[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 259)

[tanja.bode at physics.gatech.edu]

User: tbode
Date: 2012/03/05 04:00 PM

Modified:
 /
  ET.tex

Log:
 Clear up TOV solver atmosphere statement.

File Changes:

Directory: /
============

File [modified]: ET.tex
Delta lines: +2 -2
===================================================================
--- ET.tex	2012-03-05 21:01:13 UTC (rev 258)
+++ ET.tex	2012-03-05 21:59:59 UTC (rev 259)
@@ -1048,13 +1048,13 @@
 $\Phi$ the logarithm of the lapse.  The routine also supplies the analytically known 
 solution in the exterior,
 \begin{eqnarray}
-     P & = & {\tt TOV\_atmosphere},\nonumber \\
+     P & = & P({\tt TOV\_atmosphere}),\nonumber \\
      m & = & M, \nonumber\\
   \Phi & = &\dfrac{1}{2} \log(1-2M / r)
   \label{eq:TOVexterior}
 \end{eqnarray}
 where {\tt TOV\_atmosphere} is a parameter used to specify the density of the 
-ambient atmosphere.  Since the isotropic radius $\bar{r}$ is the more 
+ambient atmosphere and a polytropic equation of state is assumed. Since the isotropic radius $\bar{r}$ is the more 
 commonly preferred choice to initiate dynamical calculations, the code then 
 transforms all variables into isotropic coordinates, integrating the radius 
 conversion formula