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-rw-r--r--doc/documentation.tex4
-rwxr-xr-xinterface.ccl3
2 files changed, 4 insertions, 3 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}
diff --git a/interface.ccl b/interface.ccl
index bad74fa..742b784 100755
--- a/interface.ccl
+++ b/interface.ccl
@@ -4,9 +4,10 @@ implements: HydroBase
public:
+# These variables correspond to the Valencia formulation
+
CCTK_REAL rho type = GF Timelevels = 3 tags='ProlongationParameter="HydroBase::prolongation_type" tensortypealias="Scalar" interpolator="matter"' "rest mass density"
CCTK_REAL press type = GF Timelevels = 3 tags='ProlongationParameter="HydroBase::prolongation_type" tensortypealias="Scalar" interpolator="matter"' "gas pressure"
CCTK_REAL eps type = GF Timelevels = 3 tags='ProlongationParameter="HydroBase::prolongation_type" tensortypealias="Scalar" interpolator="matter"' "internal energy"
CCTK_REAL vel[3] type = GF Timelevels = 3 tags='ProlongationParameter="HydroBase::prolongation_type" tensortypealias="U" interpolator="matter"' "velocity"
-