Aps/MaclaurinSpheroidFreeFall: Difference between revisions
| Line 9: | Line 9: | ||
<tr><td align="left"> | <tr><td align="left"> | ||
<font color="darkgreen"> | <font color="darkgreen"> | ||
" | "What is the form of the collapse under gravitational forces of a uniformly rotating spheroidal gas cloud? In the special case where initially the gas is absolutely cold and of uniform density within the spheroid, we show that the collapse proceeds through a series of uniform, uniformly rotating spheroids until a disk is formed." | ||
</font> | </font> | ||
</td></tr> | </td></tr> | ||
| Line 20: | Line 20: | ||
==Simplified Governing Relations== | ==Simplified Governing Relations== | ||
When studying the dynamical evolution of strictly axisymmetric configurations, it proves useful to write the spatial operators in our overarching set of [[PGE|principal governing equations]] in terms of cylindrical coordinates and to simplify the individual equations as described in our [[AxisymmetricConfigurations/PGE#Governing_Equations_.28CYL..29|accompanying discussion]]. The resulting set of simplified governing relations is | When studying the dynamical evolution of strictly axisymmetric configurations, it proves useful to write the spatial operators in our overarching set of [[PGE|principal governing equations]] in terms of cylindrical coordinates, <math>(\varpi, \varphi, z)</math>, and to simplify the individual equations as described in our [[AxisymmetricConfigurations/PGE#Governing_Equations_.28CYL..29|accompanying discussion]]. The resulting set of simplified governing relations is … | ||
<div align="center"> | <div align="center"> | ||
Revision as of 17:46, 1 November 2021
Free-Fall Collapse of an Homogeneous Spheroid
| Free-Fall Collapse of an Homogeneous Spheroid |
|---|
|
"What is the form of the collapse under gravitational forces of a uniformly rotating spheroidal gas cloud? In the special case where initially the gas is absolutely cold and of uniform density within the spheroid, we show that the collapse proceeds through a series of uniform, uniformly rotating spheroids until a disk is formed." |
|
— Drawn from 📚 D. Lynden-Bell (1962, Math. Proc. Cambridge Phil. Soc., Vol. 58, Issue 4, pp. 709 - 711) |
Simplified Governing Relations
When studying the dynamical evolution of strictly axisymmetric configurations, it proves useful to write the spatial operators in our overarching set of principal governing equations in terms of cylindrical coordinates, , and to simplify the individual equations as described in our accompanying discussion. The resulting set of simplified governing relations is …
Equation of Continuity
Euler Equation
Adiabatic Form of the
First Law of Thermodynamics
Poisson Equation
Key References
- 📚 D. Lynden-Bell (1962, Math. Proc. Cambridge Phil. Soc., Vol. 58, Issue 4, pp. 709 - 711): On the gravitational collapse of a cold rotating gas cloud
NOTE … according to the new ADS listing, the authors associated with this paper should be, D. Lynden-Bell & C. T. C. Wall (Charles Terence Clegg "Terry" Wall); however, the archived article, itself, lists Lynden-Bell as the sole author while indicating that the paper was simply being communicated by Wall.

- D. Lynden-Bell (1964), ApJ, 139, 1195 - 1216: On Large-Scale Instabilities during Gravitational Collapse and the Evolution of Shrinking Maclaurin Spheroids
- Classic paper by C. C. Lin, Leon Mestel, and Frank Shu (1965, ApJ, 142, 1431 - 1446) titled, "The Gravitational Collapse of a Uniform Spheroid."
See Also
|
Appendices: | VisTrailsEquations | VisTrailsVariables | References | Ramblings | VisTrailsImages | myphys.lsu | ADS | |