Aps/MaclaurinSpheroidFreeFall: Difference between revisions

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"In the course of researches on the formation of galaxies one meets the following idealized problem.  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."
"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."
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==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 as follows:
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 &hellip;


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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, (ϖ,φ,z), and to simplify the individual equations as described in our accompanying discussion. The resulting set of simplified governing relations is …

Equation of Continuity

dρdt+ρϖϖ[ϖϖ˙]+ρz[ρz˙]=0


Euler Equation

e^ϖ[dϖ˙dtϖφ˙2]+e^φ[d(ϖφ˙)dt+ϖ˙φ˙]+e^z[dz˙dt]=e^ϖ[1ρPϖ+Φϖ]e^z[1ρPz+Φz]


Adiabatic Form of the
First Law of Thermodynamics

dϵdt+Pddt(1ρ)=0


Poisson Equation

1ϖϖ[ϖΦϖ]+2Φz2=4πGρ.

Key References

Comment by J. E. Tohline: In §II of this "1964" article, Lynden-Bell references his 1962 article with an incorrect year (Lynden-Bell 1963); within his list of REFERENCES, the year (1962) is correct, but the journal volume is incorrectly identified as 50 (it should be vol. 58).
Comment by J. E. Tohline: In §II of this "1964" article, Lynden-Bell references his 1962 article with an incorrect year (Lynden-Bell 1963); within his list of REFERENCES, the year (1962) is correct, but the journal volume is incorrectly identified as 50 (it should be vol. 58).

 

  • 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

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