Difference between revisions of "User:Tohline/2DStructure/ToroidalGreenFunction"

From VistrailsWiki
Jump to navigation Jump to search
Line 1,150: Line 1,150:
==Uniform-Density Torus==
==Uniform-Density Torus==


From an [[User:Tohline/Apps/DysonWongTori#Introducing_Toroidal_Coordinates|accompanying review]], we see that for a torus of major radius <math>~R</math> and minor radius <math>~d</math>, the most accommodating (cylindrical-coordinate-based) radial  coordinate location of the toroidal coordinate system's ''anchor ring'', <math>~a</math>, is defined such that,
In an [[User:Tohline/Apps/Wong1973Potential#Wong.27s_.281973.29_Analytic_Potential|accompanying discussion]], we build upon the above technical foundation and detail how [http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)] was able to complete both integrals to derive an analytic expression for the potential (inside as well as outside) of axisymmetric, uniform-density tori having an arbitrarily specified ratio of the major to minor (cross-sectional) radii, <math>~R/d</math>.  This is an outstanding accomplishment that has received little attention in the astrophysics literature and, therefore, has heretofore been underappreciated.
<div align="center">
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~a^2</math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>~R^2 - d^2 \, .</math>
  </td>
</tr>
<tr>
  <td align="center" colspan="3">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], Eq. (2.8)
  </td>
</tr>
</table>
</div>
Then the corresponding (toroidal-coordinate-based) radial coordinate location <math>~\eta_0</math> of the surface of the torus is,
<div align="center">
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\eta_0</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\cosh^{-1}\biggl(\frac{R}{d}\biggr) \, .</math>
  </td>
</tr>
<tr>
  <td align="center" colspan="3">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], Eq. (2.9)
  </td>
</tr>
</table>
</div>
Alternatively, given <math>~\eta_0</math> and the value of the parameter <math>~a</math>, we have,
<div align="center">
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~R</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~a \coth\eta_0 \, ,</math>
  </td>
</tr>
 
<tr>
  <td align="right">
<math>~d</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\frac{a}{\sinh\eta_0} \, .</math>
  </td>
</tr>
<tr>
  <td align="center" colspan="3">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], Eqs. (2.10) &amp; (2.11)
  </td>
</tr>
</table>
</div>
 
If such an axisymmetric torus has a uniform density, <math>~\rho_0</math>, then according to the Cohl &amp; Tohline (1999) expression, the gravitational potential is,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{CT}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~ - 2G\rho_0 a^2 \biggl[ \frac{(\cosh\eta - \cos\theta)}{\sinh\eta } \biggr]^{1 / 2}
\int_{\eta_0}^\infty d\eta^' \int_{-\pi}^\pi d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{- 1 / 2}(\Chi)  \, .
</math>
  </td>
</tr>
</table>
 
In contrast, according to Wong's (1973) expression, the gravitational potential is,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
- 2G \rho_0 a^2 (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n
\int_{\eta_0}^\infty d\eta^' ~\sinh\eta^'~P_{n-1 / 2}(\cosh\eta_<) ~Q_{n-1 / 2}(\cosh\eta_>)
\int_{-\pi}^\pi \frac{ \cos[n(\theta - \theta^')] d\theta^' }{(\cosh\eta^' - \cos\theta^')^{5/2}}
\, .
</math>
  </td>
</tr>
<tr>
  <td align="center" colspan="3">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], p. 293, Eq. (2.55)
  </td>
</tr>
</table>
 
===Which Is Easier to Evaluate?===
Upon evaluation, the expressions for <math>~\Phi_\mathrm{CT}</math> and for <math>~\Phi_\mathrm{W}</math> should give identical values for the gravitational potential at all coordinate locations <math>~(\eta,\theta)</math> across the entire meridional plane.  But which of the two expressions is easier to evaluate?
 
====CT====
If the desire is to perform the evaluation numerically, then the <math>~\Phi_\mathrm{CT}</math> expression is almost certainly easier to contend with.  It ''only'' requires a double integration; and as has been detailed in an [[User:Tohline/2DStructure/ToroidalCoordinates#Expression_for_the_Axisymmetric_Potential|accompanying discussion]], the only relatively unfamiliar special function that appears in the integrand, <math>~Q_{-\frac{1}{2}}(\Chi)</math>, can be re-expressed in terms of (the more familiar) complete elliptic integral of the first kind, namely,
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~Q_{-\frac{1}{2}}(\Chi)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\mu K(\mu) \, ,
</math>
  </td>
</tr>
</table>
where,
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\mu</math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>~\biggl[ \frac{2}{\Chi + 1} \biggr]^{1 / 2}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\biggl[ \frac{2 \sinh\eta \cdot \sinh\eta^' }{ \cosh(\eta^' + \eta) - \cos(\theta^' - \theta) } \biggr]^{1 / 2} \, .</math>
  </td>
</tr>
</table>
 
The task is daunting, however, if the desire is to evaluate the expression for <math>~\Phi_\mathrm{CT}</math> ''analytically.'' To our knowledge, no one has yet been able to start from the expression as presented here for <math>~\Phi_\mathrm{CT}</math> and complete the integral over the angular coordinate, <math>~\theta^'</math>, analytically, let alone analytically evaluate the second, ''radial'' integral.  This is principally because the integrand of the first (angular) integral contains a nontrivial function multiplied by a special function whose argument is, itself, a nontrivial function of both <math>~\theta^'</math> and <math>~\eta^'</math>.
 
====W====
 
At first glance, the expression for <math>~\Phi_\mathrm{W}</math> is much more complex than the expression for <math>~\Phi_\mathrm{CT}</math>.  It not only requires a double integration, but also an infinite-series summation over the integer index, <math>~n</math>; and the radial integrand contains a product of two (relatively unfamiliar) associated Legendre functions of various half-integer orders (toroidal functions).  Developing a numerical algorithm to evaluate <math>~\Phi_\mathrm{W}</math> to a certain accuracy &#8212; presumably set by the number of terms included in the summation over <math>~n</math> &#8212; would certainly be a more challenging task than developing a numerical algorithm to evaluate <math>~\Phi_\mathrm{CT}</math>.
 
=====Analytic Integration Over the Angular Coordinate=====
However, focusing only on the integration over the angular coordinate, we see that the integrand in the expression for <math>~\Phi_\mathrm{W}</math> is significantly less imposing than the one that appears in the expression for <math>~\Phi_\mathrm{CT}</math>.  [http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)] was able to evaluate this definite integral in closed form, analytically.  While Wong does not record the detailed steps that he used to evaluate this definite integral, he does indicate that he received guidance from Volume I of [https://authors.library.caltech.edu/43491/1/Volume%201.pdf A. Erd&eacute;lyi's (1953)] ''Higher Transcendental Functions''.  We therefore presume that he adopted the line of reasoning that we have [[#A.3|detailed in the Appendix, below, in deriving the expression labeled]] <font color="green" size="+1">&#x2462;</font>.  Wong recognized, what we have explicitly demonstrated, namely,
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\int_{-\pi}^\pi d\theta^' (\cosh\eta^' - \cos\theta^')^{- 5 / 2} \cos[n(\theta - \theta^')]</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="right">
<math>~2\cos(n\theta)
\int_0^\pi \frac{ \cos(n\theta^')~d\theta^' }{ (\cosh\eta^' - \cos \theta^')^{\frac{5}{2}} }
</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\frac{8\sqrt{2}}{3} \biggl[ \frac{\cos(n\theta)}{\sinh^2\eta^'} \biggr] Q^2_{n- \frac{1}{2}} (\cosh\eta^') \,.
</math>
  </td>
</tr>
 
<tr>
  <td align="center" colspan="5">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], p. 293, Eq. (2.56)
  </td>
</tr>
</table>
 
<table border="1" cellpadding="10" align="center" width="90%"><tr><td align="left">
<font color="red">'''CAUTION:'''</font>&nbsp; It is important to appreciate that, in this expression as well as in the expressions to follow, the term, <math>~Q^2_{n-\frac{1}{2}}(z)</math>, is ''not'' the square of the zero-order toroidal function, <math>~Q^0_{n - \frac{1}{2}}(z)</math>, but is instead the toroidal function of order two.  In an [[User:Tohline/Appendix/Mathematics/ToroidalSynopsis01#Evaluating_Q2.CE.BD|accompanying discussion]] we present an analytic expression for <math>~Q^2_{-\frac{1}{2}}(z)</math> &#8212; and a separate analytic expression for <math>~Q^1_{-\frac{1}{2}}(z)</math> &#8212; in terms of complete elliptic integrals, as well as a recurrence relation that can be used to generate analytic expressions for all other order-two (and all other order-one) toroidal functions that have higher half-integer degrees, <math>~n-\tfrac{1}{2}</math> for <math>~n \ge 1</math>.
</td></tr></table>
 
 
Hence, Wong was able to simplify the expression for <math>~\Phi_\mathrm{W}</math> to one that &#8212; albeit, in addition to an infinite summation over the index, <math>~n</math> &#8212; only requires integration over the radial coordinate, <math>~\eta^'</math>.  Specifically, he obtained,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
- 2G \rho_0 a^2 (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n
\int_{\eta_0}^\infty d\eta^' ~\sinh\eta^'~P_{n-1 / 2}(\cosh\eta_<) ~Q_{n-1 / 2}(\cosh\eta_>)\biggl\{
\frac{8\sqrt{2}}{3} \biggl[ \frac{\cos(n\theta)}{\sinh^2\eta^'} \biggr] Q^2_{n- \frac{1}{2}} (\cosh\eta^')
\biggr\}
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
- \biggl( \frac{16\sqrt{2}}{3}  \biggr) G \rho_0 a^2 (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
\int_{\eta_0}^\infty d\eta^' \Biggl[ \frac{Q^2_{n- \frac{1}{2}} (\cosh\eta^')}{\sinh\eta^'} \Biggr] ~P_{n-1 / 2}(\cosh\eta_<) ~Q_{n-1 / 2}(\cosh\eta_>)
\, .
</math>
  </td>
</tr>
 
<tr>
  <td align="center" colspan="3">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], p. 294, Eq. (2.57)
  </td>
</tr>
</table>
 
=====Analytic Integration Over the Radial Coordinate=====
 
Now, in considering how to handle integration over the radial coordinate, <math>~\eta^'</math>, let's examine, first, the case where <math>~\eta^' \ge \eta_0 > \eta</math>, that is, the potential is being evaluated at a location that is entirely outside of the torus.  In this case,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
- \biggl( \frac{16\sqrt{2}}{3}  \biggr) G \rho_0 a^2 (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta) ~P_{n-1 / 2}(\cosh\eta)
\int_{\eta_0}^\infty d\eta^' \Biggl[ \frac{Q^2_{n- \frac{1}{2}} (\cosh\eta^')}{\sinh\eta^'} \Biggr] ~Q_{n-1 / 2}(\cosh\eta^')
\, .
</math>
  </td>
</tr>
</table>
 
So we are interested in carrying out the "radial" integral,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~
\int_{\eta_0}^\infty d\eta^' \sinh\eta^' \Biggl[ \frac{Q^2_{n- \frac{1}{2}} (\cosh\eta^')}{\sinh^2\eta^'} \Biggr] ~Q_{n-1 / 2}(\cosh\eta^')
</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\int_{\cosh(\eta_0)}^{\cosh(\infty)} dt \Biggl[ \frac{Q^2_{n- \frac{1}{2}} (t)~Q_{n-\frac{1}{2}}(t)}{t^2 - 1} \Biggr]  \, ,
</math>
  </td>
</tr>
</table>
where we have made the association, <math>~\cosh\eta^' \rightarrow t</math>, in which case, <math>~dt = \sinh\eta^' d\eta^'</math>.  Following the line of reasoning that we have [[#A.4|detailed in the Appendix, below, in deriving the expression labeled]] <font color="green" size="+1">&#x2463;</font>, this integral can be evaluated in closed form to give,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~
\int_a^b\biggl[  \frac{Q_{n - \frac{1}{2}}^2(t) ~Q_{n - \frac{1}{2}}(t) }{(t^2-1)}\biggr]~dt
</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\frac{1}{4} \biggl[
(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(t) ~ Q_{n - \frac{1}{2}}(t)
-  (n+\tfrac{1}{2})Q_{n+\frac{1}{2}}(t) Q_{n - \frac{1}{2}}^2(t)
\biggr]_a^b \, .
</math>
  </td>
</tr>
<tr>
  <td align="center" colspan="3">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], Eq. (2.58)
  </td>
</tr>
</table>
Hence, we have,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
- \biggl( \frac{4\sqrt{2}}{3}  \biggr) G \rho_0 a^2 (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times P_{n-1 / 2}(\cosh\eta)
\biggl[
(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(t) ~ Q_{n - \frac{1}{2}}(t)
-  (n+\tfrac{1}{2})Q_{n+\frac{1}{2}}(t) Q_{n - \frac{1}{2}}^2(t)
\biggr]_{t = \cosh \eta_0}^{t = \cosh\infty} \, .
</math>
  </td>
</tr>
</table>
Or, given that, in this uniform-density configuration, the [[User:Tohline/Apps/DysonWongTori#DensityFormula|density is exactly the mass divided by the torus volume]], that is,
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\rho_0 = \frac{M}{V}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\frac{M \sinh^3\eta_0}{2\pi^2 a^3 \cosh{\eta_0}} \, ,</math>
  </td>
</tr>
</table>
we have,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
-  \frac{2\sqrt{2}~ GM}{3\pi^2 a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times P_{n-1 / 2}(\cosh\eta)
\biggl[
(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(t) ~ Q_{n - \frac{1}{2}}(t)
-  (n+\tfrac{1}{2})Q_{n+\frac{1}{2}}(t) Q_{n - \frac{1}{2}}^2(t)
\biggr]_{t = \cosh \eta_0}^{t = \cosh\infty} \, .
</math>
  </td>
</tr>
</table>
 
In a [[User:Tohline/Appendix/Mathematics/ToroidalFunctions#Asymptotic_Behavior|separate chapter]], we have examined the asymptotic behavior of the toroidal functions, <math>~Q_{n-\tfrac{1}{2}}(t)</math>, which is,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\lim_{\chi\rightarrow \infty} Q_{n-\frac{1}{2}}(t)</math>
  </td>
  <td align="center">
<math>~\propto</math>
  </td>
  <td align="left">
<math>~
\frac{1}{t^{n+\frac{1}{2}} } \, .
</math>
  </td>
</tr>
 
</table>
This means that, at the upper integration limit, these toroidal functions go to zero.  As a result, we can write,
 
<table border="1" align="center" cellpadding="8">
<tr><td align="center">Exterior Solution: &nbsp;<math>~\eta_0 \ge \eta</math></td></tr>
<tr><td align="left">
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
-  \frac{2\sqrt{2}~ GM}{3\pi^2 a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times P_{n-1 / 2}(\cosh\eta)
\biggl[
(n+\tfrac{1}{2})Q_{n+\frac{1}{2}}(\cosh \eta_0) Q_{n - \frac{1}{2}}^2(\cosh \eta_0)
- (n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(\cosh \eta_0) ~ Q_{n - \frac{1}{2}}(\cosh \eta_0)
\biggr] \, .
</math>
  </td>
</tr>
</table>
 
</td></tr>
</table>
 
This expression matches the potential for the ''exterior region'' that is obtained by combining [http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong's (1973)] Eqs. (2.59), (2.61) and (2.63).
 
Now, let's examine the potential evaluated at a radial location, <math>~\eta</math>, that is positioned inside the surface of the torus.  That is, <math>~\eta_0 < \eta \le \infty</math>.  We need to add expressions that have two different sets of integration limits as follows.  First, over the subregion, <math>~\eta \le \eta^' \le \infty</math>, we use the same expression for <math>~\Phi_\mathrm{W}</math> but employ the new limits, as indicated; and second, over the subregion <math>~\eta_0 \le \eta^' \le \eta</math>, we swap the roles of <math>~P_{n-\frac{1}{2}}</math> and <math>~Q_{n-\frac{1}{2}}</math>.
 
<table border="0" cellpadding="5" align="center">
 
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\Phi_\mathrm{W}|_\mathrm{subregion1} + \Phi_\mathrm{W}|_\mathrm{subregion2}
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
-  \frac{2\sqrt{2}~ GM}{3\pi^2 a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times P_{n-1 / 2}(\cosh\eta)
\biggl[
(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(t) ~ Q_{n - \frac{1}{2}}(t)
-  (n+\tfrac{1}{2})Q_{n+\frac{1}{2}}(t) Q_{n - \frac{1}{2}}^2(t)
\biggr]_{t = \cosh \eta}^{t = \cosh\infty}
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
-  \frac{2\sqrt{2}~ GM}{3\pi^2 a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times Q_{n-1 / 2}(\cosh\eta)
\biggl[
(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(t) ~ P_{n - \frac{1}{2}}(t)
-  (n+\tfrac{1}{2})P_{n+\frac{1}{2}}(t) Q_{n - \frac{1}{2}}^2(t)
\biggr]_{t = \cosh \eta_0}^{t = \cosh\eta}
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
-  \frac{2\sqrt{2}~ GM}{3\pi^2 a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times \biggl\{ P_{n-1 / 2}(\cosh\eta)
\biggl[
(n+\tfrac{1}{2})Q_{n+\frac{1}{2}}(\cosh\eta) Q_{n - \frac{1}{2}}^2(\cosh\eta)
- (n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(\cosh\eta) ~ Q_{n - \frac{1}{2}}(\cosh\eta)
\biggr]
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
+ Q_{n-1 / 2}(\cosh\eta)
\biggl[
(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(\cosh\eta) ~ P_{n - \frac{1}{2}}(\cosh\eta)
-  (n+\tfrac{1}{2})P_{n+\frac{1}{2}}(\cosh\eta) Q_{n - \frac{1}{2}}^2(\cosh\eta)
\biggr]
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
- Q_{n-1 / 2}(\cosh\eta)
\biggl[
(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(\cosh{\eta_0}) ~ P_{n - \frac{1}{2}}(\cosh{\eta_0})
-  (n+\tfrac{1}{2})P_{n+\frac{1}{2}}(\cosh{\eta_0}) Q_{n - \frac{1}{2}}^2(\cosh{\eta_0})
\biggr]
\biggr\}
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
-  \frac{2\sqrt{2}~ GM}{3\pi^2 a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times \biggl\{ P_{n-1 / 2}(\cosh\eta)
\biggl[
(n+\tfrac{1}{2})Q_{n+\frac{1}{2}}(\cosh\eta) Q_{n - \frac{1}{2}}^2(\cosh\eta)
\biggr]
- Q_{n-1 / 2}(\cosh\eta)
\biggl[
(n+\tfrac{1}{2})P_{n+\frac{1}{2}}(\cosh\eta) Q_{n - \frac{1}{2}}^2(\cosh\eta)
\biggr]
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
- Q_{n-1 / 2}(\cosh\eta)
\biggl[
(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(\cosh{\eta_0}) ~ P_{n - \frac{1}{2}}(\cosh{\eta_0})
-  (n+\tfrac{1}{2})P_{n+\frac{1}{2}}(\cosh{\eta_0}) Q_{n - \frac{1}{2}}^2(\cosh{\eta_0})
\biggr]
\biggr\}
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
-  \frac{2\sqrt{2}~ GM}{3\pi^2 a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times \biggl\{ 
Q_{n-1 / 2}(\cosh\eta)
\biggl[
(n+\tfrac{1}{2})P_{n+\frac{1}{2}}(\cosh{\eta_0}) Q_{n - \frac{1}{2}}^2(\cosh{\eta_0})
- (n - \tfrac{3}{2}) ~ P_{n - \frac{1}{2}}(\cosh{\eta_0})~Q^2_{n + \frac{1}{2}}(\cosh{\eta_0})
\biggr]
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
- (n+\tfrac{1}{2})Q_{n - \frac{1}{2}}^2(\cosh\eta)  \biggl[
Q_{n-1 / 2}(\cosh\eta) P_{n+\frac{1}{2}}(\cosh\eta)
- Q_{n+\frac{1}{2}}(\cosh\eta) P_{n-1 / 2}(\cosh\eta)
\biggr]
\biggr\}
</math>
  </td>
</tr>
</table>
 
Drawing on the identified "Key Equation" expression,
 
{{ User:Tohline/Math/EQ_Toroidal06 }}
 
and adopting the associations, <math>~z = \xi = \cosh\eta</math> and <math>~\ell \rightarrow (n-\tfrac{1}{2})</math>, we recognize that,
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~(n+\tfrac{1}{2})[P_{n+\frac{1}{2}}(\cosh\eta) Q_{n-\frac{1}{2}} (\cosh\eta) - P_{n-\frac{1}{2}}(\cosh\eta)Q_{n+\frac{1}{2}}(\cosh\eta)] </math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
1 \, .
</math>
  </td>
</tr>
</table>
 
Hence, we can write,
 
<table border="1" align="center" cellpadding="8">
<tr><td align="center">Interior Solution: &nbsp;<math>~\eta \ge \eta_0 </math></td></tr>
<tr><td align="left">
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
-  \frac{2\sqrt{2}~ GM}{3\pi^2 a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta)
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times \biggl\{ 
Q_{n-1 / 2}(\cosh\eta)
\biggl[
  (n+\tfrac{1}{2})P_{n+\frac{1}{2}}(\cosh{\eta_0}) Q_{n - \frac{1}{2}}^2(\cosh{\eta_0})
- (n - \tfrac{3}{2}) ~ P_{n - \frac{1}{2}}(\cosh{\eta_0})~Q^2_{n + \frac{1}{2}}(\cosh{\eta_0})
\biggr] - Q_{n - \frac{1}{2}}^2(\cosh\eta) \biggr\} \, .
</math>
  </td>
</tr>
</table>
 
</td></tr>
</table>
 
 
This expression matches the potential for the ''interior region'' that is obtained by combining [http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong's (1973)] Eqs. (2.59), (2.60) and (2.62).  Finally, drawing on yet another identified "Key Equation," namely,
 
{{ User:Tohline/Math/EQ_Toroidal08 }}
 
[[File:CommentButton02.png|right|100px|Comment by J. E. Tohline on 2 July 2018:  Note that this matches [http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong's (1973)] Eq. (2.64), except that the numerator on the right-hand side of his equation contains  the hyperbolic sine function raised to the first power whereas in our expression it is squared.  We are confident that it should be squared, in part, because the term ''is'' squared when it reappears in Wong's Eq. (2.65).]]and adopting the associations, <math>~\mu \rightarrow 2</math>, <math>~\nu \rightarrow \theta</math>, and <math>~z \rightarrow \cosh\eta</math>, we see that,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~
\sum_{n=0}^\infty \epsilon_n  \cos(n\theta) ~Q^2_{n-\frac{1}{2}}(\cosh\eta)
</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
(-1)^2~\biggl(\frac{\pi}{2} \biggr)^{1 / 2} \Gamma(2 + \tfrac{1}{2})\biggl[ \frac{ \sinh^2\eta }{(\cosh\eta - \cos\theta)^{\frac{5}{2}}} \biggr]
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\biggl(\frac{\pi}{2} \biggr)^{1 / 2} \biggl[ \frac{4! \sqrt{\pi}}{ 4^2 \cdot 2! } \biggr] \biggl[ \frac{ \sinh^2\eta }{(\cosh\eta - \cos\theta)^{\frac{5}{2}} } \biggr]
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
\biggl(\frac{1}{2} \biggr)^{1 / 2} \biggl[ \frac{ 3\pi}{ 2^2} \biggr] \biggl[ \frac{ \sinh^2\eta }{(\cosh\eta - \cos\theta)^{\frac{5}{2}} } \biggr] \, .
</math>
  </td>
</tr>
<tr>
  <td align="center" colspan="3">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], Eq. (2.64)<br />except, see accompanying (pink, scroll-over balloon) COMMENT
  </td>
</tr>
</table>
 
[[File:CommentButton02.png|right|100px|Comment by J. E. Tohline on 2 July 2018:  Note that this matches [http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong's (1973)] Eq. (2.65), except that in his expression the first term inside the curly braces on the right-hand side contains an extra factor of &pi;.  We are confident that our derived expression is correct because it is consistent with the immediately preceding expression &#8212; labeled Eq. (2.64) in [http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)].]]Hence, the ''interior solution'' can be rewritten as,
 
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~\Phi_\mathrm{W}(\eta,\theta)\bigr|_\mathrm{interior}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~ \frac{ GM}{2\pi a}  \biggl[ \frac{\sinh^3\eta_0}{ \cosh{\eta_0}} \biggr] \biggl\{ \biggl[ \frac{ \sinh\eta }{(\cosh\eta - \cos\theta) } \biggr]^2
~ -  ~ \frac{2^2\sqrt{2}~ }{3\pi}  (\cosh\eta - \cos\theta)^{1 / 2}
\sum\limits^\infty_{n=0} \epsilon_n \cos(n\theta) \, .
</math>
  </td>
</tr>
 
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>~
\times
Q_{n-1 / 2}(\cosh\eta)
\biggl[
(n+\tfrac{1}{2})P_{n+\frac{1}{2}}(\cosh{\eta_0}) Q_{n - \frac{1}{2}}^2(\cosh{\eta_0})
- (n - \tfrac{3}{2}) ~ P_{n - \frac{1}{2}}(\cosh{\eta_0})~Q^2_{n + \frac{1}{2}}(\cosh{\eta_0})
\biggr] \biggr\} \, .
</math>
  </td>
</tr>
<tr>
  <td align="center" colspan="3">
[http://adsabs.harvard.edu/abs/1973AnPhy..77..279W Wong (1973)], Eq. (2.65)<br />except, see accompanying (pink, scroll-over balloon) COMMENT
  </td>
</tr>
</table>


=Appendix: Selected Toroidal Function Relationships=
=Appendix: Selected Toroidal Function Relationships=

Revision as of 20:50, 18 July 2018

Using Toroidal Coordinates to Determine the Gravitational Potential

NOTE:   An earlier version of this chapter has been shifted to our "Ramblings" Appendix.

Whitworth's (1981) Isothermal Free-Energy Surface
|   Tiled Menu   |   Tables of Content   |  Banner Video   |  Tohline Home Page   |


Here we build upon our accompanying review of the types of numerical techniques that various astrophysics research groups have developed to solve for the Newtonian gravitational potential, <math>~\Phi(\vec{x})</math>, given a specified, three-dimensional mass distribution, <math>~\rho(\vec{x})</math>. Our focus is on the use of toroidal coordinates to solve the integral formulation of the Poisson equation, namely,

<math>~ \Phi(\vec{x})</math>

<math>~=</math>

<math>~ -G \iiint \frac{\rho(\vec{x}^{~'})}{|\vec{x}^{~'} - \vec{x}|} d^3x^' \, .</math>

For the most part, we will adopt the notation used by C.-Y. Wong (1973, Annals of Physics, 77, 279); in an accompanying discussion, we review additional results from this insightful 1973 paper, as well as a paper of his that was published the following year in The Astrophysical Journal, namely, Wong (1974).

In order to accomplish this task, we first present the expressions that define how toroidal coordinates, <math>~(\eta,\theta,\psi)</math>, map to and from Cartesian coordinates <math>~(x, y, z)</math>, and present the toroidal-coordinate expression for the differential volume element, <math>~d^3 x</math>.

Basic Elements of a Toroidal Coordinate System

Given the meridional-plane coordinate location of a toroidal-coordinate system's axisymmetric anchor ring, <math>~(\varpi,z) = (a,Z_0)</math>, the relationship between toroidal coordinates <math>~(\eta,\theta,\psi) </math>and Cartesian coordinates <math>~(x, y, z)</math> is,

<math>~x</math>

<math>~=</math>

<math>~\frac{a \sinh\eta \cos\psi}{(\cosh\eta - \cos\theta)} \, ,</math>

<math>~y</math>

<math>~=</math>

<math>~\frac{a \sinh\eta \sin\psi}{(\cosh\eta - \cos\theta)} \, ,</math>

<math>~z - Z_0</math>

<math>~=</math>

<math>~\frac{a \sin\theta}{(\cosh\eta - \cos\theta)} \, .</math>

This set of coordinate relations appears as equations 2.1 - 2.3 in Wong (1973). This set of relations may also be found, for example, on p. 1301 within eq. (10.3.75) of [MF53]; in §14.19 of NIST's Digital Library of Mathematical Functions; or even within Wikipedia. (In most cases the implicit assumption is that <math>~Z_0 = 0</math>.) It is clear, of course, that the cylindrical radial coordinate is,

<math>~\varpi = (x^2 + y^2)^{1 / 2}</math>

<math>~=</math>

<math>~\frac{a \sinh\eta}{(\cosh\eta - \cos\theta)} \, .</math>


Mapping the other direction [see equations 2.13 - 2.15 of Wong (1973) ], we have,

<math>~\eta</math>

<math>~=</math>

<math>~\ln\biggl(\frac{r_1}{r_2} \biggr) \, ,</math>

<math>~\cos\theta</math>

<math>~=</math>

<math>~\frac{(r_1^2 + r_2^2 - 4a^2)}{2r_1 r_2} \, ,</math>

<math>~\tan\psi</math>

<math>~=</math>

<math>~\frac{y}{x} \, ,</math>

where,

<math>~r_1^2 </math>

<math>~\equiv</math>

<math>~[(x^2 + y^2)^{1 / 2} + a]^2 + (z-Z_0)^2 \, ,</math>

<math>~r_2^2 </math>

<math>~\equiv</math>

<math>~[(x^2 + y^2)^{1 / 2} - a]^2 + (z-Z_0)^2 \, ,</math>

and <math>~\theta</math> has the same sign as <math>~(z-Z_0)</math>.

 

Comment by J. E. Tohline on 16 August 2017: In equation (2.17) of his §IIB — when Wong (1973) introduces the differential volume element — the variable used to represent the azimuthal coordinate angle switches from ψ to Φ. We will stick with the ψ notation, here.

According to p. 1301, eq. (10.3.75) of [MF53] — or, for example, as found in Wikipedia — in toroidal coordinates the differential volume element is,

<math>~d^3x</math>

<math>~=</math>

<math>~h_\eta h_\theta h_\psi d\eta d\theta d\psi</math>

<math>~=</math>

<math>~\biggl[ \frac{a^3 \sinh\eta}{(\cosh\eta - \cos\theta)^3} \biggr] d\eta~ d\theta~ d\psi \, .</math>


Green's Function Expression

As presented by Wong (1973)

Referencing [MF53], Wong (1973) states that, in toroidal coordinates, the Green's function is,

<math>~\frac{1}{|~\vec{x} - {\vec{x}}^{~'} ~|} </math>

<math>~=</math>

<math>~ \frac{1}{\pi a} \biggl[ (\cosh\eta - \cos\theta)(\cosh \eta^' - \cos\theta^') \biggr]^{1 /2 } \sum\limits^\infty_{m,n=0} (-1)^m \epsilon_m \epsilon_n ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} </math>

 

 

<math>~ \times \cos[m(\psi - \psi^')]\cos[n(\theta - \theta^')] ~\begin{cases}P^m_{n-1 / 2}(\cosh\eta) ~Q^m_{n-1 / 2}(\cosh\eta^') ~~~\eta^' > \eta \\P^m_{n-1 / 2}(\cosh\eta^') ~Q^m_{n-1 / 2}(\cosh\eta)~~~\eta^' < \eta \end{cases}\, , </math>

Wong (1973), p. 293, Eq. (2.53)
[see also: J. W. Bates (1997), p. 3685, Eq. (31)]
[see also: Cohl, Tohline, Rau, & Srivastava (2000), §6.2, Eq. (48)]

where, <math>~P^m_{n-1 / 2}, Q^m_{n-1 / 2}</math> are Associated Legendre Functions of the first and second kind with order <math>~n - \tfrac{1}{2}</math> and degree <math>~m</math> (toroidal harmonics), and <math>~\epsilon_m</math> is the Neumann factor, that is, <math>~\epsilon_0 = 1</math> and <math>~\epsilon_m = 2</math> for all <math>~m \ge 1</math>. This Green's function expression can indeed be found as eq. (10.3.81) on p. 1304 of [MF53], but it should be noted that the MF53 expression differs from Wong's in two respects (see footnote 2 on p. 370 of Cohl et al. (2000) for a proposed explanation): First, the factor, <math>~(-1)^m</math>, appears as <math>~(-i)^m</math> in MF53; and, second, in the term that is composed of a ratio of gamma functions, the denominator appears in MF53 as <math>~\Gamma(n - m + \tfrac{1}{2})</math>, whereas it should be <math>~\Gamma(n + m + \tfrac{1}{2})</math>, as presented here.

Rearranging Terms and Incorporating Special-Function Relations

Let's focus on the situation when <math>~\eta^' > \eta</math>, and begin rearranging or substituting terms.

<math>~\frac{1}{|~\vec{x} - {\vec{x}}^{~'} ~|} </math>

<math>~=</math>

<math>~ \frac{1}{\pi a} \biggl[ (\cosh\eta - \cos\theta)(\cosh \eta^' - \cos\theta^') \biggr]^{1 /2 } \sum\limits^\infty_{m=0} (-1)^m \epsilon_m \cos[m(\psi - \psi^')] </math>

 

 

<math>~ \times \sum\limits^\infty_{n=0} \epsilon_n \cos[n(\theta - \theta^')] ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} ~P^m_{n-1 / 2}(\cosh\eta) ~Q^m_{n-1 / 2}(\cosh\eta^') </math>

 

<math>~=</math>

<math>~ \frac{ [ (\cosh\eta - \cos\theta)(\cosh \eta^' - \cos\theta^')]^{1 /2 } }{\pi a \sqrt{\sinh\eta^'} \sqrt{\sinh\eta} } \sum\limits^\infty_{m=0} (-1)^m \epsilon_m \cos[m(\psi - \psi^')] </math>

 

 

<math>~ \times \sum\limits^\infty_{n=0} \epsilon_n \cos[n(\theta - \theta^')] \biggl\{ ~ \sqrt{ \frac{\pi}{2} }~\Gamma(n-m+\tfrac{1}{2}) \sqrt{\sinh\eta}~P^m_{n-1 / 2}(\cosh\eta) \biggl\}\biggr\{ ~\sqrt{ \frac{2}{\pi} }~\frac{\sqrt{\sinh\eta^'}}{\Gamma(n + m + \tfrac{1}{2})} Q^m_{n-1 / 2}(\cosh\eta^') \biggr\} </math>

The term contained within the first set of curly braces on the right-hand side of this expression can be replaced by the derived expression labeled in the Appendix, below, and simultaneously the term contained within the second set of curly braces can be replaced by the derived expression labeled in the same Appendix. After making these substitutions, we have,

<math>~\frac{1}{|~\vec{x} - {\vec{x}}^{~'} ~|} </math>

<math>~=</math>

<math>~ \frac{ [ (\cosh\eta - \cos\theta)(\cosh \eta^' - \cos\theta^')]^{1 /2 } }{\pi a \sqrt{\sinh\eta^'} \sqrt{\sinh\eta} } \sum\limits^\infty_{m=0} (-1)^m \epsilon_m \cos[m(\psi - \psi^')] </math>

 

 

<math>~ \times \sum\limits^\infty_{n=0} \epsilon_n \cos[n(\theta - \theta^')] \biggl\{ ~ (-1)^{-n}Q^n_{m-1 / 2}(\coth\eta) \biggl\}\biggr\{ ~(-1)^{-m} P^{-n}_{m-1 / 2}(\coth\eta^') \biggr\} </math>

 

<math>~=</math>

<math>~ \frac{ [ (\cosh\eta - \cos\theta)(\cosh \eta^' - \cos\theta^')]^{1 /2 } }{\pi a \sqrt{\sinh\eta^'} \sqrt{\sinh\eta} } \sum\limits^\infty_{m=0} \epsilon_m \cos[m(\psi - \psi^')] </math>

 

 

<math>~ \times \sum\limits^\infty_{n=0} (-1)^{n} \epsilon_n \cos[n(\theta - \theta^')] Q^n_{m-1 / 2}(\coth\eta) P^{-n}_{m-1 / 2}(\coth\eta^') \, , </math>

where, in writing this last expression we have acknowledged that, since <math>~n</math> is either zero or a positive integer, <math>~(-1)^{-n} = (-1)^n</math>. Next we draw upon the "Key Equation" relation,

LSU Key.png

<math>~ Q_\nu[t t^' - (t^2-1)^{1 / 2} (t^{'2} - 1)^{1 / 2} \cos\psi] </math>

<math>~=</math>

<math>~ Q_\nu(t) P_\nu(t^') + 2\sum_{n=1}^\infty (-1)^n Q^n_\nu(t) P^{-n}_\nu(t^') \cos(n\psi) </math>

A. Erdélyi (1953):  Volume I, §3.11, p. 169, eq. (4)

Valid for:    

<math>~t, t^'</math>  real

       

<math>~1 < t^' < t</math>

       

<math>~\nu \ne -1, -2, -3, </math> …

       

<math>~\psi</math>   real

which, after making the substitutions, <math>~\nu \rightarrow (m - \tfrac{1}{2})</math> and <math>~\psi \rightarrow (\theta - \theta^')</math>, and incorporating the Neumann factor, <math>~\epsilon_n</math>, becomes,

<math>~ Q_{m - \frac{1}{2} }\ [t t^' - (t^2-1)^{1 / 2} (t^{'2} - 1)^{1 / 2} \cos(\theta- \theta^') ] </math>

<math>~=</math>

<math>~ \sum_{n=0}^\infty (-1)^n \epsilon_n Q^n_{m - \frac{1}{2} }(t) P^{-n}_{m - \frac{1}{2} }(t^') \cos[(n(\theta- \theta^')] \, . </math>

Finally, after making the associations, <math>~t \rightarrow \coth\eta</math> and <math>~t^' \rightarrow \coth\eta^'</math>, this last expression allows us to rewrite Wong's (1973) Green's function in a significantly more compact form, namely,

<math>~\frac{1}{|~\vec{x} - {\vec{x}}^{~'} ~|} </math>

<math>~=</math>

<math>~ \frac{ [ (\cosh\eta - \cos\theta)(\cosh \eta^' - \cos\theta^')]^{1 /2 } }{\pi a \sqrt{\sinh\eta^'} \sqrt{\sinh\eta} } \sum\limits^\infty_{m=0} \epsilon_m \cos[m(\psi - \psi^')] Q_{m - \frac{1}{2}}(\Chi) \, , </math>

where the argument, <math>~\Chi</math>, of the toroidal function, <math>~Q_{m - \frac{1}{2}}</math>, is,

<math>~\Chi</math>

<math>~\equiv</math>

<math>~ t t^' - (t^2-1)^{1 / 2} (t^{'2} - 1)^{1 / 2} \cos(\theta- \theta^') </math>

 

<math>~=</math>

<math>~ \coth\eta \coth\eta^' - (\coth^2\eta-1)^{1 / 2} (\coth^2\eta'- 1)^{1 / 2} \cos(\theta- \theta^') </math>

 

<math>~=</math>

<math>~ \frac{\cosh\eta \cosh\eta^'}{\sinh\eta \sinh\eta^'} - \biggl[ \frac{1}{\sinh^2\eta} \biggr]^{1 / 2} \biggl[ \frac{1}{\sinh^2\eta'}\biggr]^{1 / 2} \cos(\theta- \theta^') </math>

 

<math>~=</math>

<math>~ \frac{\cosh\eta \cosh\eta^' - \cos(\theta- \theta^') }{\sinh\eta \sinh\eta^'} \, . </math>

As Presented in Cohl & Tohline (1999)

This last, compact Green's function expression — which we have derived, here, from Wong's (1973) published Green's function by drawing strategically upon a variety of special function relations — precisely matches the "compact cylindrical Green's function expression" that has been derived independently by Cohl & Tohline (1999) via a less tortuous route, namely,

<math>~ \frac{1}{|\vec{x} - \vec{x}^{~'}|}</math>

<math>~=</math>

<math>~ \frac{1}{\pi \sqrt{\varpi \varpi^'}} \sum_{m=0}^{\infty} \epsilon_m \cos[m(\psi - \psi^')] Q_{m- 1 / 2}(\Chi) </math>

 

Cohl & Tohline (1999), p. 88, Eq. (17)

 

<math>~=</math>

<math>~ \frac{1}{a\pi} \biggl[ \frac{(\cosh\eta^' - \cos\theta^')}{\sinh\eta^' } \frac{(\cosh\eta - \cos\theta)}{\sinh\eta } \biggr]^{1 / 2} \sum_{m=0}^{\infty} \epsilon_m \cos[m(\psi - \psi^')] Q_{m- 1 / 2}(\Chi) \, , </math>

where,

<math>~\Chi</math>

<math>~\equiv</math>

<math>~ \frac{(\varpi^')^2 + \varpi^2 + (z^' - z)^2}{2\varpi^' \varpi} </math>

<math>~=</math>

<math>~ \frac{\cosh\eta \cdot \cosh\eta^' - \cos(\theta^' - \theta) }{ \sinh\eta \cdot \sinh\eta^'} \, . </math>

   

Cohl & Tohline (1999), p. 88, Eq. (16)


Note from J. E. Tohline (June, 2018):  This is the first time that I have been able to formally demonstrate to myself that these two separately derived Green's function expressions are identical. See, however, the earlier identification of new addition theorems in association with equations (49) and (50) of Cohl et al. (2000).

Gravitational Potential

Quite generally, then, the gravitational potential can be obtained at any coordinate location, <math>~(\eta,\theta,\psi)</math> — both inside and outside of a specified mass distribution — by carrying out three nested spatial integrals over the product of:  <math>~\rho(\vec{x}^{~'})</math>, the differential volume element, and the Green's function as specified either by Wong (1973) or by Cohl & Tohline (1999).

In what follows we will make an effort to elucidate the pros and cons of adopting one Green's function expression over the other. In each case we begin by writing the expression for the potential in such a way that variations in the azimuthal coordinate, <math>~\psi</math>, are described by Fourier components, <math>~\Phi_m^{(1)}(\eta,\theta)</math> and <math>~\Phi_m^{(2)}(\eta,\theta)</math>, of the potential, such that,

<math>~\Phi(\vec{x}) = \tfrac{1}{2}\Phi_0^{(1)}(\eta,\theta) + \sum_{m=1}^\infty \cos (m\psi) \Phi_m^{(1)}(\eta,\theta) + \sum_{m=1}^\infty \sin (m\psi) \Phi_m^{(2)}(\eta,\theta) \, .</math>

Each Fourier component of the potential depends explicitly on the corresponding Fourier component of the density distribution, defined such that,

<math>~\rho(\vec{x}) = \tfrac{1}{2}\rho_0^{(1)}(\eta,\theta) + \sum_{m=1}^\infty \cos (m\psi) \rho_m^{(1)}(\eta,\theta) + \sum_{m=1}^\infty \sin (m\psi) \rho_m^{(2)}(\eta,\theta) \, .</math>

LaTeX mathematical expressions cut-and-pasted directly from
NIST's Digital Library of Mathematical Functions

As an additional primary point of reference, note that according to §1.8(i) of NIST's Digital Library of Mathematical Functions, a Fourier Series is defined as follows:

<math>~f(x)</math>

<math>~=</math>

<math>~\tfrac{1}{2}a_{0}+\sum^{\infty}_{n=1}\biggl[ a_{n}\cos\bigl(nx\bigr)+b_{n}\sin\bigl(nx\bigr) \biggr],</math>

<math>~a_n</math>

<math>~=</math>

<math>~\frac{1}{\pi}\int^{\pi}_{-\pi}f(x)\cos\bigl(nx\bigr)\mathrm{d}x,</math>

<math>~b_n</math>

<math>~=</math>

<math>~\frac{1}{\pi}\int^{\pi}_{-\pi}f(x)\sin\bigl(nx\bigr)\mathrm{d}x.</math>

Notice, therefore, that,

<math>~\rho_m^{(1)}(\eta,\theta)</math>

<math>~=</math>

<math>~\frac{1}{\pi}\int^{\pi}_{-\pi}\rho(\eta,\theta,\psi)\cos\bigl(m\psi\bigr)\mathrm{d}\psi,</math>

    and,    

<math>~\rho_m^{(2)}(\eta,\theta)</math>

<math>~=</math>

<math>~\frac{1}{\pi}\int^{\pi}_{-\pi}\rho(\eta,\theta,\psi)\sin\bigl(m\psi\bigr)\mathrm{d}\psi \, .</math>


The CT99 Expression for the Potential

In Three-Dimensional Generality

Employing the Green's function expression derived by Cohl & Tohline (1999), the gravitational potential for any three-dimensional matter distribution is,

<math>~ \Phi(\eta,\theta,\psi)</math>

<math>~=</math>

<math>~ -G \iiint \rho(\eta^',\theta^',\psi^') \biggl\{ \frac{1}{|\vec{x}^{~'} - \vec{x}|} \biggr\} \biggl[ \frac{a^3 \sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^3} \biggr] d\eta^'~ d\theta^'~ d\psi^' </math>

 

<math>~=</math>

<math>~ -\frac{Ga^2}{\pi} \int d\eta^' \int d\theta^' \int d\psi^' \iiint \rho(\eta^',\theta^',\psi^') \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^3} \biggr] </math>

 

 

<math>~ \times \biggl[ \frac{(\cosh\eta^' - \cos\theta^')}{\sinh\eta^' } \frac{(\cosh\eta - \cos\theta)}{\sinh\eta } \biggr]^{1 / 2} \sum_{m=0}^{\infty} \epsilon_m \cos[m(\psi - \psi^')] Q_{m- 1 / 2}(\Chi) </math>

 

<math>~=</math>

<math>~ -\frac{Ga^2}{\pi} \biggl[ \frac{(\cosh\eta - \cos\theta)}{\sinh\eta } \biggr]^{1 / 2} \sum_{m=0}^{\infty} \epsilon_m \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{m- 1 / 2}(\Chi) \int d\psi^' \rho(\eta^',\theta^',\psi^') </math>

 

 

<math>~ \times [\cos(m\psi)\cos(m\psi^') + \sin(m\psi)\sin(m\psi^') ] </math>

 

<math>~=</math>

<math>~ -\frac{Ga^2}{\pi} \biggl[ \frac{(\cosh\eta - \cos\theta)}{\sinh\eta } \biggr]^{1 / 2} \biggl\{ \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{- \frac{1}{2}}(\Chi) \int_{-\pi}^{\pi} d\psi^' \rho(\eta^',\theta^',\psi^') </math>

 

 

<math>~ + \sum_{m=1}^{\infty} 2\cos(m\psi) \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{m- 1 / 2}(\Chi) \int_{-\pi}^\pi d\psi^' \rho(\eta^',\theta^',\psi^') \cos(m\psi^') </math>

 

 

<math>~ + \sum_{m=1}^{\infty} 2\sin(m\psi) \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{m- 1 / 2}(\Chi) \int_{-\pi}^\pi d\psi^' \rho(\eta^',\theta^',\psi^') \sin(m\psi^') \biggr\} </math>

 

<math>~=</math>

<math>~ - Ga^2 \biggl[ \frac{(\cosh\eta - \cos\theta)}{\sinh\eta } \biggr]^{1 / 2} \biggl\{ \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{- \frac{1}{2}}(\Chi) \rho_0^{(1)}(\eta^',\theta^') </math>

 

 

<math>~ + \sum_{m=1}^{\infty} 2\cos(m\psi) \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{m- 1 / 2}(\Chi) \rho_m^{(1)}(\eta^',\theta^') </math>

 

 

<math>~ + \sum_{m=1}^{\infty} 2\sin(m\psi) \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{m- 1 / 2}(\Chi) \rho_m^{(2)}(\eta^',\theta^') \biggr\} \, . </math>

We conclude, therefore, that each one of the Fourier components of the gravitational potential is given by the expression,

<math>~\Phi_m^{(1),(2)}(\eta,\theta)</math>

<math>~=</math>

<math>~ - 2Ga^2 \biggl[ \frac{(\cosh\eta - \cos\theta)}{\sinh\eta } \biggr]^{1 / 2} \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{m- 1 / 2}(\Chi) \rho_m^{(1),(2)}(\eta^',\theta^') \, , </math>

Cohl & Tohline (1999), p. 88, Eq. (20)

where, as above,

<math>~\Chi</math>

<math>~\equiv</math>

<math>~ \frac{\cosh\eta \cdot \cosh\eta^' - \cos(\theta^' - \theta) }{ \sinh\eta \cdot \sinh\eta^'} \, . </math>

For Axisymmetric Systems

For axisymmetric systems, the density distribution has no dependence on the azimuthal coordinate, <math>~\psi</math>. Hence, for all <math>~m > 0</math>, the Fourier components of the density, <math>~\rho_m^{(1),(2)}</math>, are zero. The only nonzero component is, <math>~\rho_0^{(1)}(\eta,\theta) = 2\rho(\eta,\theta)</math>. For axisymmetric systems, then, the gravitational potential is,

<math>~\Phi(\eta,\theta)</math>

<math>~=</math>

<math>~\tfrac{1}{2}\Phi_0^{(1)}(\eta,\theta)</math>

 

<math>~=</math>

<math>~ - 2Ga^2 \biggl[ \frac{(\cosh\eta - \cos\theta)}{\sinh\eta } \biggr]^{1 / 2} \int d\eta^' \int d\theta^' \biggl[ \frac{\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^5} \biggr]^{1 / 2} Q_{- 1 / 2}(\Chi) \rho(\eta^',\theta^') \, . </math>

Cohl & Tohline (1999), p. 88, Eqs. (31) & (32a)

Wong's Expression for the Potential

Fully Three-Dimensional Case

Employing Wong's (1973) Green's function expression, the gravitational potential for any three-dimensional matter distribution is,

<math>~ \Phi(\vec{x})</math>

<math>~=</math>

<math>~ -G \iiint \rho(\eta^',\theta^',\psi^') \biggl\{ \frac{1}{|\vec{x}^{~'} - \vec{x}|} \biggr\} \biggl[ \frac{a^3 \sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^3} \biggr] d\eta^'~ d\theta^'~ d\psi^' </math>

 

<math>~=</math>

<math>~ - \frac{a^2G}{\pi} \int d\eta^' \int d\theta^' \int d\psi^' \biggl[ \frac{\rho(\eta^',\theta^',\psi^') ~\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^3} \biggr] \biggl[ (\cosh\eta - \cos\theta)(\cosh \eta^' - \cos\theta^') \biggr]^{1 /2 } \sum\limits^\infty_{n=0} \sum\limits^\infty_{m=0}(-1)^m \epsilon_m \epsilon_n ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} </math>

 

 

<math>~ \times \cos[m(\psi - \psi^')]\cos[n(\theta - \theta^')] ~P^m_{n-1 / 2}(\cosh\eta_<) ~Q^m_{n-1 / 2}(\cosh\eta_>) </math>

 

<math>~=</math>

<math>~ - \frac{a^2G}{\pi} (\cosh\eta - \cos\theta)^{1 / 2} \sum\limits^\infty_{n=0} \epsilon_n \sum\limits^\infty_{m=0}(-1)^m \epsilon_m ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} \int d\eta^' ~P^m_{n-1 / 2}(\cosh\eta_<) ~Q^m_{n-1 / 2}(\cosh\eta_>) </math>

 

 

<math>~ \times~ \int d\theta^' \biggl[ \frac{ ~\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr]\cos[n(\theta - \theta^')] \int d\psi^' \rho(\eta^',\theta^',\psi^') [\cos(m\psi)\cos(m\psi^') + \sin(m\psi) \sin(m\psi^')] </math>

 

<math>~=</math>

<math>~ - \frac{a^2G}{\pi} (\cosh\eta - \cos\theta)^{1 / 2} \sum\limits^\infty_{n=0} \epsilon_n \biggl\{ \int d\eta^' ~P_{n-1 / 2}(\cosh\eta_<) ~Q_{n-1 / 2}(\cosh\eta_>) \int d\theta^' \biggl[ \frac{ ~\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr]\cos[n(\theta - \theta^')] \int_{-\pi}^\pi d\psi^' \rho(\eta^',\theta^',\psi^') </math>

 

 

<math>~ +~ \sum\limits^\infty_{m=1} 2\cos(m\psi)(-1)^m ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} \int d\eta^' ~P^m_{n-1 / 2}(\cosh\eta_<) ~Q^m_{n-1 / 2}(\cosh\eta_>) \int d\theta^' \biggl[ \frac{ ~\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr]\cos[n(\theta - \theta^')] \int_{-\pi}^\pi d\psi^' \rho(\eta^',\theta^',\psi^') \cos(m\psi^') </math>

 

 

<math>~ +~ \sum\limits^\infty_{m=1} 2 \sin(m\psi)(-1)^m ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} \int d\eta^' ~P^m_{n-1 / 2}(\cosh\eta_<) ~Q^m_{n-1 / 2}(\cosh\eta_>) \int d\theta^' \biggl[ \frac{ ~\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr]\cos[n(\theta - \theta^')] \int_{-\pi}^\pi d\psi^' \rho(\eta^',\theta^',\psi^') \sin(m\psi^') \biggr\} </math>

 

<math>~=</math>

<math>~ - a^2G (\cosh\eta - \cos\theta)^{1 / 2} \sum\limits^\infty_{n=0} \epsilon_n \biggl\{ \int d\eta^' ~P_{n-1 / 2}(\cosh\eta_<) ~Q_{n-1 / 2}(\cosh\eta_>) \int d\theta^' \biggl[ \frac{ ~\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr]\cos[n(\theta - \theta^')] \rho_0^{(1)}(\eta^',\theta^') </math>

 

 

<math>~ +~ \sum\limits^\infty_{m=1} 2\cos(m\psi)(-1)^m ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} \int d\eta^' ~P^m_{n-1 / 2}(\cosh\eta_<) ~Q^m_{n-1 / 2}(\cosh\eta_>) \int d\theta^' \biggl[ \frac{ ~\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr]\cos[n(\theta - \theta^')] \rho_m^{(1)}(\eta^',\theta^') </math>

 

 

<math>~ +~ \sum\limits^\infty_{m=1} 2 \sin(m\psi)(-1)^m ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} \int d\eta^' ~P^m_{n-1 / 2}(\cosh\eta_<) ~Q^m_{n-1 / 2}(\cosh\eta_>) \int d\theta^' \biggl[ \frac{ ~\sinh\eta^'}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr]\cos[n(\theta - \theta^')] \rho_m^{(2)} (\eta^',\theta^') \biggr\} \, . </math>

We conclude, therefore, that each one of the Fourier components of the gravitational potential is given by the expression,

<math>~\Phi_m^{(1),(2)} (\eta,\theta)</math>

<math>~=</math>

<math>~ - 2Ga^2 (\cosh\eta - \cos\theta)^{1 / 2} \sum\limits^\infty_{n=0} \epsilon_n (-1)^m ~\frac{\Gamma(n-m+\tfrac{1}{2})}{\Gamma(n + m + \tfrac{1}{2})} </math>

 

 

<math>~\times \int d\eta^' ~\sinh\eta^' ~ P^m_{n-1 / 2}(\cosh\eta_<) ~ Q^m_{n-1 / 2}(\cosh\eta_>) \int d\theta^' \biggl\{ \frac{ \cos[n(\theta - \theta^')]}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr\} \rho_m^{(1),(2)}(\eta^',\theta^') \, . </math>

Axisymmetric Systems

For axisymmetric systems, the density distribution has no dependence on the azimuthal coordinate, <math>~\psi</math>. Hence, for all <math>~m > 0</math>, the Fourier components of the density, <math>~\rho_m^{(1),(2)}</math>, are zero. The only nonzero component is, <math>~\rho_0^{(1)}(\eta,\theta) = 2\rho(\eta,\theta)</math>. For axisymmetric systems, then, the gravitational potential is,

<math>~\Phi(\eta,\theta)</math>

<math>~=</math>

<math>~\tfrac{1}{2}\Phi_0^{(1)}(\eta,\theta)</math>

 

<math>~=</math>

<math>~ - 2Ga^2 (\cosh\eta - \cos\theta)^{1 / 2} \sum\limits^\infty_{n=0} \epsilon_n \int d\eta^' ~\sinh\eta^'~P^0_{n-1 / 2}(\cosh\eta_<) ~Q^0_{n-1 / 2}(\cosh\eta_>) \int d\theta^' \biggl\{ \frac{ ~\cos[n(\theta - \theta^')]}{(\cosh\eta^' - \cos\theta^')^{5/2}} \biggr\} \rho(\eta^',\theta^') \, . </math>

Wong (1973), p. 293, Eq. (2.55)

Uniform-Density Torus

In an accompanying discussion, we build upon the above technical foundation and detail how Wong (1973) was able to complete both integrals to derive an analytic expression for the potential (inside as well as outside) of axisymmetric, uniform-density tori having an arbitrarily specified ratio of the major to minor (cross-sectional) radii, <math>~R/d</math>. This is an outstanding accomplishment that has received little attention in the astrophysics literature and, therefore, has heretofore been underappreciated.

Appendix: Selected Toroidal Function Relationships

Here, we draw from the set of toroidal function relationships that have been identified as "Key Equations" in our accompanying Equations appendix. Two related appendices — numbered A.3 and A.4 — may be found in an accompanying discussion.

A.1

Beginning with the identified "Key Equation",

LSU Key.png

<math>~Q_{n-1 / 2}^m (\lambda)</math>

<math>~=</math>

<math>~(-1)^n \frac{\pi^{3/2}}{\sqrt{2}~ \Gamma(n-m+1 / 2)} (x^2-1)^{1 / 4} P_{m-1 / 2}^n(x) \, , </math>

Gil, Segura, & Temme (2000):  eq. (8)

where:    

<math>~\lambda \equiv x/\sqrt{x^2-1}</math>

we'll identify <math>~x</math> with <math>~\cosh\eta</math> — in which case we have <math>~\lambda = \coth\eta</math> — and switch the index notations, <math>~n \leftrightarrow m</math>. This gives,

<math>~Q_{m-1 / 2}^n (\coth\eta)</math>

<math>~=</math>

<math>~(-1)^m \frac{\pi^{3/2}}{\sqrt{2} ~\Gamma(m-n+\frac{1}{2})} (\sinh\eta)^{1 / 2} P_{n-1 / 2}^m(\cosh\eta) \, . </math>

Drawing upon the Euler reflection formula for gamma functions, namely,

LSU Key.png

<math>~ \Gamma(z) ~\Gamma(1-z) </math>

<math>~=</math>

<math>~ \frac{\pi}{\sin(\pi z)} </math>

<math>~\biggl|</math>

for example, if
<math>~z \rightarrow (m-n + \tfrac{1}{2})</math>

<math>~\Rightarrow ~~~\Gamma(m-n+\tfrac{1}{2})~\Gamma(n-m+\tfrac{1}{2})</math>

<math>~=</math>

<math>~\pi \biggl\{\sin\biggl[ \frac{\pi}{2} + \pi(m-n) \biggr] \biggr\}^{-1}</math>

 

<math>~=</math>

<math>~\pi (-1)^{m-n} </math>

DLMF §5.5(ii)

<math>~\biggl|</math>
Valid for:

   <math>~z \ne0, \pm 1, \pm 2, </math> …

<math>~\biggl|</math>

where it is understood that <math>~m</math> and <math>~n</math> are each either zero or a positive integer, this toroidal-function relation becomes,

<math>~Q_{m-1 / 2}^n (\coth\eta)</math>

<math>~=</math>

<math>~(-1)^m~ \frac{\pi^{3/2}}{\sqrt{2} } \biggl[ \frac{ \Gamma(n - m +\frac{1}{2}) }{ \pi (-1)^{m-n} } \biggr] (\sinh\eta)^{1 / 2} P_{n-1 / 2}^m(\cosh\eta) </math>

 

 

<math>~=</math>

<math>~ (-1)^n \sqrt{ \frac{\pi}{2} } ~\Gamma(n - m + \tfrac{1}{2} )(\sinh\eta)^{1 / 2} P_{n-1 / 2}^m(\cosh\eta) \, . </math>


A.2

Again, beginning with the identified "Key Equation",

LSU Key.png

<math>~Q_{n-1 / 2}^m (\lambda)</math>

<math>~=</math>

<math>~(-1)^n \frac{\pi^{3/2}}{\sqrt{2}~ \Gamma(n-m+1 / 2)} (x^2-1)^{1 / 4} P_{m-1 / 2}^n(x) \, , </math>

Gil, Segura, & Temme (2000):  eq. (8)

where:    

<math>~\lambda \equiv x/\sqrt{x^2-1}</math>

this time, without switching index notations, we'll identify <math>~x</math> with <math>~\coth\eta</math> — in which case we have <math>~\lambda = \cosh\eta</math>. This gives,

<math>~Q_{n-1 / 2}^m (\cosh\eta)</math>

<math>~=</math>

<math>~(-1)^n \frac{\pi^{3/2}}{\sqrt{2} ~\Gamma(n-m+\frac{1}{2})} \biggl( \frac{1}{\sinh\eta} \biggr)^{1 / 2} P_{m-1 / 2}^n(\coth\eta) \, . </math>

Drawing upon the same Euler reflection formula for gamma functions, as quoted above, this toroidal function relation can be rewritten as,

<math>~Q_{n-1 / 2}^m (\cosh\eta)</math>

<math>~=</math>

<math>~(-1)^n \frac{\pi^{3/2}}{\sqrt{2} } \biggl[ \frac{\Gamma(m-n+\frac{1}{2})}{\pi (-1)^{m-n}} \biggr] \biggl( \frac{1}{\sinh\eta} \biggr)^{1 / 2} P_{m-1 / 2}^n(\coth\eta) </math>

 

<math>~=</math>

<math>~(-1)^{-m}~ \sqrt{\frac{\pi}{2}} \biggl[ \frac{\Gamma(m-n+\frac{1}{2})}{\sqrt{\sinh\eta}} \biggr] P_{m-1 / 2}^n(\coth\eta) \, . </math>

Finally, calling upon the "Key Equation" relation,

LSU Key.png

<math>~ P_\nu^n(z) </math>

<math>~=</math>

<math>~ \frac{\Gamma(\nu + n + 1)}{\Gamma(\nu - n + 1)} P_\nu^{-n}(z) </math>

A. Erdélyi (1953):  Volume I, §3.3.1, p. 140, eq. (7)

making the index notation substitution, <math>~\nu \rightarrow (m-\tfrac{1}{2})</math>, and associating <math>~z</math> with <math>~ \coth\eta</math> gives,

<math>~P^n_{m-\frac{1}{2}}(\coth\eta)</math>

<math>~=</math>

<math>~\biggl[ \frac{\Gamma(m+n+\frac{1}{2})}{\Gamma(m-n+\frac{1}{2})} \biggr]P^{-n}_{m-\frac{1}{2}}(\coth\eta) \, .</math>

As a result, we can write,

<math>~Q_{n-1 / 2}^m (\cosh\eta)</math>

<math>~=</math>

<math>~(-1)^{-m}~ \sqrt{\frac{\pi}{2}} \biggl[ \frac{\Gamma(m+n+\frac{1}{2})}{\sqrt{\sinh\eta}} \biggr] P_{m-1 / 2}^{-n}(\coth\eta) </math>

 

<math>~\Rightarrow ~~~ P_{m-1 / 2}^{-n}(\coth\eta) </math>

<math>~=</math>

<math>~(-1)^m~\sqrt{\frac{2}{\pi}} \biggl[ \frac{\sqrt{\sinh\eta}}{\Gamma(m+n+\frac{1}{2})} \biggr] Q_{n-1 / 2}^m (\cosh\eta) \, . </math>


A.3

Here, our objective is to evaluate the definite integral,

<math>~\int_{-\pi}^{\pi} \frac{\cos[n(\theta - \theta^')] d\theta}{(\cosh\eta - \cos\theta)^{5 / 2}} </math>

<math>~=</math>

<math>~ \cos(n\theta^') \int_{-\pi}^{\pi} \frac{ \cos(n\theta) ~ d\theta}{(\cosh\eta - \cos\theta)^{5 / 2}} + \sin(n\theta^') \cancelto{0}{ \int_{-\pi}^{\pi} \frac{ \sin(n\theta) d\theta}{(\cosh\eta - \cos\theta)^{5 / 2}} } </math>

 

<math>~=</math>

<math>~ 2 \cos(n\theta^') \int_{0}^{\pi} \frac{ \cos(n\theta)~ d\theta}{(\cosh\eta - \cos\theta)^{5 / 2}} \, . </math>

Notice that, since the limits of the integration are <math>~-\pi</math> to <math>~+\pi</math>:   The second integral on the right-hand-side goes to zero because the numerator of its integrand — i.e., <math>~\sin(n\theta)</math> — is an odd function; and, with regard to the first integral on the right-hand-side, the lower integration limit can be set to zero and the result doubled because the numerator of its integrand — i.e., <math>~\cos(n\theta)</math> — is an even function.

Drawing from Volume I of A. Erdélyi's (1953) Higher Transcendental Functions, we find the following "Key Equation":

LSU Key.png

<math>~Q_\nu^\mu(z)</math>

<math>~=</math>

<math>~ e^{i \mu \pi} ~ (2\pi)^{-\frac{1}{2}} (z^2-1)^{\mu/2} ~\Gamma(\mu + \tfrac{1}{2})~\biggl\{ \int_0^\pi (z - \cos t)^{-\mu - \frac{1}{2}} \cos[(\nu + \tfrac{1}{2})t] ~dt -\cos(\nu\pi) \int_0^\infty (z + \cosh t)^{-\mu - \frac{1}{2}} e^{-(\nu + \frac{1}{2})t} ~dt \biggr\} </math>

A. Erdélyi (1953):  Volume I, §3.7, p. 156, eq. (10)

Valid for:    

<math>~\mathrm{Re} ~\nu > -\tfrac{1}{2}</math> 

    and    

<math>~\mathrm{Re} (\nu + \mu + 1) > 0 \, .</math>

Next we adopt the associations, <math>~z \rightarrow \cosh\eta</math>, <math>~t \rightarrow \theta</math>, <math>~\mu \rightarrow 2</math>, and, <math>~\nu \rightarrow n - \tfrac{1}{2}</math>, where <math>~n</math> is zero or a positive integer. In this case we have,

<math>~Q_{n - \frac{1}{2}}^2 (\cosh\eta)</math>

<math>~=</math>

<math>~ (2\pi)^{-\frac{1}{2}} (\cosh^2\eta-1) ~\Gamma(\tfrac{5}{2})~\biggl\{ \int_0^\pi (\cosh\eta - \cos \theta)^{-\frac{5}{2}} \cos(n\theta) ~d\theta - \cancelto{0}{\cos[(n-\tfrac{1}{2})\pi] }~~\int_0^\infty (\cosh\eta + \cosh \theta)^{- \frac{5}{2}} e^{-n\theta} ~d\theta \biggr\} \, , </math>

where the prefactor of the second term — that is, <math>~\cos[(n-\tfrac{1}{2})\pi] </math> — goes to zero for all allowable values of the integer, <math>~n</math>. Hence, we conclude that,

<math>~2\cos(n\theta^') \int_0^\pi \frac{ \cos(n\theta)~d\theta }{ (\cosh\eta - \cos \theta)^{\frac{5}{2}} } </math>

<math>~=</math>

<math>~\frac{ 2(2\pi)^{\frac{1}{2}} Q_{n - \frac{1}{2}}^2 (\cosh\eta) \cos(n\theta^')}{ (\cosh^2\eta-1) ~\Gamma(\tfrac{5}{2})~ } </math>

 

<math>~=</math>

<math>~\biggl[ \frac{ 2^3 \sqrt{2} }{ 3 } \biggr] \frac{ Q_{n - \frac{1}{2}}^2(\cosh\eta) \cos(n\theta^')}{ \sinh^2\eta } \, . </math>

where we have set,

<math>~ \Gamma(\tfrac{5}{2}) = \Gamma(\tfrac{1}{2} + 2) = \frac{ \sqrt{\pi} \cdot 4! }{4^2 \cdot 2!} = \frac{\sqrt{\pi} \cdot 2^3\cdot 3}{ 2^5 } = \frac{3 \sqrt{\pi}}{2^2} \, . </math>

A.4

Beginning with the identified "Key Equation",

LSU Key.png

<math>~ \int_a^b\biggl[(\nu - \sigma)(\nu + \sigma + 1) + (\rho^2 - \mu^2)(1 - z^2)^{-1} \biggr] w_\nu^\mu ~w_\sigma^\rho ~dz </math>

<math>~=</math>

<math>~ \biggl[ z(\nu-\sigma) w_\nu^\mu ~w_\sigma^\rho + (\sigma+\rho) w_\nu^\mu ~ w_{\sigma-1}^\rho - (\nu + \mu) w_{\nu - 1}^\mu ~w_\sigma^\rho \biggr]_a^b </math>

A. Erdélyi (1953):  Volume I, §3.12, p. 169, eq. (1)

where, <math>~w_\nu^\mu(z)</math> and <math>~w_\sigma^\rho(z)</math> denote any solutions of Legendre's differential equation

we will adopt the associations:   <math>~z \rightarrow t</math>, <math>~\mu \rightarrow 2</math>, <math>~\nu \rightarrow (n - \tfrac{1}{2})</math>, <math>~\rho \rightarrow 0</math>, and <math>~\sigma \rightarrow ( n - \tfrac{1}{2})</math>. As a result, Erdélyi's (1953) expression becomes,

<math>~ \int_a^b\biggl[ -4(1 - t^2)^{-1} \biggr] Q_{n - \frac{1}{2}}^2(t) ~X_{n - \frac{1}{2}}(t) ~dt </math>

<math>~=</math>

<math>~ \biggl[ (n - \tfrac{1}{2} ) Q_{n - \frac{1}{2}}^2(t) ~ X_{n - \frac{3}{2}}(t) - (n + \tfrac{3}{2}) Q_{n - \frac{3}{2}}^2(t) ~X_{n - \frac{1}{2}}(t) \biggr]_a^b \, . </math>

Drawing upon the recurrence "Key Equation,"

LSU Key.png

<math>~(\nu - \mu + 1)P^\mu_{\nu + 1} (z)</math>

<math>~=</math>

<math>~ (2\nu + 1)z P_\nu^\mu(z) - (\nu + \mu)P^\mu_{\nu-1}(z) </math>

Abramowitz & Stegun (1995), p. 334, eq. (8.5.3)

NOTE: <math>~Q_\nu^\mu</math>, as well as <math>~P_\nu^\mu</math>, satisfies this same recurrence relation.

which means, after making the associations, <math>~z \rightarrow t</math>, <math>~\mu \rightarrow 0</math> and <math>~\nu \rightarrow (n-\tfrac{1}{2})</math>, that,

<math>~(n+\tfrac{1}{2})X_{n+\frac{1}{2}}(t)</math>

<math>~=</math>

<math>~2n t X_{n-\frac{1}{2}}(t) - (n-\tfrac{1}{2})X_{n - \frac{3}{2}}(t)</math>

<math>~\Rightarrow ~~~(n-\tfrac{1}{2})X_{n - \frac{3}{2}}(t) </math>

<math>~=</math>

<math>~2n t X_{n-\frac{1}{2}}(t) - (n+\tfrac{1}{2})X_{n+\frac{1}{2}}(t)</math>

the integral can be rewritten as,

<math>~ \int_a^b\biggl[ \frac{Q_{n - \frac{1}{2}}^2(t) ~X_{n - \frac{1}{2}}(t) }{(t^2-1)}\biggr]~dt </math>

<math>~=</math>

<math>~ \frac{1}{4} \biggl\{ \biggl[ 2n t X_{n-\frac{1}{2}}(t) - (n+\tfrac{1}{2})X_{n+\frac{1}{2}}(t) \biggr] Q_{n - \frac{1}{2}}^2(t) - (n + \tfrac{3}{2}) Q_{n - \frac{3}{2}}^2(t) ~X_{n - \frac{1}{2}}(t) \biggr\}_a^b </math>

 

<math>~=</math>

<math>~ \frac{1}{4} \biggl\{ \biggl[ 2n t Q_{n - \frac{1}{2}}^2(t) - (n + \tfrac{3}{2}) Q_{n - \frac{3}{2}}^2(t) \biggr] X_{n - \frac{1}{2}}(t) - (n+\tfrac{1}{2})X_{n+\frac{1}{2}}(t) Q_{n - \frac{1}{2}}^2(t) \biggr\}_a^b \, . </math>

Returning to the same recurrence "Key Equation," but this time adopting the associations, <math>~z \rightarrow t</math>, <math>~\mu \rightarrow 2</math> and <math>~\nu \rightarrow (n-\tfrac{1}{2})</math>, we can write,

<math>~(n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(t)</math>

<math>~=</math>

<math>~ 2n t Q^2_{n - \frac{1}{2}}(t) - (n + \tfrac{3}{2}) Q^2_{n - \frac{3}{2}} (t) \, , </math>

in which case the integral becomes,

<math>~ \int_a^b\biggl[ \frac{Q_{n - \frac{1}{2}}^2(t) ~X_{n - \frac{1}{2}}(t) }{(t^2-1)}\biggr]~dt </math>

<math>~=</math>

<math>~ \frac{1}{4} \biggl\{ (n - \tfrac{3}{2})Q^2_{n + \frac{1}{2}}(t) ~ X_{n - \frac{1}{2}}(t) - (n+\tfrac{1}{2})X_{n+\frac{1}{2}}(t) Q_{n - \frac{1}{2}}^2(t) \biggr\}_a^b \, . </math>

See Also

  • P. Lucht (2016), The Charged Bowl in Toroidal Coordinates — Note from Tohline: On 3 July 2018 I stumbled on this article by Phil Lucht, who lists his affiliation as Rimrock Digital Technology (rimrock at emission.com), Salt Lake City, Utah. As I have done over the past approximately half a year, Lucht appears to have spent quite a bit of time investigating how toroidal coordinates might be used to solve a few specific potential problems. He draws on many of the same, rich technical resource publications as I have done and, at one point, explicitly expresses amazement at the extensive amount of useful material that can be found in [MF53]. Anyone digging into this topic would be well-advised to read Lucht's Overview and Summary — especially including the subsection titled, Legendre Functions — and to recognize that his document contains a large number of technically detailed appendices.
     
    To provide one point of comparison with [MF53], Lucht derived an analytic expression for the potential outside of a torus (with toroidal-coordinate radius, <math>~\eta_0</math>) whose surface is held at uniform potential, <math>~\Phi_0</math>. This is in contrast to Wong's (1973) derivation — which we have verified, above — of the potential outside (as well as inside) of a torus having uniform charge/mass. For his particular example problem, Lucht obtains,

    <math>~\Phi(\eta,\theta)</math>

    <math>~=</math>

    <math>~ \Phi_0 \frac{\sqrt{2}}{\pi} \sqrt{\cosh\eta - \cos\theta} \sum_{n=0}^\infty \epsilon_n P_{n-\frac{1}{2}}(\cosh\eta) \Biggl[ \frac{Q_{n-\frac{1}{2}}(\cosh\eta_0)}{P_{n-\frac{1}{2}}(\cosh\eta_0)} \Biggr] \cos(n\theta) \, , </math>

    Lucht (2016), p. 68, Eq. (10.1.11)

    then he points out that the associated expression for the potential, which appears as equation (10.3.80) on p. 1304 of [MF53], is missing the Neumann factor, <math>~\epsilon_n</math>.


Whitworth's (1981) Isothermal Free-Energy Surface

© 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