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==Part III== Now, suppose that <math>f = (a_0 + b_0z)</math>. We have, <table border=0 cellpadding=2 align="center"> <tr> <td align="right"> LAWE </td> <td align="center"> <math>=</math> </td> <td align="left"> <math>\biggl[ \xi^{-2}(1+3z)^2 + 2n(1+3z)z^2 \theta^{n-1} + n^2 \xi^2 \theta^{2(n-1)}z^4 \biggr] \cdot \cancelto{0}{\frac{d^2f}{dz^2}} + (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1} + \alpha \theta^{n-1} z\biggr](a_0 + b_0z) + \biggl\{ (n-1) + (n - 3)z \biggr\} \theta^{n-1} z \cdot b_0 </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1} \biggr](a_0 + b_0z) + \biggl\{ (n+1)\alpha (a_0 + b_0z) + b_0(n-1) + b_0(n - 3)z \biggr\} \theta^{n-1} z </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1} \biggr](a_0 + b_0z) + \biggl\{ (n+1)\alpha (a_0 ) + b_0(n-1) + \biggl[(n - 3) + (n+1)\alpha \biggr]b_0z \biggr\} \theta^{n-1} z \, . </math> </td> </tr> </table> Now, in order for the last term to be zero, we need, <table border=0 cellpadding=2 align="center"> <tr> <td align="right"> <math>0</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> \biggl[(n - 3) + (n+1)\alpha \biggr] </math> </td> </tr> <tr> <td align="right"> <math>\Rightarrow ~~~ \alpha</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> \frac{3-n}{n+1} \, . </math> </td> </tr> </table> This is precisely the relation that results from the definition of <math>\alpha \equiv (3 - 4/\gamma_g)</math> if the model is evolved assuming <math>\gamma_g = (n+1)/n</math>. We simultaneously seek the relation, <table border=0 cellpadding=2 align="center"> <tr> <td align="right"> <math>0</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> (n+1)\alpha (a_0 ) + b_0(n-1) </math> </td> </tr> <tr> <td align="right"> <math>\Rightarrow ~~~ b_0</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> \biggl[ \frac{n+1}{1-n} \biggr] \alpha (a_0 ) </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> a_0 \biggl[ \frac{3-n}{1-n} \biggr] </math> </td> </tr> </table> It appears as though the leading coefficient, <math>a_0</math>, is arbitrary, so we will set it equal to unity. This means that the displacement function is, <table border=0 cellpadding=2 align="center"> <tr> <td align="right"> <math>f</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> 1 + \biggl[ \frac{3-n}{1-n} \biggr]z \, . </math> </td> </tr> </table> This expression for the displacement function, <math>f</math>, is identical to the [[SSC/Stability/InstabilityOnsetOverview#ExactPolytropicSolution|expression found inside the square brackets of our separately derived exact solution of the polytropic LAWE]]. Furthermore, given the notation, <math>(\sigma_c^2/\gamma_g) = (\mathfrak{F}-2\alpha)</math>, the first term on the RHS of the LAWE will go to zero when, <math>\mathfrak{F} = 2(3-n)/(n+1)</math>.
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