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<font color="darkblue">'''[[User:Tohline/SSC/Perturbations|Solution Strategy]]'''</font> | |||
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<font color="darkblue">'''[[User:Tohline/SSC/VirialStability|Virial Stability]]'''</font> | |||
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Example Solutions: | |||
* [[User:Tohline/SSC/UniformDensity|Uniform-density sphere]] | |||
* [[User:Tohline/SSC/Polytropes|Polytropes]] | |||
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===<font color="darkblue">'''[[User:Tohline/SphericallySymmetricConfigurations|Dynamics]]:'''</font>=== | ===<font color="darkblue">'''[[User:Tohline/SphericallySymmetricConfigurations|Dynamics]]:'''</font>=== |
Revision as of 21:23, 9 September 2012
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Preface from the original version of this HyperText Book (H_Book):
November 18, 1994
Much of our present, basic understanding of the structure, stability, and dynamical evolution of individual stars, short-period binary star systems, and the gaseous disks that are associated with numerous types of stellar systems (including galaxies) is derived from an examination of the behavior of a specific set of coupled, partial differential equations. These equations — most of which also are heavily utilized in studies of continuum flows in terrestrial environments — are thought to govern the underlying physics of all macroscopic "fluid" systems in astronomy. Although relatively simple in form, they prove to be very rich in nature... <more>
Pictorial Table of Contents
Context
- Principal Governing Equations
- Continuity Equation
- Euler Equation
- <math>1^\mathrm{st}</math> Law of Thermodynamics
- Poisson Equation
- Virial Equations
Applications
Spherically Symmetric Configurations
Structure:
Example Solutions: |
Stability:
Example Solutions: |
Dynamics:
Two-Dimensional Configurations
- Introduction
Structure:
- Solution Strategies
- Example Solutions:
- Maclaurin Spheroids
- Rotationally Flattened, Isothermal Structures
- Polytropic Tori:
- Papaloizou-Pringle (massless) Tori
- Self-gravitating Tori
- Infinitesimally Thin, Nonaxisymmetric Disk
Stability:
Dynamics:
Three-Dimensional Configurations
- Introduction
Structure:
- Solution Strategies
- Example Solutions:
- Ellipsoidal Figures of Equilibrium
- Compressible Analogs of Riemann Ellipsoids; see also Note to Hirschmann & Neilsen and Suggested Strategy by Joel
Stability:
Dynamics:
Appendices
See Also
- NIST Digital Library of Mathematical Functions; see also the related CUP Publication
© 2014 - 2021 by Joel E. Tohline |