective effects – grexons
- 14 Collective scattering
- 15 Linear response and dispersion relations
- 16 Damping and decay
- 17 Star-gas interactions
- 18 Problems and extensions
- 19 Bibliography
- Part II Infinite inhomogeneous systems – galaxy clustering
- Part III Finite spherical systems – clusters of galaxies, galactic nuclei, globular clusters
- Part IV Finite flattened systems – galaxies
- Index
Summary
Of making many books there is no end; and much study is a weariness of the flesh.
EcclesiastesIn listing references, I have only included those most directly related to the text. The subject advances so fast that, at time t, there is not much point in listing a bibliography which is up-to-date as of a time t - τ, for it will be out of date by about t + τ. And these days the most informative complete bibliography is found in Astronomy and Astrophysics Abstracts. So with apologies to everyone, past and present, who is not mentioned, here are the references on which parts of the text are based, or to which the text refers directly. Other related references can be found in the sections on problems and extensions. They provide an entry into the literature rather than a summary of it.
There are a number of classical texts on stellar dynamics, orbit theory and celestial mechanics. Representative examples are:
Arnold, V.I., 1978. Mathematical Methods of Classical Mechanics (New York: Springer-Verlag).
Chandrasekhar, S., 1960. Principles of Stellar Dynamics (New York: Dover).
Chandrasekhar, S., 1961. Hydrodynamic and Hydromagnetic Stability (London: Oxford UP).
Chandrasekhar, S., 1969. Ellipsoidal Figures of Equilibrium (New Haven: Yale UP).
Hagihara, Y., 1970, 1972. Celestial Mechanics (Cambridge Mass: MIT Press).
Hamilton, W.R., 1834. On a general method in dynamics Phil. Trans. Roy. Soc., Pt. 11, 124, 247.
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- Chapter
- Information
- Gravitational Physics of Stellar and Galactic Systems , pp. 131 - 134Publisher: Cambridge University PressPrint publication year: 1985