User:Tohline/ThreeDimensionalConfigurations/EFE Energies

Properties of Homogeneous Ellipsoids (2)

In addition to pulling from §53 of Chandrasekhar's EFE, here, we lean heavily on the papers by M. D. Weinberg & S. Tremaine (1983, ApJ, 271, 586) (hereafter, WT83) and by D. M. Christodoulou, D. Kazanas, I. Shlosman, & J. E. Tohline (1995, ApJ, 446, 472) (hereafter, Paper I).

Sequence-Defining Dimensionless Parameters

A Riemann sequence of S-type ellipsoids is defined by the value of the dimensionless parameter,

<math>~f</math>

<math>~\equiv</math>

<math>~\frac{\zeta}{\Omega} = </math> constant,

[ EFE, §48, Eq. (31) ]
[ WT83, Eq. (5) ]
[ Paper I, Eq. (2.1) ]

where, <math>~\zeta</math> is the system's vorticity as measured in a frame rotating with angular velocity, <math>~\Omega</math>. Alternatively, we can use the dimensionless parameter,

<math>~x</math>

<math>~\equiv</math>

<math>~\biggl[\frac{ab}{a^2 + b^2} \biggr]f \, ,</math>

[ EFE, §48, Eq. (40) ]
[ Paper I, Eq. (2.2) ]

or,

<math>~\Lambda</math>

<math>~\equiv</math>

<math>~-\biggl[\frac{ab}{a^2 + b^2} \biggr] \Omega f = -\Omega x \, .</math>

[ WT83, Eq. (4) ]

Conserved Quantities

Algebraic expressions for the conserved energy, <math>~E</math>, angular momentum, <math>~L</math>, and circulation, <math>~C</math>, are, respectively,

<math>~E</math>	<math>~=</math>	<math>~\frac{1}{2}v^2 + \frac{1}{2}(a^2 + b^2)(\Lambda^2 + \Omega^2) - 2ab\Lambda\Omega - 2I </math>
	<math>~\rightarrow</math>	<math>~\cancelto{0}{\frac{1}{2}v^2} + \frac{1}{2} [(a+bx)^2 + (b+ax)^2]\Omega^2 - 2I \, ,</math>

[ 1^st expression — EFE, §53, Eq. (239) ]
[ 2^nd expression — Paper I, Eq. (2.7) ]

where — see an accompanying discussion for the definitions of <math>~A_1</math>, <math>~A_2</math>, and <math>~A_3</math>,

<math>~I</math>

<math>~=</math>

<math>~A_1a^2 + A_2b^2 + A_3c^2 \, ;</math>

[ 1^st expression — EFE, §53, Eq. (239) ]
[ 2^nd expression — Paper I, Eq. (2.8) ]

<math>~\frac{5L}{M}</math>	<math>~=</math>	<math>~(a^2 + b^2)\Omega - 2ab\Lambda</math>
	<math>~=</math>	<math>~ (a^2 + b^2 + 2abx)\Omega \, ;</math>

[ 1^st expression — EFE, §53, Eq. (240) ]
[ 2^nd expression — Paper I, Eq. (2.5) ]

<math>~\frac{5C}{M}</math>	<math>~=</math>	<math>~(a^2 + b^2)\Lambda - 2ab\Omega</math>
	<math>~=</math>	<math>~- [2ab + (a^2 + b^2)x ]\Omega \, .</math>

[ 1^st expression — EFE, §53, Eq. (241) ]
[ 2^nd expression — Paper I, Eq. (2.6) ]

Note that, based on the units chosen in Paper I, <math>~M = 5</math>, and <math>~abc = 15/4</math>.

Aside: Chandra's Notation

According to equation (107) in §21 of EFE, it appears as though,

<math>~A_i - A_j</math>

<math>~=</math>

<math>~- (a_i^2 - a_j^2)A_{ij} \, .</math>

And, according to equation (105) in §21 of EFE, it appears as though,

<math>~B_{ij}</math>

<math>~=</math>

<math>~A_j - a_i^2A_{ij} \, .</math>

Hence, according to equation (8) in §39 of EFE, the angular frequency of a Jacobi ellipsoid is,

<math>~\Omega^2</math>	<math>~=</math>	<math>~2\biggl[ 1 - \biggl(\frac{a_3}{a_1}\biggr)^2 \biggr]B_{13}</math>
	<math>~=</math>	<math>~2\biggl[ 1 - \biggl(\frac{a_3}{a_1}\biggr)^2 \biggr]\biggl\{A_3 - a_1^2A_{13}\biggr\}</math>
	<math>~=</math>	<math>~2\biggl[ 1 - \biggl(\frac{a_3}{a_1}\biggr)^2 \biggr] \biggl\{A_3 + a_1^2\biggl[\frac{A_1-A_3}{a_1^2-a_3^2} \biggr] \biggr\} </math>

No! Do equations (4) and (5) instead!

Free Energy Surface(s)

Scope

Consider a self-gravitating ellipsoid having the following properties:

• Semi-axis lengths, <math>~(x,y,z)_\mathrm{surface} = (a,b,c)</math>, and corresponding volume, <math>~4\pi/(3abc)</math>  ; and consider only the situations <math>0 \le b/a \le 1</math> and <math>0 \le c/a \le 1</math>  ;
• Total mass, <math>~M</math>  ;
• Uniform density, <math>~\rho = (3 M)/(4\pi abc) </math>  ;
• Figure is spinning about its c axis with angular velocity, <math>~\Omega</math>  ;
• Internal, steady-state flow exhibiting the following characteristics:
• No vertical (z) motion;
• Elliptical (x-y plane) streamlines everywhere having an ellipticity that matches that of the overall figure, that is, <math>~e = (1-b^2/a^2)^{1/2}</math>  ;
• The velocity components, <math>~v_x</math> and <math>~v_y</math>, are linear in the coordinate and, overall, characterized by the magnitude of the vorticity, <math>~\zeta</math>  .

Such a configuration is uniquely specified by the choice of six key parameters:   <math>~a</math>, <math>~b</math>, <math>~c</math>, <math>~M</math>, <math>~\Omega</math>, and <math>~\zeta</math>  .

Free Energy of Incompressible, Constant Mass Systems

We are interested, here, in examining how the free energy of such a system will vary as it is allowed to "evolve" as an incompressible fluid — i.e., holding <math>~\rho</math> fixed — through different ellipsoidal shapes while conserving its total mass. Following Paper I, we choose to set <math>~M = 5</math> — which removes mass from the list of unspecified key parameters — and we choose to set <math>~\rho = \pi^{-1}</math>, which is then reflected in a specification of the semi-axis, <math>~c</math>, in terms of the other two semi-axes, namely,

<math>~c</math>

<math>~=</math>

<math>~\frac{3M}{4\pi(ab)\rho} = \frac{15}{4ab} \, .</math>

Moving forward, then, a unique ellipsoidal configuration is identified via the specification of four, rather than six, key parameters —   <math>~a</math>, <math>~b</math>, <math>~\Omega</math>, and <math>~\zeta</math>   — and the free energy of that configuration is given by the expression,

<math>~E</math>

<math>~=</math>

<math>~\frac{1}{2} [(a+bx)^2 + (b+ax)^2]\Omega^2 - 2I \, ,</math>

[ EFE, §53, Eq. (239) ]
[ Paper I, Eq. (2.7) ]

where,

<math>~x</math>

<math>~\equiv</math>

<math>~\biggl[\frac{ab}{a^2 + b^2} \biggr]\frac{\zeta}{\Omega} \, ,</math>

[ EFE, §48, Eq. (40) ]
[ Paper I, Eq. (2.2) ]

and,

<math>~I</math>

<math>~=</math>

<math>~A_1a^2 + A_2b^2 + A_3\biggl(\frac{15}{4ab}\biggr)^2 \, ,</math>

[ 1^st expression — EFE, §53, Eq. (239) ]
[ 2^nd expression — Paper I, Eq. (2.8) ]

— see an accompanying discussion for the definitions of the ellipticity-dependent coefficients, <math>~A_1(e)</math>, <math>~A_2(e)</math>, and <math>~A_3(e)</math>.

See Also

• Properties of Maclaurin Spheroids
• Excerpts from Maclaurin's (1742) A Treatise of Fluxions

© 2014 - 2021 by Joel E. Tohline |   H_Book Home   |   YouTube   | Appendices: | Equations | Variables | References | Ramblings | Images | myphys.lsu | ADS | 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