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| ==Part III== | | ==Part III== |
| As a result,
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| <table border=0 cellpadding=2 align="center">
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| <tr>
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| <td align="right">
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| <math>\biggl[ \frac{dz}{d\xi} \biggr]^{-1}\mathrm{LAWE}</math>
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| </td>
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| <td align="center">
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| <math>=</math>
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| </td>
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| <td align="left">
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| <math>
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| \biggl(\frac{dz}{d\xi}\biggr) \cdot \frac{d^2f}{dz^2}
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| +
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| \biggl( \frac{d^2z}{d\xi^2}\biggr) \cdot \frac{df}{dz}
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| + \biggl[4\xi^{-1} + (n+1)\theta^{-1} (\theta^')\biggr] \cdot \frac{df}{dz}
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| + (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1}
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| + \alpha \xi^{-1} \theta^{-1} (\theta^')\biggr]\biggl[ \frac{dz}{d\xi} \biggr]^{-1} f
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| <math>=</math>
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| </td>
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| <td align="left">
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| <math>
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| - \biggl[\xi^{-1}(1 + 3z) + n \xi \theta^{n-1} z^2 \biggr]
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| \frac{d^2f}{dz^2}
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| + \biggl\{
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| \biggl( \frac{d^2z}{d\xi^2}\biggr)
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| +
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| \biggl[4\xi^{-1} + (n+1)\xi \theta^{n-1} z\biggr]
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| \biggr\}\cdot \frac{df}{dz}
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| + (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1}
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| + \alpha \theta^{n-1} z\biggr]\biggl[ \frac{dz}{d\xi} \biggr]^{-1} f
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| </math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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| <math>=</math>
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| </td>
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| <td align="left">
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| <math>
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| - \biggl[\xi^{-1}(1 + 3z) + n \xi \theta^{n-1} z^2 \biggr]
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| \frac{d^2f}{dz^2}
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| + \biggl\{
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| 4\xi^{-2}(1 + 3z)
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| +
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| 2n \theta^{n-1} [1 + 4z]z
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| +
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| n(n+1)\xi^2 \theta^{2(n-1)} z^3
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| +
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| 4\xi^{-1} + (n+1)\xi \theta^{n-1} z
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| \biggr\}\cdot \frac{df}{dz}
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| + (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1}
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| + \alpha \theta^{n-1} z\biggr]\biggl[ \frac{dz}{d\xi} \biggr]^{-1} f
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| </math>
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| </td>
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| </tr>
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| </table>
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|
| Now, suppose that <math>f = (a_0 + b_0z)</math>. We have, | | Now, suppose that <math>f = (a_0 + b_0z)</math>. We have, |
| Line 1,841: |
Line 1,692: |
| \biggl[\xi^{-1}(1 + 3z) + n \xi \theta^{n-1} z^2 \biggr]^2 | | \biggl[\xi^{-1}(1 + 3z) + n \xi \theta^{n-1} z^2 \biggr]^2 |
| \cdot \cancelto{0}{\frac{d^2f}{dz^2}} | | \cdot \cancelto{0}{\frac{d^2f}{dz^2}} |
| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| -\biggl[\xi^{-1}(1 + 3z) + n \xi \theta^{n-1} z^2 \biggr] \biggl\{
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| 4\xi^{-2}(1 + 3z)
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| +
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| 2n \theta^{n-1} [1 + 4z]z
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| +
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| n(n+1)\xi^2 \theta^{2(n-1)} z^3
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| +
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| 4\xi^{-1} + (n+1)\xi \theta^{n-1} z
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| \biggr\}b_0
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| + (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1}
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| + \alpha \theta^{n-1} z\biggr]\cdot (a_0 + b_0 z)
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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| <math>=</math>
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| </td>
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| <td align="left">
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| <math>
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| (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1}
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| \biggr](a_0 + b_0 z)
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| +
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| \alpha (n+1) \theta^{n-1} (a_0 z + b_0 z^2)
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| </math>
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| </td>
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| </tr>
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|
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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|
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| </td>
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| <td align="left">
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| <math>
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| - (1 + 3z)\biggl\{
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| 4\xi^{-3}(1 + 3z)
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| +
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| 2n \xi^{-1}\theta^{n-1} [1 + 4z]z
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| +
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| n(n+1)\xi \theta^{2(n-1)} z^3
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| +
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| 4\xi^{-2} + (n+1) \theta^{n-1} z
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| \biggr\}b_0
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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|
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| </td>
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| <td align="left">
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| <math>
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| - n \theta^{n-1} z^2 \biggl\{
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| 4\xi^{-1}(1 + 3z)
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| +
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| 2n \xi \theta^{n-1} [1 + 4z]z
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| +
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| n(n+1)\xi^3 \theta^{2(n-1)} z^3
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| +
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| 4 + (n+1)\xi^2 \theta^{n-1} z
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| \biggr\}b_0
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| \, .
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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| <math>=</math>
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| </td>
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| <td align="left">
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| <math>
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| (n+1)\biggl[\biggl(\frac{\sigma_c^2}{6\gamma_\mathrm{g} } \biggr) \theta^{-1}
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| \biggr](a_0 + b_0 z)
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| +
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| \alpha (n+1) \theta^{n-1} (a_0 z + b_0 z^2)
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| -
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| b_0(1+3z)(n+1)\theta^{n-1}z
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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|
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| </td>
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| <td align="center">
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|
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| </td>
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| <td align="left">
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| <math>
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| - (1 + 3z)\biggl\{
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| 4\xi^{-3}(1 + 3z)
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| +
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| 2n \xi^{-1}\theta^{n-1} [1 + 4z]z
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| +
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| n(n+1)\xi \theta^{2(n-1)} z^3
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| +
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| 4\xi^{-2}
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| \biggr\}b_0
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| </math>
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| </td>
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| </tr>
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| <tr>
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| <td align="right">
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| </td>
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| <td align="center">
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| </td>
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| <td align="left">
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| <math>
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| - n z^2 \biggl\{
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| 4\xi^{-1}\theta^{n-1} (1 + 3z)
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| +
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| 2n \xi \theta^{2(n-1)} [1 + 4z]z
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| +
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| n(n+1)\xi^3 \theta^{3(n-1)} z^3
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| +
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| 4\theta^{n-1} + (n+1)\xi^2 \theta^{2(n-1)} z
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| \biggr\}b_0
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| \, .
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| </math> | | </math> |
| </td> | | </td> |
Hypergeometric Differential Equation
According to §9.151 (p. 1045) of Gradshteyn & Ryzhik (1965), "… a hypergeometric series is one of the solutions of the differential equation,
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which is called the hypergeometric equation. And, according to §9.10 (p. 1039) of Gradshteyn & Ryzhik (1965), "A hypergeometric series is a series of the form,
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Among other attributes, Gradshteyn & Ryzhik (1965) note that this, "… series terminates if or is equal to a negative integer or to zero."
LAWE
Familiar Foundation
Drawing from an accompanying discussion, we have the,
LAWE: Linear Adiabatic Wave (or Radial Pulsation) Equation
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where,
Multiplying through by , and making the variable substitutions,
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the LAWE may be rewritten as,
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If we furthermore adopt the variable definition,
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we obtain what we will refer to as the,
Specifically for Polytropes
Let's look at the expression for the function, , that arises in the context of polytropic spheres.
General Expression for the Function μ
First, we note that,
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where,
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Hence,
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Alternatively,
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Yes!
Trial Displacement Function
Now, building on an accompanying discussion, let's guess,
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Flipping it around, we have alternatively,
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Plug into Kopal (1948) LAWE
Replace ftrial by μ
Plugging this trial function into the Kopal (1948) LAWE and recognizing that , we find,
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Noting that, and
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the frequency-squared term may be rewritten as,
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Replace μ by ftrial
Making instead the alternate substitution, namely,
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we have,
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Noting that,
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we furthermore can write,
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Seek Hypergeometric Form
Start with the standard LAWE, namely,
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Part I
Try switching the independent variable from to such that,
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and,
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Part II
| Part I Summary … |
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Also,
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WRONG:
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BETTER:
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As a result,
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LAWE
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Part III
Now, suppose that . We have,
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Example Density- and Pressure-Profiles
| Properties of Analytically Defined, Spherically Symmetric, Equilibrium Structures |
| Model |
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| Uniform-density |
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| Linear |
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| Parabolic |
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| Polytrope |
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Uniform Density
In the case of a uniform-density, incompressible configuration, the Kopal (1948) LAWE becomes,
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Given that, in the equilibrium state,
we obtain the LAWE derived by 📚 T. E. Sterne (1937, MNRAS, Vol. 97, pp. 582 - 593) — see his equation (1.91) on p. 585 — namely,
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where,
This also matches, respectively, equations (8) and (9) of 📚 Z. Kopal (1948, Proc. NAS, Vol. 34, Issue 8, pp.377-384), aside from what, we presume, is a type-setting error that appears in the numerator of the second term on the RHS of his equation (8): appears, whereas it should be .
In order to see if this differential equation is of the same form as the hypergeometric expression, we'll make the substitution,
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in which case the 📚 Sterne (1937) LAWE may be rewritten as,
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This is, indeed, of the hypergeometric form if we set
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Combining this last pair of expressions gives,
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and,
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Example α = -1
If we set , then the eigenvector is,
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and the corresponding eigenfrequency is obtained from the expression,
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As we have reviewed in a separate discussion, this is identical to the eigenvector identified by 📚 Sterne (1937) as mode "".
More Generally
More generally, in agreement with 📚 Sterne (1937), for any (positive integer) mode number, , we find,
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And, in terms of the hypergeometric function series, the corresponding eigenfunction is,
See Also