ParabolicDensity/Axisymmetric/Structure: Difference between revisions

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===Gravitational Potential===
===Gravitational Potential===
For an oblate-spheroidal configuration &#8212; that is, when <math>a_s < a_m = a_\ell</math> &#8212; the gravitational potential may be obtained from the expression,
As we have detailed in [[ThreeDimensionalConfigurations/FerrersPotential|an accompanying discussion]], for an oblate-spheroidal configuration &#8212; that is, when <math>a_s < a_m = a_\ell</math> &#8212; the gravitational potential may be obtained from the expression,


In our [[ThreeDimensionalConfigurations/FerrersPotential|accompanying discussion]]  we find that,
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====Index Symbol Expressions====
The expression for the zeroth-order normalization term <math>(I_{BT})</math>, and the relevant pair of 1<sup>st</sup>-order index symbol expressions are:
The expression for the zeroth-order normalization term <math>(I_{BT})</math>, and the relevant pair of 1<sup>st</sup>-order index symbol expressions are:



Revision as of 10:18, 5 August 2024

Parabolic Density Distribution


Part I:   Gravitational Potential

 


Part II:   Spherical Structures

 


Part III:   Axisymmetric Equilibrium Structures

 


Part IV:   Triaxial Equilibrium Structures (Exploration)

 

Axisymmetric (Oblate) Equilibrium Structures

Here we specifically discuss the case of configurations that exhibit concentric ellipsoidal iso-density surfaces of the form,

ρ

=

ρc[1−(x2+y2aℓ2+z2as2)],

that is, axisymmetric (am=aℓ, i.e., oblate) configurations with parabolic density distributions. Much of our presentation, here, is drawn from our separate, detailed description of what we will refer to as Ferrers potential.

Gravitational Potential

As we have detailed in an accompanying discussion, for an oblate-spheroidal configuration — that is, when as<am=aℓ — the gravitational potential may be obtained from the expression,

Φgrav(𝐱)(−πGρc)

=

12IBTa12−(A1x2+A2y2+A3z2)+(A12x2y2+A13x2z2+A23y2z2)+16(3A11x4+3A22y4+3A33z4),

where, in the present context, we can rewrite this expression as,

Φgrav(𝐱)(−πGρc)

=

12IBTaℓ2−[Aℓ(x2+y2)+Asz2]+[Aℓℓx2y2+Aℓsx2z2+Aℓsy2z2]+16[3Aℓℓx4+3Aℓℓy4+3Assz4]

 

=

12IBTaℓ2−[Aℓϖ2+Asz2]+[Aℓℓx2y2+Aℓsϖ2z2]+12[Aℓℓ(x4+y4)+Assz4]

 

=

12IBTaℓ2−[Aℓϖ2+Asz2]+Aℓℓ2[(x2+y2)2]+12[Assz4]+[Aℓsϖ2z2]

 

=

12IBTaℓ2−[Aℓϖ2+Asz2]+Aℓℓ2[ϖ4]+12[Assz4]+[Aℓsϖ2z2]

⇒Φgrav(𝐱)(−πGρcaℓ2)

=

12IBT−[Aℓ(ϖ2aℓ2)+As(z2aℓ2)]+12[Aℓℓaℓ2(ϖ4aℓ4)+Assaℓ2(z4aℓ4)+2Aℓsaℓ2(ϖ2z2aℓ4)].

Index Symbol Expressions

The expression for the zeroth-order normalization term (IBT), and the relevant pair of 1st-order index symbol expressions are:

IBT =

2Aℓ+As(1−e2)=2(1−e2)1/2[sin−1ee];

Aℓ

=

1e2[sin−1ee−(1−e2)1/2](1−e2)1/2;

As =

2e2[(1−e2)−1/2−sin−1ee](1−e2)1/2,

[EFE], Chapter 3, Eq. (36)
[T78], §4.5, Eqs. (48) & (49)

where the eccentricity,

e≡[1−(asaℓ)2]1/2.

The relevant 2nd-order index symbol expressions are:

aℓ2Aℓℓ

=

14e4{−(3+2e2)(1−e2)+3(1−e2)1/2[sin−1ee]};

32aℓ2Ass

=

(4e2−3)e4(1−e2)+3(1−e2)1/2e4[sin−1ee];

aℓ2Aℓs

=

1e4{(3−e2)−3(1−e2)1/2[sin−1ee]}.

We can crosscheck this last expression by drawing on a shortcut expression,

Aℓs

=

−Aℓ−As(aℓ2−as2)

⇒aℓ2Aℓs

=

1e2{As−Aℓ}

 

=

1e2{2e2[(1−e2)−1/2−sin−1ee](1−e2)1/2−1e2[sin−1ee−(1−e2)1/2](1−e2)1/2}

 

=

1e4{[2−2(1−e2)1/2sin−1ee]−[(1−e2)1/2sin−1ee−(1−e2)]}

 

=

1e4{(3−e2)−3(1−e2)1/2sin−1ee}.

See Also

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