Difference between revisions of "User:Tohline/SSC/Perspective Reconciliation"

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(Begin reconciliation discussion)
 
(→‎Linearizing the Key Relations: Begin laying out derivation table)
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<table border="3" align="center" cellpadding="10">
<table border="3" align="center" cellpadding="10">
<tr>
  <th align="center" colspan="2"><font color="darkgreen" size="+1">Continuity Equation</font></th>
</tr>
<tr>
<tr>
   <th align="center" width="50%">Lagrangian Perspective</th>
   <th align="center" width="50%">Lagrangian Perspective</th>
   <th align="center" width="50%">Eulerian Perspective</th>
   <th align="center" width="50%">Eulerian Perspective</th>
</tr>
<tr>
  <td align="center">
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\frac{d\rho}{dt}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~- \rho \nabla\cdot\vec{v}</math>
  </td>
</tr>
</table>
</div>
  </td>
  <td align="center">
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\frac{\partial\rho}{\partial t}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~- \rho \nabla\cdot\vec{v} - \vec{v}\cdot \nabla\rho</math>
  </td>
</tr>
</tr>
</table>
</table>
</div>


  </td>
</tr>
<tr>
  <th align="center" colspan="2">Spherically Symmetric Initial Configurations &amp; Purely Radial Perturbations</th>
</tr>
<tr>
  <td align="center">


<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\frac{d\rho}{dt}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~-  \frac{\rho}{r^2} \frac{\partial}{\partial r} \biggl( r^2 v_r \biggr)</math>
  </td>
</tr>
</table>
</div>
  </td>
  <td align="center">
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\frac{\partial\rho}{\partial t}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~- \frac{\rho}{r^2} \frac{\partial}{\partial r} \biggl( r^2 v_r \biggr) - v_r \frac{\partial \rho}{\partial r}</math>
  </td>
</tr>
</table>
</div>
  </td>
</tr>
</table>


=See Also=
=See Also=

Revision as of 23:44, 11 December 2014

Reconciling Eulerian versus Lagrangian Perspectives

Whitworth's (1981) Isothermal Free-Energy Surface
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Linearizing the Key Relations

Continuity Equation
Lagrangian Perspective Eulerian Perspective

<math>~\frac{d\rho}{dt}</math>

<math>~=</math>

<math>~- \rho \nabla\cdot\vec{v}</math>

<math>~\frac{\partial\rho}{\partial t}</math>

<math>~=</math>

<math>~- \rho \nabla\cdot\vec{v} - \vec{v}\cdot \nabla\rho</math>

Spherically Symmetric Initial Configurations & Purely Radial Perturbations

<math>~\frac{d\rho}{dt}</math>

<math>~=</math>

<math>~- \frac{\rho}{r^2} \frac{\partial}{\partial r} \biggl( r^2 v_r \biggr)</math>

<math>~\frac{\partial\rho}{\partial t}</math>

<math>~=</math>

<math>~- \frac{\rho}{r^2} \frac{\partial}{\partial r} \biggl( r^2 v_r \biggr) - v_r \frac{\partial \rho}{\partial r}</math>

See Also