[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 310)

jfaber at einsteintoolkit.org jfaber at einsteintoolkit.org
Tue Mar 13 11:19:25 CDT 2012


User: jfaber
Date: 2012/03/13 11:19 AM

Modified:
 /
  ET.tex

Log:
 One more change to "specific internal energy"

File Changes:

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

File [modified]: ET.tex
Delta lines: +2 -2
===================================================================
--- ET.tex	2012-03-13 16:15:16 UTC (rev 309)
+++ ET.tex	2012-03-13 16:19:25 UTC (rev 310)
@@ -1519,8 +1519,8 @@
 hydrodynamic quantities, with several different reconstruction methods
 and Riemann solvers, as we discuss below.  In such a scheme, we define
 a set of ``conserved'' hydrodynamic variables, defined in terms of the
-``primitive'' physical variables such as mass and internal energy
-density, pressure, and velocity.  Wherever derivatives of hydrodynamic
+``primitive'' physical variables such as mass density, specific internal energy, 
+pressure, and velocity.  Wherever derivatives of hydrodynamic
 terms appear in the evolution equations for the conserved variables,
 they are restricted to appear only inside divergence terms
 (referred to as fluxes) and never in the source terms.  By calculating fluxes between pairs of neighboring points where  field and hydrodynamic terms are evaluated, we



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