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[svn:einsteintoolkit] EOS_Omni/trunk/doc/ (Rev. 43)
by cott＠tapir.caltech.edu 19 Apr '11

19 Apr '11

User: cott Date: 2011/04/19 07:12 PM Modified: /trunk/doc/ documentation.tex Log: * describe hybrid EOS File Changes: Directory: /trunk/doc/ ====================== File [modified]: documentation.tex Delta lines: +57 -3 =================================================================== --- trunk/doc/documentation.tex 2011-04-19 15:16:15 UTC (rev 42) +++ trunk/doc/documentation.tex 2011-04-20 00:12:05 UTC (rev 43) @@ -76,6 +76,18 @@ % homepage at www.cactuscode.org) \usepackage{../../../../doc/latex/cactus} +\newenvironment{equationarray} +{\arraycolsep 0.14 em +\begin{eqnarray}} +{\end{eqnarray}} + +\newenvironment{equationarray*} +{\arraycolsep 0.14 em +\begin{eqnarray*}} +{\end{eqnarray*}} + + + \begin{document} % The author of the documentation @@ -290,8 +302,46 @@ \subsection{Hybrid} -\textbf{TODO: Not yet documented.} +The hybrid EOS was introduced by \cite{janka:93} for use in simplified +simulations of stellar collapse to mimic (1) the stiffening of the +nuclear EOS at nuclear density and (2) to include thermal pressure in +the postbounce phase. It consists of two polytropes characterized by +($K_1$, $\gamma_1$) and ($K_2$, $\gamma_2$) and a thermal $\gamma-$law +component described by $\gamma_\mathrm{th}$. Polytrope 1 is soft and +describes a gas of relativistic degenerate electrons with $\gamma_1 +\approx 4/3$. It is used below nuclear density ($\rho_\mathrm{nuc} +\approx 2\times10^{14}\,\mathrm{g\,cm}^{-3}$) and smoothly matched to +polytrope 2 which applies above $\rho_\mathrm{nuc}$, is stiff, and +models the repulsive core of the strong force above nuclear density +($\gamma_2 \gtrsim 2.5$). $K_2$ is completely determined by +$P_1(\rho_\mathrm{nuc}) = P_2(\rho_\mathrm{nuc})$ and $K_1, \gamma_1,$ +and $\gamma_2$. The full functional form of the EOS +$P=P(\rho,\epsilon)$ with the thermal component (which takes into +account shock heating) is given by +\begin{equationarray} + P & = & \frac{\gamma - \gamma_{\rm th}}{\gamma - 1} + K \rho_{\rm nuc}^{\gamma_1 - \gamma} + \rho^{\gamma} - \frac{(\gamma_{\rm th} - 1) (\gamma - \gamma_1)} + {(\gamma_1 - 1) (\gamma_2 - 1)} + K \rho_{\rm nuc}^{\gamma_1 - 1} \rho + + (\gamma_{\rm th} - 1) \rho \epsilon\,. + \label{eq:hybrid_eos} +\end{equationarray}% +The \texttt{EOS\_Omni} parameters for the hybrid EOS are the following: + +\begin{tabular}{ll} +\texttt{hybrid\_gamma1} & $\gamma_1$, $\gamma_1 = 1.325$ is an appropriate choice.\\ +\texttt{hybrid\_gamma2} & $\gamma_2$, $\gamma_2 = 2.5$ is an appropriate choice.\\ +\texttt{hybrid\_gamma\_th} & $\gamma_\mathrm{th}$, perhaps $1.5$.\\ +\texttt{hybrid\_k1} & $K_1$, $0.4640517$ in solar units for relativistic degenerate e$^{-}$.\\ +\texttt{hybrid\_rho\_nuc} & nuclear density, standard is $3.238607\times 10^{-4}$ in solar units. +\end{tabular} + + + + + \subsection{Finite-Temperature Nuclear} \textbf{TODO: Not yet documented; not even mentioned yet in some other @@ -363,10 +413,14 @@ -%\begin{thebibliography}{9} +\begin{thebibliography}{9} +\bibitem{janka:93} Janka, H.-T., Zwerger, T., \& Moenchmeyer, R.\ 1993, Astron. Astrophys., 268, 360 -%\end{thebibliography} + + +\end{thebibliography} + % Do not delete next line % END CACTUS THORNGUIDE

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[svn:einsteintoolkit] www/release-info/ (Rev. 560)
by knarf＠cct.lsu.edu 19 Apr '11

19 Apr '11

User: knarf Date: 2011/04/19 01:43 PM Modified: /release-info/ parse_testsuite_results.cgi Log: set new date for marking old results File Changes: Directory: /release-info/ ========================= File [modified]: parse_testsuite_results.cgi Delta lines: +2 -2 =================================================================== --- release-info/parse_testsuite_results.cgi 2011-04-19 18:00:34 UTC (rev 559) +++ release-info/parse_testsuite_results.cgi 2011-04-19 18:43:15 UTC (rev 560) @@ -20,8 +20,8 @@ my $nthreads = 1; my %fileinfo = (); -#my $too_old = "Mon Mar 28 00:00:00 CDT 2011"; -my $too_old = "1 week ago"; +my $too_old = "Tue Apr 19 12:00:00 CDT 2011"; +#my $too_old = "1 week ago"; # open each log file one by one foreach my $filename (@filenames) {

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[svn:einsteintoolkit] www/release-info/ (Rev. 559)
by knarf＠cct.lsu.edu 19 Apr '11

19 Apr '11

User: knarf Date: 2011/04/19 01:00 PM Modified: /release-info/ run_tests Log: special run-command for philip File Changes: Directory: /release-info/ ========================= File [modified]: run_tests Delta lines: +2 -2 =================================================================== --- release-info/run_tests 2011-04-18 19:53:36 UTC (rev 558) +++ release-info/run_tests 2011-04-19 18:00:34 UTC (rev 559) @@ -8,8 +8,6 @@ cd ET_2011_05 export CCTK_TESTSUITE_RUN_COMMAND="mpirun -np \$nprocs \$exe \$parfile" -hostname | grep ^philip && - export CCTK_TESTSUITE_RUN_COMMAND="mpirun -machinefile $PBS_NODEFILE -np \$nprocs \$exe \$parfile" hostname | grep ^qb && export CCTK_TESTSUITE_RUN_COMMAND="/usr/local/packages/mvapich2/1.4/intel-11.1/bin/mpirun_rsh -hostfile $PBS_NODEFILE -np \$nprocs /bin/env MV2_ENABLE_AFFINITY=0 \$exe \$parfile" hostname | grep macbook-pro.local && @@ -27,6 +25,8 @@ export CCTK_TESTSUITE_RUN_PROCESSORS=2 export OMP_NUM_THREADS=2;; esac + hostname | grep ^philip && + export CCTK_TESTSUITE_RUN_COMMAND="mpirun -machinefile $PBS_NODEFILE -np \$nprocs /home/knarf/work/ET/openmp$OMP_NUM_THREADS \$parfile" # makeing sure openmp is really used through an external script hostname | grep ^numrel && export CCTK_TESTSUITE_RUN_COMMAND="~/bin/mpirun$OMP_NUM_THREADS -np \$nprocs \$exe \$parfile"

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[svn:einsteintoolkit] Hydro_InitExcision/trunk/test/ (Rev. 116)
by knarf＠cct.lsu.edu 19 Apr '11

19 Apr '11

User: knarf Date: 2011/04/19 12:22 PM Modified: /trunk/test/ test.ccl Log: raise tolerance for absolute errors. These are shock-tubes which larger absolute values of variables File Changes: Directory: /trunk/test/ ======================= File [modified]: test.ccl Delta lines: +1 -1 =================================================================== --- trunk/test/test.ccl 2011-04-18 04:49:10 UTC (rev 115) +++ trunk/test/test.ccl 2011-04-19 17:22:01 UTC (rev 116) @@ -1,2 +1,2 @@ -ABSTOL 1.e-10 +ABSTOL 3.e-10 RELTOL 1.e-10

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[svn:einsteintoolkit] EinsteinExamples/trunk/par/ (Rev. 22)
by knarf＠cct.lsu.edu 19 Apr '11

19 Apr '11

User: knarf Date: 2011/04/19 11:29 AM Modified: /trunk/par/ qc0-mclachlan.par Log: set the number of timelevels of the ADM metric to three to avoid problems with the AHFinder File Changes: Directory: /trunk/par/ ====================== File [modified]: qc0-mclachlan.par Delta lines: +3 -0 =================================================================== --- trunk/par/qc0-mclachlan.par 2010-11-21 03:27:30 UTC (rev 21) +++ trunk/par/qc0-mclachlan.par 2011-04-19 16:29:21 UTC (rev 22) @@ -259,6 +259,9 @@ ADMBase::initial_dtlapse = "zero" ADMBase::initial_dtshift = "zero" +# needed for AHFinderDirect +ADMBase::metric_timelevels = 3 + TwoPunctures::par_b = 1.168642873 TwoPunctures::par_m_plus = 0.453 TwoPunctures::par_m_minus = 0.453

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[svn:einsteintoolkit] EOS_Omni/trunk/doc/ (Rev. 42)
by cott＠tapir.caltech.edu 19 Apr '11

19 Apr '11

User: cott Date: 2011/04/19 10:16 AM Modified: /trunk/doc/ documentation.tex Log: * some work on documentation. more to come File Changes: Directory: /trunk/doc/ ====================== File [modified]: documentation.tex Delta lines: +84 -62 =================================================================== --- trunk/doc/documentation.tex 2011-03-31 17:40:09 UTC (rev 41) +++ trunk/doc/documentation.tex 2011-04-19 15:16:15 UTC (rev 42) @@ -79,7 +79,8 @@ \begin{document} % The author of the documentation -\author{Christian D. Ott \textless cott(a)tapir.caltech.edu\textgreater} +\author{Christian D. Ott \textless cott(a)tapir.caltech.edu\textgreater, \\ +Erik Schnetter \textless eschnetter(a)perimeterinstitute.ca\textgreater} % The title of the document (not necessarily the name of the Thorn) \title{EOS\_Omni} @@ -87,7 +88,7 @@ % the date your document was last changed, if your document is in CVS, % please use: % \date{$ $Date: 2004-01-07 12:12:39 -0800 (Wed, 07 Jan 2004) $ $} -\date{June 27 2010} +\date{April 19, 2011} \maketitle @@ -98,9 +99,14 @@ % \def\mydef etc \begin{abstract} - This thorn provides a unified EOS (Equation Of State) interface and - implements multiple EOS\@. Currently, these are the polytropic EOS, - the gamma-law EOS, and a hybrid EOS\@. + \noindent This thorn provides a unified EOS (Equation Of State) + interface and implements multiple analytic EOS and provides table + reader and interpolation routines for finite-temperature + microphysical EOS available from {\tt + http://www.stellarcollapse.org}\@. Currently, the implemented + analytic EOS are the polytropic EOS, the gamma-law EOS, a hybrid EOS + consisting of a 2-piece piecewise-polytrope with an a thermal, + gamma-law component. \end{abstract} @@ -110,24 +116,22 @@ Equations of State (EOS) are crucial for hydrodynamics and hydro codes (as well as other codes needing/providing microphysics) are closely coupled to EOS and call EOS routines many times for -each grid point during the caculation of a time update. +each grid point during the calculation of a time update. -\texttt{EOS\_Omni} is presently coded for cold and hot EOS, -including those based on microphysical models. It does currently -assume nuclear statistical equilibrium (NSE) with density, -specific internal energy (or temperature), and electron fraction -being the independent variables. \texttt{EOS\_Omni} can be called -on arrays or on single grid points. +\texttt{EOS\_Omni} is presently coded for cold and hot EOS, including +those based on microphysical models. It does currently assume nuclear +statistical equilibrium (NSE) with rest-mass density $\rho$, specific +internal energy $\epsilon$ (or temperature $T$), and electron fraction +$Y_e$ being the independent variables. \texttt{EOS\_Omni} can be +called on arrays or on single grid points. \section{Units} -This thorn uses \emph{solar} units where $c = G = M_{sun} = 1$. -\textbf{TODO: confirm this.} +This thorn uses \emph{solar} units where $c = G = M_{\odot} = 1$. +Temperatures are measured in MeV. - - \section{Using This Thorn} \subsection{Basic Usage} @@ -138,12 +142,13 @@ \begin{verbatim} void FUNCTION EOS_Omni_press(CCTK_INT IN eoskey, \ CCTK_INT IN havetemp, \ + CCTK_REAL IN rf_precision, \ CCTK_INT IN npoints, \ CCTK_REAL IN ARRAY rho, \ CCTK_REAL INOUT ARRAY eps, \ CCTK_REAL INOUT ARRAY temp, \ CCTK_REAL IN ARRAY ye, \ - CCTK_REAL OUT ARRAY press, \ + CCTK_REAL OUT ARRAY press \ CCTK_INT OUT ARRAY keyerr, \ CCTK_INT OUT anyerr) \end{verbatim} @@ -155,20 +160,32 @@ \item \texttt{eoskey = 1}: Polytropic EOS \item \texttt{eoskey = 2}: Gamma-Law EOS \item \texttt{eoskey = 3}: Hybrid EOS (2 Polys, 1 Gamma-Law), used - for core-collapse simulations. + for stellar core collapse simulations. + \item \texttt{eoskey = 4}: Finite-temperature microphysical EOS \end{itemize} -\item \texttt{havetemp} tells the EOS whether the internal energy - should be calculated from the temperature first, i.e.\ whether the - call is $\epsilon=\epsilon(\rho,T,Y_e), X=X(\rho,\epsilon,Y_e)$ - (both $\epsilon$ and $X$ are calculated and returned \textbf{TODO: - confirm this}) (\texttt{havetemp = 1}), or - $X=X(\rho,\epsilon,Y_e)$ (the temperature is ignored) - (\texttt{havetemp = 0}), +\item \texttt{havetemp} determines whether the EOS is to be called as + a function of $(\rho,\epsilon,Y_e)$ (\texttt{havetemp = 0}), as a + function of $(\rho,T,Y_e)$ (\texttt{havetemp = 1}). + \texttt{havetemp = 0} is the method of choice for analytic EOS during + evolution, but at the initial data stage one may need to set + \texttt{havetemp = 1} (with $T=0$) to obtain initial values for + $\epsilon$. In the case of a finite-temperature EOS (that usually + is a function of $(\rho,T,Y_e)$), a call with \texttt{havetemp = 0} + will first lead to the solution of $T(\rho,\epsilon,Y_e$) via a + Newton-Raphson-type iteration (using the supplied value of $T$ as + the starting point) and will then calculate the requested dependent + variable as a function of $X=X(\rho,T,Y_e)$. Both $X$ and the updated + $T$ are returned. + \item \texttt{npoints} tells the EOS how many data points are passed in, \item \texttt{rho,eps,temp,ye,press} are obvious, -\item \texttt{keyerr} is an array (with $n$ entries for $n$ data points) - containing error codes (relevant only for tabular EOS), +\item \texttt{rf\_precision} is a real number telling the root finding + algorithm (for finding $T(\rho,\epsilon,Y_e)$) at what relative error + to terminate the iteration. $10^{-10}$ is a good value. +\item \texttt{keyerr} is an array (with $n$ entries for $n$ data + points) containing error codes (relevant only for tabulated + microphysical EOS), \item \texttt{anyerr} is an integer $>0$ in case any error occured. \end{itemize} @@ -202,7 +219,7 @@ \subsection{Polytropic} -The \textt{poly} EOS is a \emph{polytropic} equation of state, which +The \texttt{poly} EOS is a \emph{polytropic} equation of state, which does not allow for changes in entropy: \begin{eqnarray} p & = & K \rho^\gamma @@ -215,22 +232,20 @@ temperature'' (\texttt{havetemp = 1}), then this is done using the relation \begin{eqnarray} - \epsilon & = & \frac{K}{\gamma-1} rho^{\gamma-1} + \epsilon & = & \frac{K}{\gamma-1} \rho^{\gamma-1} +\label{eq:polyeps} \end{eqnarray} (which actually ignores the temperature). -The parameter \texttt{poly\_gamma\_ini} influences the definition of -this EOS via unit conversions: $K$ is first converted from solar units -to cgs units using \texttt{poly\_gamma\_ini}, and then converted back -to solar units using \texttt{poly\_gamma}. \textbf{TODO: confirm - this.} Contrary to what the parameter name suggests, this EOS thorn -makes no distinction between initial data setup and time evolution; if -such a distinction is required, then it must be implemented outside of -this thorn. +Internally, \texttt{EOS\_Omni} uses cgs units and on startup converts +the EOS parameters from solar units to cgs units. This conversion +depends on $\gamma$ and the value of $\gamma$ at the initial +data stage (\texttt{poly\_gamma\_ini}) is used for this. +Note that contrary to what the parameter name suggests, +\texttt{EOS\_Omni} does not make a distinction between initial data +setup and time evolution; if such a distinction is required, it must +be implemented outside of this thorn. -Note: Although this EOS depends on a parameter called $\gamma$, it -should not be confused with the ``gamma-law'' EOS, which is different. - Note also: This polytropic EOS is also used as fall-back when other EOS fail. @@ -245,27 +260,34 @@ energy, and $\gamma$ is the adiabatic index set via \texttt{gl\_gamma}. -The parameter \texttt{poly\_gamma\_ini} (not \texttt{gl\_gamma\_ini}!) -influences the definition of this EOS via unit conversions: $K$ is -first converted from solar units to cgs units using -\texttt{poly\_gamma\_ini}, and then converted back to solar units -using \texttt{gl\_gamma}. \textbf{TODO: confirm this.} Note that the -parameter \texttt{gl\_gamma\_ini} is actually unused. \textbf{TODO: - confirm this.} Contrary to what the parameter name suggests, this -EOS thorn makes no distinction between initial data setup and time -evolution; if such a distinction is required, then it must be -implemented outside of this thorn. +At the initial data stage, it may be necessary to set up initial +values for $\epsilon$. For this, the \texttt{gl} EOS +implements equation (\ref{eq:polyeps}) just like the \texttt{poly} +EOS and the parameters \texttt{poly\_gamma\_ini} and +\texttt{gl\_k} must be set for this. -If the internal energy $\epsilon$ is to be ``calculated from the -temperature'' (\texttt{havetemp = 1}), then this is done using the -relation -\begin{eqnarray} - \epsilon & = & \frac{K}{\gamma-1} rho^{\gamma-1} -\end{eqnarray} -(which actually ignores the temperature). $K$ the polytropic constant -set via \texttt{gl\_k}. This is the same relation as for the -polytropic equation of state above. + +%%% The parameter \texttt{poly\_gamma\_ini} (not \texttt{gl\_gamma\_ini}!) +%%% influences the definition of this EOS via unit conversions: $K$ is +%%% first converted from solar units to cgs units using +%%% \texttt{poly\_gamma\_ini}, and then converted back to solar units +%%% using \texttt{gl\_gamma}. \textbf{TODO: confirm this.} Note that the +%%% parameter \texttt{gl\_gamma\_ini} is actually unused. \textbf{TODO: +%%% confirm this.} Contrary to what the parameter name suggests, this +%%% EOS thorn makes no distinction between initial data setup and time +%%% evolution; if such a distinction is required, then it must be +%%% implemented outside of this thorn. +%%% If the internal energy $\epsilon$ is to be ``calculated from the +%%% temperature'' (\texttt{havetemp = 1}), then this is done using the +%%% relation +%%% \begin{eqnarray} +%%% \epsilon & = & \frac{K}{\gamma-1} rho^{\gamma-1} +%%% \end{eqnarray} +%%% (which actually ignores the temperature). $K$ the polytropic constant +%%% set via \texttt{gl\_k}. This is the same relation as for the +%%% polytropic equation of state above. + \subsection{Hybrid} \textbf{TODO: Not yet documented.} @@ -301,8 +323,8 @@ \begin{table} \begin{tabular}{ll|ll} - Old Parameter & Old Value & New Parameter & New Value - \\\hline + Old Parameter & Old Value & New Parameter & New Value\\ + \hline EOS\_Polytrope::eos\_gamma & & EOS\_Omni::poly\_gamma & \\ @@ -328,7 +350,7 @@ \end{table} \begin{table} - \begin{tabular}{ll} + \begin{tabular}{llll} EOS & Description & Old Name & New Name \\\hline poly & polytropic & ??? & 2D\_Polytrope \\ gl & gamma-law & ??? & Ideal\_Fluid \\

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[svn:einsteintoolkit] pyGWAnalysis/trunk/ (Rev. 2)
by reisswig＠tapir.caltech.edu 18 Apr '11

18 Apr '11

User: reisswig Date: 2011/04/18 05:27 PM Added: /trunk/ COPYRIGHT, README /trunk/DataAnalysis/ AdLIGO_ZERO_DET_high_P.dat, AdVrefsens.dat, DataAnalysis.py, RadiatedQuantities.py, eligo.dat, harmonics.py /trunk/DiscreteFunction/ DiscreteFunction.py, Utils.py, WaveFunction.py /trunk/Examples/ integrate-modes-ffi.py, rad.py Log: Scripts and first examples. File Changes: Directory: /trunk/DataAnalysis/ =============================== File [added]: AdLIGO_ZERO_DET_high_P.dat Delta lines: <Unavailable> File [added]: AdVrefsens.dat Delta lines: <Unavailable> File [added]: DataAnalysis.py Delta lines: <Unavailable> File [added]: RadiatedQuantities.py Delta lines: <Unavailable> File [added]: eligo.dat Delta lines: <Unavailable> File [added]: harmonics.py Delta lines: <Unavailable> Directory: /trunk/DiscreteFunction/ =================================== File [added]: DiscreteFunction.py Delta lines: <Unavailable> File [added]: Utils.py Delta lines: <Unavailable> File [added]: WaveFunction.py Delta lines: <Unavailable> Directory: /trunk/Examples/ =========================== File [added]: integrate-modes-ffi.py Delta lines: <Unavailable> File [added]: rad.py Delta lines: <Unavailable> Directory: /trunk/ ================== File [added]: COPYRIGHT Delta lines: <Unavailable> File [added]: README Delta lines: <Unavailable>

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[svn:einsteintoolkit] www/release-info/ (Rev. 558)
by knarf＠cct.lsu.edu 18 Apr '11

18 Apr '11

User: knarf Date: 2011/04/18 02:53 PM Modified: /release-info/ compile_tests Log: use GetComponents from release branch File Changes: Directory: /release-info/ ========================= File [modified]: compile_tests Delta lines: +1 -1 =================================================================== --- release-info/compile_tests 2011-04-18 18:04:14 UTC (rev 557) +++ release-info/compile_tests 2011-04-18 19:53:36 UTC (rev 558) @@ -7,7 +7,7 @@ # Ensure that Cactus does not already exist test ! -e $CROOT -wget --no-check-certificate https://github.com/gridaphobe/CRL/raw/master/GetComponents -O GetComponents +wget --no-check-certificate https://github.com/gridaphobe/CRL/raw/ET_2011_05/GetComponents -O GetComponents wget http://svn.einsteintoolkit.org/manifest/$LOC/einsteintoolkit.th -O einsteintoolkit.th chmod a+x GetComponents

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[svn:einsteintoolkit] www/release-info/ (Rev. 557)
by schnetter＠cct.lsu.edu 18 Apr '11

18 Apr '11

User: eschnett Date: 2011/04/18 01:04 PM Modified: /release-info/ hopper__1_1.log, hopper__2_2.log Log: Update Hopper results File Changes: Directory: /release-info/ ========================= File [modified]: hopper__1_1.log Delta lines: +10 -10 =================================================================== --- release-info/hopper__1_1.log 2011-04-18 17:47:46 UTC (rev 556) +++ release-info/hopper__1_1.log 2011-04-18 18:04:14 UTC (rev 557) @@ -773,11 +773,11 @@ AHFinderDirect: Kerr-definition-expansion Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-definition-expansion-product - Success: 2 files compared, 2 differ in the last digits + Success: 2 files compared, 1 differ in the last digits AHFinderDirect: Kerr-definition-inner-expansion Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-definition-mean-curvature - Success: 2 files compared, 2 differ in the last digits + Success: 2 files compared, 1 differ in the last digits AHFinderDirect: Kerr-modification-radius Success: 2 files compared, 1 differ in the last digits AHFinderDirect: Kerr-rotating-180 @@ -789,13 +789,13 @@ AHFinderDirect: Kerr-selection-areal-radius-definition-expansion-product Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-selection-mean-coordinate-radius - Success: 2 files compared, 2 differ in the last digits + Success: 2 files compared, 1 differ in the last digits AHFinderDirect: checkpointML - Success: 7 files compared, 7 differ in the last digits + Success: 7 files compared, 6 differ in the last digits AHFinderDirect: misner1.2-025 Success: 55 files compared, 9 differ in the last digits AHFinderDirect: recoverML - Success: 5 files compared, 5 differ in the last digits + Success: 5 files compared, 3 differ in the last digits CarpetIOHDF5: CarpetWaveToyNewRecover_test_1proc Success: 12 files compared, 7 differ in the last digits CarpetIOHDF5: CarpetWaveToyRecover_test_1proc @@ -807,7 +807,7 @@ DistortedBHIVP: E2xeon_test_dbh Success: 100 files compared, 44 differ in the last digits Exact: Schwarzschild_EF - Failure: 112 files compared, 27 differ, 27 differ significantly + Success: 112 files compared, 7 differ in the last digits Exact: bowl-evolution Success: 24 files identical Exact: bowl-init @@ -1007,15 +1007,15 @@ WeylScal4: teukolsky Success: 8 files compared, 6 differ in the last digits WeylScal4: teukolskyID - Success: 8 files compared, 6 differ in the last digits + Failure: 8 files missing, 0 files compared, 0 differ ======================================================================== Summary for configuration sim - Time -> Fri Apr 8 22:22:50 PDT 2011 - Host -> nid04944 + Time -> Mon Apr 18 10:17:36 PDT 2011 + Host -> nid04945 User -> schnette Total available tests -> 171 @@ -1032,10 +1032,10 @@ nonstaggered (from CarpetReduce) staggered (from CarpetReduce) - Schwarzschild_EF (from Exact) halfsphere_pugh_ppm (from Hydro_InitExcision) x_flip_pugh_ppm (from Hydro_InitExcision) x_pugh_ppm (from Hydro_InitExcision) + teukolskyID (from WeylScal4) ======================================================================== File [modified]: hopper__2_2.log Delta lines: +33 -46 =================================================================== --- release-info/hopper__2_2.log 2011-04-18 17:47:46 UTC (rev 556) +++ release-info/hopper__2_2.log 2011-04-18 18:04:14 UTC (rev 557) @@ -154,6 +154,18 @@ Tests missed for different number of processors required: + checkpointML in AHFinderDirect + (EinsteinAnalysis/AHFinderDirect/test/checkpointML.par) + Requires 1 processors + + misner1.2-025 in AHFinderDirect + (EinsteinAnalysis/AHFinderDirect/test/misner1.2-025.par) + Requires 1 processors + + recoverML in AHFinderDirect + (EinsteinAnalysis/AHFinderDirect/test/recoverML.par) + Requires 1 processors + CarpetWaveToyNewRecover_test_1proc in CarpetIOHDF5 (Carpet/CarpetIOHDF5/test/CarpetWaveToyNewRecover_test_1proc.par) Requires 1 processors @@ -220,7 +232,7 @@ ADMConstraints [4] - AHFinderDirect [15] + AHFinderDirect [12] DistortedBHIVP [1] @@ -341,12 +353,6 @@ Kerr-selection-mean-coordinate-radius - checkpointML - - misner1.2-025 - - recoverML - DistortedBHIVP: E2xeon_test_dbh @@ -772,39 +778,33 @@ ADMConstraints: test_ADM Success: 16 files identical AHFinderDirect: Kerr - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-Cartoon Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-definition-expansion - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-definition-expansion-product - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-definition-inner-expansion - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-definition-mean-curvature - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-modification-radius - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 1 differ in the last digits AHFinderDirect: Kerr-rotating-180 - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-rotating-90 Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-selection-areal-radius - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 1 differ in the last digits AHFinderDirect: Kerr-selection-areal-radius-definition-expansion-product - Failure: 2 files compared, 2 differ, 2 differ significantly + Success: 2 files compared, 2 differ in the last digits AHFinderDirect: Kerr-selection-mean-coordinate-radius - Failure: 2 files compared, 2 differ, 2 differ significantly - AHFinderDirect: checkpointML - Failure: 7 files compared, 7 differ, 7 differ significantly - AHFinderDirect: misner1.2-025 - Failure: 55 files compared, 9 differ, 2 differ significantly - AHFinderDirect: recoverML - Failure: 5 files compared, 5 differ, 5 differ significantly + Success: 2 files compared, 1 differ in the last digits DistortedBHIVP: E2xeon_test_dbh Success: 100 files compared, 44 differ in the last digits Exact: Schwarzschild_EF - Failure: 112 files compared, 27 differ, 27 differ significantly + Success: 112 files compared, 7 differ in the last digits Exact: bowl-evolution Success: 24 files identical Exact: bowl-init @@ -882,7 +882,7 @@ InterpToArray: wavetoy Success: 25 files compared, 1 differ in the last digits ML_BSSN_Test: gw3d_Exact_ord4_15 - Success: 6 files compared, 6 differ in the last digits + Failure: 6 files compared, 6 differ, 6 differ significantly ML_BSSN_Test: gw3d_McLachlan_ord4_15 Success: 105 files compared, 105 differ in the last digits ML_BSSN_Test: gw3d_McLachlan_ord4_30 @@ -1011,39 +1011,26 @@ Summary for configuration sim - Time -> Fri Apr 8 23:00:14 PDT 2011 - Host -> nid04944 + Time -> Mon Apr 18 10:55:32 PDT 2011 + Host -> nid04945 User -> schnette Total available tests -> 171 - Unrunnable tests -> 46 - Runnable tests -> 125 + Unrunnable tests -> 49 + Runnable tests -> 122 Total number of thorns -> 161 Number of tested thorns -> 37 - Number of tests passed -> 107 + Number of tests passed -> 117 Number passed only to - set tolerance -> 70 - Number failed -> 18 + set tolerance -> 80 + Number failed -> 5 Tests failed: - Kerr (from AHFinderDirect) - Kerr-definition-expansion (from AHFinderDirect) - Kerr-definition-expansion-product (from AHFinderDirect) - Kerr-definition-inner-expansion (from AHFinderDirect) - Kerr-definition-mean-curvature (from AHFinderDirect) - Kerr-modification-radius (from AHFinderDirect) - Kerr-rotating-180 (from AHFinderDirect) - Kerr-selection-areal-radius (from AHFinderDirect) - Kerr-selection-areal-radius-definition-expansion-product (from AHFinderDirect) - Kerr-selection-mean-coordinate-radius (from AHFinderDirect) - checkpointML (from AHFinderDirect) - misner1.2-025 (from AHFinderDirect) - recoverML (from AHFinderDirect) - Schwarzschild_EF (from Exact) halfsphere_pugh_ppm (from Hydro_InitExcision) x_flip_pugh_ppm (from Hydro_InitExcision) x_pugh_ppm (from Hydro_InitExcision) + gw3d_Exact_ord4_15 (from ML_BSSN_Test) gw3d_McLachlan_ord4_30 (from ML_BSSN_Test) ========================================================================

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[svn:einsteintoolkit] manifest/trunk/ (Rev. 89)
by knarf＠cct.lsu.edu 18 Apr '11

18 Apr '11

User: knarf Date: 2011/04/18 12:52 PM Modified: /trunk/ einsteintoolkit.th Log: already now use release-version of GetComponents, switching this back in the trunk version after the release File Changes: Directory: /trunk/ ================== File [modified]: einsteintoolkit.th Delta lines: +1 -0 =================================================================== --- trunk/einsteintoolkit.th 2011-04-18 14:30:35 UTC (rev 88) +++ trunk/einsteintoolkit.th 2011-04-18 17:52:53 UTC (rev 89) @@ -52,6 +52,7 @@ !URL = git://github.com/gridaphobe/CRL.git !AUTH_URL = git@github.com:gridaphobe/CRL.git !CHECKOUT = GetComponents +!REPO_BRANCH = ET_2011_05

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