ParabolicDensity/Axisymmetric/Structure: Difference between revisions
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\frac{3 (1-e^2)^{1 / 2}}{e^4} \biggl[\frac{\sin^{-1}e}{e}\biggr] | \frac{3 (1-e^2)^{1 / 2}}{e^4} \biggl[\frac{\sin^{-1}e}{e}\biggr] | ||
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Revision as of 20:02, 4 August 2024
Parabolic Density Distribution
Part I: Gravitational Potential
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Part II: Spherical Structures
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Part III: Axisymmetric Equilibrium Structures
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Part IV: Triaxial Equilibrium Structures (Exploration)
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Axisymmetric (Oblate) Equilibrium Structures
Here we specifically discuss the case of configurations that exhibit concentric ellipsoidal iso-density surfaces of the form,
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that is, axisymmetric (, 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
For an oblate-spheroidal configuration — that is, when — the gravitational potential may be obtained from the expression,
In our accompanying discussion we find that,
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where, in the present context, we can rewrite this expression as,
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The expression for the zeroth-order normalization term , and the relevant pair of 1st-order index symbol expressions are:
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where the eccentricity,
The relevant 2nd-order index symbol expressions are:
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We can crosscheck this last expression by drawing on a shortcut expression,
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See Also
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Appendices: | VisTrailsEquations | VisTrailsVariables | References | Ramblings | VisTrailsImages | myphys.lsu | ADS | |