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===Potential of a Thin Hoop=== In §IIb of his [http://adsabs.harvard.edu/abs/1964ApJ...140.1067O Paper II], Ostriker (1964) derives an expression for the gravitational potential of a torus in the ''Thin Ring'' approximation, beginning specifically with the [[SR/PoissonOrigin#Step_1|integral form of the Poisson equation]] that is widely referred to in the astrophysics community as an expression for the, <div align="center" id="GravitationalPotential"> <table border="0" cellpadding="5" align="center"> <tr> <td align="center" colspan="3"> <font color="#770000">'''Scalar Gravitational Potential'''</font> </td> </tr> <tr> <td align="right"> <math>~ \Phi(\vec{x})</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~ -G \iiint \frac{\rho(\vec{x}^{~'})}{|\vec{x}^{~'} - \vec{x}|} d^3x^' \, .</math> </td> </tr> <tr> <td align="center" colspan="3"> [<b>[[Appendix/References#BT87|<font color="red">BT87</font>]]</b>], p. 31, Eq. (2-3)<br /> [<b>[[Appendix/References#EFE|<font color="red">EFE</font>]]</b>], §10, p. 17, Eq. (11)<br /> [<b>[[Appendix/References#T78|<font color="red">T78</font>]]</b>], §4.2, p. 77, Eq. (12) </td> </tr> </table> </div> (Note: Consistent with the usage favored by his doctoral dissertation advisor in [<b>[[Appendix/References#EFE|<font color="red">EFE</font>]]</b>], throughout his collection of 1964 papers Ostriker adopts a ''different sign convention'' as well as a different variable name to represent the gravitational potential.) Employing [[#Coordinate_System|Ostriker's adopted coordinate system]], and recognizing that, <font color="darkgreen">"the distance between the point of integration <math>~(0,0,\theta^')</math> and the point of observation <math>~(r,\phi,0)</math>"</font> is, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~|\vec{x}^{~'} - \vec{x}|</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~[4R(R+r\cos\phi) \sin^2(\tfrac{1}{2}\theta^') + r^2]^{1 / 2} \, ,</math> </td> </tr> <tr> <td align="center" colspan="3"> Ostriker's (1964) [http://adsabs.harvard.edu/abs/1964ApJ...140.1067O Paper II], p. 1070, Eq. (21) </td> </tr> </table> this expression for the gravitational potential becomes, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \Phi(r,\phi)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left" colspan="2"> <math>~ -G \int \int \rho(r^',\phi^') r^' (R+r^'\cos\phi^') dr^' d\phi^' \int \frac{d\theta^'}{[4R(R+r\cos\phi) \sin^2(\tfrac{1}{2}\theta^') + r^2]^{1 / 2} } </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ -G (2\sigma R) \int_0^\pi \frac{d\theta^'}{[4R(R+r\cos\phi) \sin^2(\tfrac{1}{2}\theta^') + r^2]^{1 / 2} } </math> </td> <td align="right" rowspan="4">[[File:WolframAlphaResult.png|300px|WolframAlpha result]]</td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ -\frac{4G \sigma R}{r} \int_0^\pi \frac{\tfrac{1}{2}d\theta^'}{[1 +n^2\sin^2(\tfrac{1}{2}\theta^')]^{1 / 2} } </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ -\frac{4G \sigma R}{r} \biggl[ \frac{K(k)}{\sqrt{n^2+1}} \biggr] \, ,</math> </td> </tr> <tr> <td align="center" colspan="3"> Ostriker's (1964) [http://adsabs.harvard.edu/abs/1964ApJ...140.1067O Paper II], p. 1070, Eq. (22) </td> </tr> </table> where, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~n^2 \equiv \frac{4R(R+r\cos\phi)}{r^2}</math> </td> <td align="center"> and </td> <td align="left"> <math>~k \equiv \biggl[ \frac{n^2}{n^2+1} \biggr]^{1 / 2} \, .</math> </td> </tr> <tr> <td align="center" colspan="3"> Ostriker's (1964) [http://adsabs.harvard.edu/abs/1964ApJ...140.1067O Paper II], p. 1070, Eq. (23) </td> </tr> </table> <table border="1" cellpadding="10" align="center" width="85%"><tr><td align="left"> Mapping back to cylindrical coordinates, for the moment, we recognize that, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~r^2</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(\varpi - R)^2 + z^2</math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow ~~~ n^2</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{4R\varpi}{(\varpi - R)^2 + z^2}</math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow ~~~ n^2 + 1</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{4R\varpi + (\varpi - R)^2 + z^2}{(\varpi - R)^2 + z^2} = \frac{(\varpi + R)^2 + z^2}{(\varpi - R)^2 + z^2} \, .</math> </td> </tr> </table> Acknowledging as well that the mass of Ostriker's "thin hoop" is, <math>~M = 2\pi \sigma R</math>, his expression for the potential becomes, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\Phi(\varpi,z)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ -\frac{2G M}{\pi} \biggl[ \frac{K(k)}{\sqrt{(\varpi + R)^2 + z^2}} \biggr] \, ,</math> </td> </tr> </table> where, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~k</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl[ \frac{4R\varpi}{(\varpi + R)^2 + z^2} \biggr]^{1 / 2} \, .</math> </td> </tr> </table> After adopting the variable association, <math>~R \leftrightarrow a</math>, it is clear that Ostriker's derived expression is identical to the Key Equation that we have [[Apps/DysonWongTori#Thin_Ring_Approximation|identified elsewhere]] as providing the, <table border="0" cellpadding="5" align="center"> <tr> <td align="center" colspan="1"><font color="#770000">'''Gravitational Potential in the Thin Ring (TR) Approximation'''</font></td> <td align="center" colspan="1" rowspan="2">[[File:FlatColorContoursCropped.png|220px|Contours for Thin Ring Approximation]]</td> </tr> <tr> <td align="center"> {{ Math/EQ TRApproximation }} </td> </tr> </table> </td></tr></table>
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