State that the HydroBase variables correspond to the Valencia formulation.

git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinBase/HydroBase/trunk@9 57fe0bb3-ccba-405f-9b23-de0201f165b7

1 files changed, 2 insertions, 2 deletions

diff --git a/doc/documentation.tex b/doc/documentation.tex
index 268068c..cdf33f7 100644
--- a/doc/documentation.tex
+++ b/doc/documentation.tex
@@ -130,7 +130,7 @@ are common to most if not all hydrodynamics codes solving the Euler
 equations, the so called primitive variables. These are also the variables which are needed
 to couple to a spacetime solver and which are usually needed by analysis thorns. The usage of
 a common set of variables by different hydrodynamics codes creates the possibility to share
-parts of the code, e.g. initial data solvers or analysis routines. 
+parts of the code, e.g.\ initial data solvers or analysis routines. 
 
 Currently the defined primitive variables are (see~\cite{livrevgrfd} for
 details):
@@ -172,7 +172,7 @@ a central access point for analysis thorns.
 
 \subsection{Acknowledgments}
 
-This thorn was produced by Tanja Bode, Roland Haas, Frank Löffler and Erik Schnetter.
+This thorn was produced by Tanja Bode, Roland Haas, Frank Löffler, and Erik Schnetter.
 
 \begin{thebibliography}{9}
 \bibitem{livrevgrrfd}