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===Our Approach=== When the stated objective is to construct steady-state equilibrium models of rotationally flattened, axisymmetric configurations, the [[AxisymmetricConfigurations/Equilibria#Axisymmetric_Configurations_.28Steady-State_Structures.29|accompanying introductory chapter]] shows how the overarching set of [[PGE#Principal_Governing_Equations|principal governing equations]] can be reduced in form to the following set of three coupled PDEs (expressed either in terms of cylindrical or spherical coordinates): <table align="center" border="1" cellpadding="10"> <tr><th align="center" colspan="2"><font size="+0">Table 1: Simplified Set of Three Coupled PDEs</font></th></tr> <tr> <th align="center" width="50%">Cylindrical Coordinate Base</th> <th align="center">Spherical Coordinate Base</th> </tr> <tr> <td align="center"> <font color="#770000">'''Poisson Equation'''</font><br /> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \frac{1}{\varpi} \frac{\partial }{\partial\varpi} \biggl[ \varpi \frac{\partial \Phi}{\partial\varpi} \biggr] + \frac{\partial^2 \Phi}{\partial z^2} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~4\pi G \rho </math> </td> </tr> </table> The Two Relevant Components of the<br /> <font color="#770000">'''Euler Equation'''</font> <br /> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"><math>~{\hat{e}}_\varpi</math>: </td> <td align="right"> <math>~0</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[ \frac{1}{\rho}\frac{\partial P}{\partial\varpi} + \frac{\partial \Phi}{\partial\varpi}\biggr] - \frac{j^2}{\varpi^3} </math> </td> </tr> <tr> <td align="right"><math>~{\hat{e}}_z</math>: </td> <td align="right"> <math>~0</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[ \frac{1}{\rho}\frac{\partial P}{\partial z} + \frac{\partial \Phi}{\partial z} \biggr] </math> </td> </tr> </table> </td> <td align="center"> <font color="#770000">'''Poisson Equation'''</font><br /> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \frac{1}{r^2} \frac{\partial }{\partial r} \biggl[ r^2 \frac{\partial \Phi }{\partial r} \biggr] + \frac{1}{r^2 \sin\theta} \frac{\partial }{\partial \theta}\biggl(\sin\theta ~ \frac{\partial \Phi}{\partial\theta}\biggr) </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~4\pi G\rho</math> </td> </tr> </table> The Two Relevant Components of the<br /> <font color="#770000">'''Euler Equation'''</font> <br /> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"><math>~{\hat{e}}_r</math>: </td> <td align="right"> <math> ~0 </math> </td> <td align="center"> = </td> <td align="left"> <math> \biggl[ \frac{1}{\rho} \frac{\partial P}{\partial r}+ \frac{\partial \Phi }{\partial r} \biggr] - \biggl[ \frac{j^2}{r^3 \sin^2\theta} \biggr] </math> </td> </tr> <tr> <td align="right"><math>~{\hat{e}}_\theta</math>: </td> <td align="right"> <math> ~0 </math> </td> <td align="center"> = </td> <td align="left"> <math> \biggl[ \frac{1}{\rho r} \frac{\partial P}{\partial\theta} + \frac{1}{r} \frac{\partial \Phi}{\partial\theta} \biggr] - \biggl[ \frac{j^2}{r^3 \sin^3\theta} \biggr] \cos\theta </math> </td> </tr> </table> </td> </tr> </table> This set of simplified governing relations must then be supplemented by a specification of: (a) a barotropic equation of state, <math>P(\rho)</math>; and (b) the equilibrium configurations's radial specific angular momentum profile <math>j(\varpi)</math>. How does this recommended modeling approach compare to the approach outlined by [https://ui.adsabs.harvard.edu/abs/1966PhRvL..17..816O/abstract Ostriker, Bodenheimer & Lynden-Bell (1966)] and further detailed and executed by [https://ui.adsabs.harvard.edu/abs/1968ApJ...151.1089O/abstract J. P. Ostriker & P. Bodenheimer (1968)]?
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