Difference between revisions of "User:Tohline/Apps/DysonWongTori"

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* [http://adsabs.harvard.edu/abs/2016AJ....152...35F T. Fukushima (2016, AJ, 152, article id. 35, 31 pp.)] — ''Zonal Toroidal Harmonic Expansions of External Gravitational Fields for Ring-like Objects''
* [http://adsabs.harvard.edu/abs/2016AJ....152...35F T. Fukushima (2016, AJ, 152, article id. 35, 31 pp.)] — ''Zonal Toroidal Harmonic Expansions of External Gravitational Fields for Ring-like Objects''
* [http://adsabs.harvard.edu/abs/2016ApJ...829...45K W.-T. Kim & S. Moon (2016, ApJ, 829, article id. 45, 22 pp.)] — ''Equilibrium Sequences and Gravitational Instability of Rotating Isothermal Rings''
* [http://adsabs.harvard.edu/abs/2016ApJ...829...45K W.-T. Kim & S. Moon (2016, ApJ, 829, article id. 45, 22 pp.)] — ''Equilibrium Sequences and Gravitational Instability of Rotating Isothermal Rings''
* [http://adsabs.harvard.edu/abs/2008MNRAS.389..156P D. Petroff & S. Horatschek (2008, MNRAS, 389,156 - 172)] — ''Uniformly Rotating Homogeneous and Polytropic Rings in Newtonian Gravity''
* [http://adsabs.harvard.edu/abs/2006IJMPB..20.3113C P. H. Chavanis (2006, International Journal of Modern Physics B, 20, 3113 - 3198)] — ''Phase Transitions in Self-Gravitating Systems''
* [http://adsabs.harvard.edu/abs/2006IJMPB..20.3113C P. H. Chavanis (2006, International Journal of Modern Physics B, 20, 3113 - 3198)] — ''Phase Transitions in Self-Gravitating Systems''
* [http://adsabs.harvard.edu/abs/2001A%26A...375.1091L M. Lombardi & G. Bertin (2001, Astronomy & Astrophysics, 375, 1091 - 1099)] — ''Boyle's Law and Gravitational Instability''
* [http://adsabs.harvard.edu/abs/2001A%26A...375.1091L M. Lombardi & G. Bertin (2001, Astronomy & Astrophysics, 375, 1091 - 1099)] — ''Boyle's Law and Gravitational Instability''

Revision as of 22:12, 10 August 2017

Self-Gravitating, Incompressible (Dyson-Wong) Tori

Much of the introductory material of this chapter has been drawn from the paper by Tohline & Hachisu (1990) titled, The Breakup of Self-Gravitating Rings, Tori, and Accretion Disks.

Whitworth's (1981) Isothermal Free-Energy Surface
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Overview

In his pioneering work, F. W. Dyson (1893, Philosophical Transactions of the Royal Society of London. A., 184, 43 - 95) used analytic techniques to determine the approximate equilibrium structure of axisymmetric, uniformly rotating, incompressible tori. C.-Y. Wong (1974, ApJ, 190, 675 - 694) extended Dyson's work, using numerical techniques to obtain more accurate — but still approximate — equilibrium structures for incompressible tori having solid body rotation. Since then, Y. Eriguchi & D. Sugimoto (1981, Progress of Theoretical Physics, 65, 1870 - 1875) and I. Hachisu, J. E. Tohline & Y. Eriguchi (1987, ApJ, 323, 592 - 613) have mapped out the full sequence of Dyson-Wong tori, beginning from a bifurcation point on the Maclaurin spheroid sequence.

References

 

Whitworth's (1981) Isothermal Free-Energy Surface

© 2014 - 2021 by Joel E. Tohline
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Recommended citation:   Tohline, Joel E. (2021), The Structure, Stability, & Dynamics of Self-Gravitating Fluids, a (MediaWiki-based) Vistrails.org publication, https://www.vistrails.org/index.php/User:Tohline/citation