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New changesets in Carpet Mercurial
by Carpet mercurial repositories 04 Apr '12

04 Apr '12

changeset: 3505:ab6a712c7eb6 tag: tip user: Ian Hinder <ian.hinder(a)aei.mpg.de> date: Wed Apr 04 13:14:38 2012 +0200 summary: Make timer tree output precision and threshold configurable with parameters

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[svn:einsteintoolkit] Workshop_Spring_2012/numerical_relativity/ (Rev. 33)
by bcmsma＠astro.rit.edu 04 Apr '12

04 Apr '12

User: bmundim Date: 2012/04/04 02:50 AM Added: /numerical_relativity/figs/ all_waves.eps, all_waves.pdf, finite_volume.eps, finite_volume.pdf, rarefaction.eps, rarefaction.pdf, shock.eps, shock.pdf Modified: /numerical_relativity/ numerical_relativity.tex Log: valencia formulation plus figs for conservation laws... (must sleep nw) File Changes: Directory: /numerical_relativity/figs/ ====================================== File [added]: all_waves.eps Delta lines: <Unavailable> File [added]: all_waves.pdf Delta lines: <Unavailable> File [added]: finite_volume.eps Delta lines: <Unavailable> File [added]: finite_volume.pdf Delta lines: <Unavailable> File [added]: rarefaction.eps Delta lines: <Unavailable> File [added]: rarefaction.pdf Delta lines: <Unavailable> File [added]: shock.eps Delta lines: <Unavailable> File [added]: shock.pdf Delta lines: <Unavailable> Directory: /numerical_relativity/ ================================= File [modified]: numerical_relativity.tex Delta lines: <Unavailable>

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[svn:einsteintoolkit] Workshop_Spring_2012/cactuswriting/ (Rev. 32)
by jfaber＠einsteintoolkit.org 03 Apr '12

03 Apr '12

User: jfaber Date: 2012/04/03 10:43 PM Added: /cactuswriting/ cactuswriting.aux, cactuswriting.log, cactuswriting.nav, cactuswriting.out, cactuswriting.pdf, cactuswriting.snm, cactuswriting.tex, cactuswriting.toc, config.png, config.tiff, interface1.png, interface1.tiff, interface2.png, interface2.tiff, interface3.png, interface3.tiff, make.png, make.tiff, param1.png, param1.tiff, param2.png, param2.tiff, schedule1.png, schedule1.tiff, schedule2.png, schedule2.tiff, schedule3.png, schedule3.tiff, srccode.png, srccode.tiff, srccode2.png, srccode2.tiff, thornlist.png, thornlist.tiff Log: Added notes on writing a cactus thorn (low level) File Changes: Directory: /cactuswriting/ ========================== File [added]: cactuswriting.aux Delta lines: <Unavailable> File [added]: cactuswriting.log Delta lines: <Unavailable> File [added]: cactuswriting.nav Delta lines: <Unavailable> File [added]: cactuswriting.out Delta lines: <Unavailable> File [added]: cactuswriting.pdf Delta lines: <Unavailable> File [added]: cactuswriting.snm Delta lines: <Unavailable> File [added]: cactuswriting.tex Delta lines: <Unavailable> File [added]: cactuswriting.toc Delta lines: <Unavailable> File [added]: config.png Delta lines: <Unavailable> File [added]: config.tiff Delta lines: <Unavailable> File [added]: interface1.png Delta lines: <Unavailable> File [added]: interface1.tiff Delta lines: <Unavailable> File [added]: interface2.png Delta lines: <Unavailable> File [added]: interface2.tiff Delta lines: <Unavailable> File [added]: interface3.png Delta lines: <Unavailable> File [added]: interface3.tiff Delta lines: <Unavailable> File [added]: make.png Delta lines: <Unavailable> File [added]: make.tiff Delta lines: <Unavailable> File [added]: param1.png Delta lines: <Unavailable> File [added]: param1.tiff Delta lines: <Unavailable> File [added]: param2.png Delta lines: <Unavailable> File [added]: param2.tiff Delta lines: <Unavailable> File [added]: schedule1.png Delta lines: <Unavailable> File [added]: schedule1.tiff Delta lines: <Unavailable> File [added]: schedule2.png Delta lines: <Unavailable> File [added]: schedule2.tiff Delta lines: <Unavailable> File [added]: schedule3.png Delta lines: <Unavailable> File [added]: schedule3.tiff Delta lines: <Unavailable> File [added]: srccode.png Delta lines: <Unavailable> File [added]: srccode.tiff Delta lines: <Unavailable> File [added]: srccode2.png Delta lines: <Unavailable> File [added]: srccode2.tiff Delta lines: <Unavailable> File [added]: thornlist.png Delta lines: <Unavailable> File [added]: thornlist.tiff Delta lines: <Unavailable>

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[svn:einsteintoolkit] Workshop_Spring_2012/numerical_relativity/ (Rev. 31)
by diener＠cct.lsu.edu 03 Apr '12

03 Apr '12

User: diener Date: 2012/04/03 10:41 PM Modified: /numerical_relativity/ numerical_relativity.tex Log: First slide on MoL. File Changes: Directory: /numerical_relativity/ ================================= File [modified]: numerical_relativity.tex Delta lines: +30 -5 =================================================================== --- numerical_relativity/numerical_relativity.tex 2012-04-04 01:40:55 UTC (rev 30) +++ numerical_relativity/numerical_relativity.tex 2012-04-04 03:41:18 UTC (rev 31) @@ -15,8 +15,8 @@ % \item 3+1 spacetime decomposition. \item The BSSN formulation. \item Puncture data. - \item Finite Differencing. -% \item The method of lines. + \item Finite differencing. + \item The method of lines. \end{itemize} } @@ -214,7 +214,7 @@ that $\psi$ has a unique solution. } -\frame{\frametitle{Finite Differencing} +\frame{\frametitle{Finite differencing} With finite differencing we discretize a function by sampling it at a collection of grid points.\pause @@ -231,7 +231,7 @@ \left. \frac{df}{dx} \right |_{x_i}\approx \frac{1}{\Delta x}\sum_{j=-1}^{j=1} a_j f_{i+j}. \end{equation} } -\frame{\frametitle{Finite Differencing (continued)} +\frame{\frametitle{Finite differencing (continued)} The coefficients $a_j$ can be found be expanding $f$ in a Taylor series around $x_i$ for the grid points in the stencil \begin{eqnarray} @@ -253,7 +253,7 @@ with the solution $a_{-1}=-1/2, a_0=0, a_1=1/2$. } -\frame{\frametitle{Finite Differencing (continued)} +\frame{\frametitle{Finite differencing (continued)} Thus we find that \begin{equation} \left. \frac{df}{dx} \right |_{x_i} = \frac{f_{i+1}-f_{i-1}}{2\Delta x} @@ -276,4 +276,29 @@ It is also clear from either approach that the error estimates are only correct if $f$ is smooth enough. } + +\frame{\frametitle{The method of lines} +Consider the set of hyperbolic PDE's +\begin{equation} +\partial_t \mathbf{q}+\mathbf{A}^i(\mathbf{q})\partial_i +\mathbf{B}(\mathbf{q}) = \mathbf{S}(\mathbf{q}). +\end{equation}\pause +The idea then is to discretize in space first, i.e.\ write the equations as +\begin{equation} +\partial_t \mathbf{q} = \mathbf{L}(\mathbf{q}), +\end{equation} +where $\mathbf{L}(\mathbf{q})$ is a discrete approximation to the equations +(e.g.\ using finite differencing).\pause + +This then turns the equations into a set of coupled ODE's with respect to +time.\pause + +If the spatial discretization (including boundary conditions) is stable +we we can then evolve the system of equations using any stable ODE time +integrator.\pause + +Often Runge-Kutta integration schemes are the scheme of choice. + + +} \end{document}

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[svn:einsteintoolkit] Workshop_Spring_2012/genrel/ (Rev. 30)
by jfaber＠einsteintoolkit.org 03 Apr '12

03 Apr '12

User: jfaber Date: 2012/04/03 08:40 PM Added: /genrel/ covderiv.png, curvtens.png, edmb.jpeg, edmb.png, elevator.jpg, elevator.png, genrel.aux, genrel.log, genrel.nav, genrel.out, genrel.pdf, genrel.snm, genrel.tex, genrel.toc, gwpol, gwpol.png, lapseshift, lapseshift.png, lortrans.png, orbits.jpg, orbits.png, timedilate.png, timedilate.tiff Log: Notes on general relativity File Changes: Directory: /genrel/ =================== File [added]: covderiv.png Delta lines: <Unavailable> File [added]: curvtens.png Delta lines: <Unavailable> File [added]: edmb.jpeg Delta lines: <Unavailable> File [added]: edmb.png Delta lines: <Unavailable> File [added]: elevator.jpg Delta lines: <Unavailable> File [added]: elevator.png Delta lines: <Unavailable> File [added]: genrel.aux Delta lines: <Unavailable> File [added]: genrel.log Delta lines: <Unavailable> File [added]: genrel.nav Delta lines: <Unavailable> File [added]: genrel.out Delta lines: <Unavailable> File [added]: genrel.pdf Delta lines: <Unavailable> File [added]: genrel.snm Delta lines: <Unavailable> File [added]: genrel.tex Delta lines: <Unavailable> File [added]: genrel.toc Delta lines: <Unavailable> File [added]: gwpol Delta lines: <Unavailable> File [added]: gwpol.png Delta lines: <Unavailable> File [added]: lapseshift Delta lines: <Unavailable> File [added]: lapseshift.png Delta lines: <Unavailable> File [added]: lortrans.png Delta lines: <Unavailable> File [added]: orbits.jpg Delta lines: <Unavailable> File [added]: orbits.png Delta lines: <Unavailable> File [added]: timedilate.png Delta lines: <Unavailable> File [added]: timedilate.tiff Delta lines: <Unavailable>

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[svn:einsteintoolkit] Workshop_Spring_2012/numerical_relativity/ (Rev. 29)
by diener＠cct.lsu.edu 03 Apr '12

03 Apr '12

User: diener Date: 2012/04/03 04:52 PM Modified: /numerical_relativity/ numerical_relativity.tex Log: Add some slides on finite differencing. File Changes: Directory: /numerical_relativity/ ================================= File [modified]: numerical_relativity.tex Delta lines: +89 -27 =================================================================== --- numerical_relativity/numerical_relativity.tex 2012-04-03 18:30:44 UTC (rev 28) +++ numerical_relativity/numerical_relativity.tex 2012-04-03 21:52:37 UTC (rev 29) @@ -15,7 +15,7 @@ % \item 3+1 spacetime decomposition. \item The BSSN formulation. \item Puncture data. -% \item Finite Differencing. + \item Finite Differencing. % \item The method of lines. \end{itemize} } @@ -31,33 +31,33 @@ \begin{align} {\cal H} & \equiv R + K^2 - K_{ij} K^{ij} = 0, \\ {\cal M}^i & \equiv D_j (K^{ij} - \gamma^{ij} K) = 0. -\end{align} -These equations were used a lot in the early years of numerical relativity. +\end{align}\pause +These equations were used a lot in the early years of numerical relativity.\pause However, it was later discovered that the ADM evolution equations are only -weakly hyperbolic. +weakly hyperbolic.\pause In the mid to late 90's a new formulation was introduced that proved to be much more robust and stable: The BSSN formulation. } \frame{\frametitle{The BSSN formulation (continued)} -\setlength{\vs}{-1.5ex} +\setlength{\vs}{-0.5ex} Introduce a conformal rescaling of the three metric\vspace{\vs} \begin{equation} \gamma_{ij} = \psi^4 \tg_{ij}.\vspace{\vs} -\end{equation} -We choose $\psi = \gamma^{1/12}$ such that the determinant of $\tg_{ij}$ is 1\vspace{\vs} +\end{equation}\pause +We choose $\psi = \gamma^{1/12}$ such that the determinant of $\tg_{ij}$ is 1%\vspace{\vs} \begin{equation} \mathrm{det}(\tg_{ij}) = \mathrm{det}(\psi^{-4}\gamma_{ij}) = \mathrm{det}(\gamma^{-1/3}\gamma_{ij}) = -\gamma^{-1} \mathrm{det}(\gamma_{ij}) = 1. \vspace{\vs} -\end{equation} +\gamma^{-1} \mathrm{det}(\gamma_{ij}) = 1.\vspace{\vs} +\end{equation}\pause In addition we introduce a trace decomposition of the extrinsic curvature.\vspace{\vs} \begin{align} K & = \gamma^{ij} K_{ij}, \\ A_{ij} & = K_{ij} - \frac{1}{3} \gamma_{ij} K.\vspace{\vs} -\end{align} +\end{align}\pause We then promote the following variables to evolution variables\vspace{\vs} \begin{align} \phi &= \ln \psi = \frac{1}{12} \ln \gamma, @@ -75,16 +75,17 @@ \begin{equation} \tG^i = \tg^{jk} \tG^i{}_{jk} = - \partial_j \tg^{ij}, \end{equation} -to evolved variables as well. +to evolved variables as well.\pause + The final set of evolution variables are $\phi$, $K$, $\tg_{ij}$, $\tA_{ij}$ -and $\tG^i$. +and $\tG^i$.\pause The BSSN evolution equations can be derived from the ADM equations. As an example take the equation for $\phi$. \begin{equation} \dt \phi = \partial_0\phi = \partial_0 \left (\frac{1}{12}\ln\gamma\right) = \frac{1}{12}\frac{1}{\gamma}\partial_0\gamma. -\end{equation} +\end{equation}\pause Using the expression for the derivative of the determinant of the metric in terms of the derivatives of the metric ($\partial_0\gamma = \gamma \gamma^{ij} \partial_0\gamma_{ij}$) we find @@ -114,13 +115,11 @@ & - 2 \tilde{A}^{ij} \partial_j\alpha + 2 \alpha ( \tilde{\Gamma}^i{}_{jk} \tilde{A}^{jk} + 6 \tilde{A}^{ij} \partial_j \phi - \frac{2}{3} \tg^{ij} \partial_j K). -\end{align}%\vspace{\vs} +\end{align} } \frame{\frametitle{The BSSN formulation (continued)} -%\raisebox{-1.2\vs}[0pt][0pt]{ Here $R_{ij} = \tilde{R}_{ij} + R^{\phi}_{ij}$, where\vspace{1.0\vs} -%}\vspace{\vs} \begin{align} R^{\phi}_{ij} = {} & - 2 \tilde{D}_i \tilde{D}_j \phi - 2 \tilde{\gamma}_{ij} @@ -142,18 +141,18 @@ \tilde{{\cal G}} & \equiv \tg-1 = 0, \\ \tilde{{\cal A}} & \equiv \tg^{ij}\tA_{ij} = 0, \\ \tilde{{\cal L}}^{i} & \equiv \tG^{i}+\partial_j\tg^{ij} = 0. -\end{align} +\end{align}\pause The constraints $\tilde{{\cal G}}$ and $\tilde{{\cal A}}$ are enforced actively -at each timestep. +at each timestep.\pause The other constraints ($\tilde{{\cal H}}$, $\tilde{{\cal M}}^i$ and -$\tilde{{\cal L}}^{i}$) are not enforced. +$\tilde{{\cal L}}^{i}$) are not enforced.\pause To improve stability and to help maintain $\tilde{{\cal L}}^{i}$ at a low level the following rule is employed in an implementation \begin{itemize} \item Where derivatives of $\tG^{i}$ are needed the evolved $\tG^{i}$ are used - directly. + directly.\pause \item Where $\tG^{i}$ are needed without taking derivatives $\tg^{jk}\tG^{i}{}_{jk}$ are used instead. \end{itemize} @@ -161,7 +160,7 @@ \frame{\frametitle{The BSSN formulation (continued)} In order to evolve a spacetime with the BSSN equations, you have to specify -the gauges $\alpha$ and $\beta^{i}$. +the gauges $\alpha$ and $\beta^{i}$.\pause Most codes use the ``moving puncture'' gauges \begin{align} @@ -179,12 +178,12 @@ \gamma^{\mathrm{ph}}_{ij} = \psi^4\gamma_{ab}, \mbox{\hspace{2em}} K^{\mathrm{ph}}_{ij} = \psi^{-2} K_{ij}, \end{equation} where $\gamma_{ij}$ is chosen to be the flat metric and $K_{ij}$ is assumed -to be tracefree. \\ +to be tracefree.\pause \\ The constraint equations become\vspace{\vs} \begin{align} 0 & = \Delta\psi +\frac{1}{8}K^{ij}K_{ij}\psi^{-7} \\ 0 & = D_j K^{ij}. -\end{align} +\end{align}\pause The momentum constraint has an analytic solution\vspace{\vs} \begin{align} K^{ij}_{\mathrm{BY}} = {} & \frac{3}{2r^2}\left ( P^i n^j + P^j n^i - @@ -197,21 +196,84 @@ \frame{\frametitle{Puncture data (continued)} \setlength{\vs}{-0.8ex} -For $K_{ij} = 0$ the Hamiltonian constraint has a simple solution for $N$ black holes. +For $K_{ij} = 0$ the Hamiltonian constraint has a simple solution for $N$ +black holes. \begin{equation} \psi = 1+\sum_{i=1}^N\frac{m_i}{2|\vec{r}-\vec{r}_i|}. -\end{equation} +\end{equation}\pause Inspired by this, for $K_{ij}\ne 0$ we make the ansatz \begin{equation} \psi=\frac{1}{\alpha}+u, \mbox{\hspace{2em}} \frac{1}{\alpha} = \sum_{i=1}^N\frac{m_i}{2|\vec{r}-\vec{r}_i|}, -\end{equation} +\end{equation}\pause In which case the Hamiltonian constraint becomes an equation for $u$ \begin{equation} \Delta u+\frac{1}{8}\alpha^7 K^{ij}K_{ij}(1+\alpha u)^{-7} = 0. -\end{equation} +\end{equation}\pause It can be shown that $u$ will be $C^2$ at the location of the `punctures' and that $\psi$ has a unique solution. } +\frame{\frametitle{Finite Differencing} +With finite differencing we discretize a function by sampling it at a +collection of grid points.\pause + +The grid points are usually (but not necessarily) equally spaced. \pause + +We can then approximate derivatives of a function at a grid point by a +weigthed sum of function values at grid points in the neighbourhood (the +stencil) of the grid point. \pause + +As an example consider a stencil containing the grid point ($f_i$) and it's two +nearest neighbors ($f_{i-1}$ and $f_{i+1}$) with +$\Delta x=x_{i+1}-x_i=x_i-x_{i-1}$. +\begin{equation} + \left. \frac{df}{dx} \right |_{x_i}\approx \frac{1}{\Delta x}\sum_{j=-1}^{j=1} a_j f_{i+j}. +\end{equation} +} +\frame{\frametitle{Finite Differencing (continued)} +The coefficients $a_j$ can be found be expanding $f$ in a Taylor series around +$x_i$ for the grid points in the stencil +\begin{eqnarray} +f(x_{i-1}) & = & f(x_i) - \left. \frac{df}{dx}\right |_{x_i} \Delta x + + \frac{1}{2} \left. \frac{d^2 f}{dx^2}\right |_{x_i} \Delta x^2 + + O((\Delta x)^3) \nonumber \\ +f(x_i) & = & f(x_i) \nonumber \\ +f(x_{i+1}) & = & f(x_i) + \left. \frac{df}{dx}\right |_{x_i} \Delta x + + \frac{1}{2} \left. \frac{d^2 f}{dx^2}\right |_{x_i} \Delta x^2 + + O((\Delta x)^3) \nonumber +\end{eqnarray} \pause +Requiring that the weighted sum approximates the derivative yields +the following equations for $a_{-1}$, $a_0$ and $a_1$ +\begin{eqnarray} +0 & = & a_{-1}+a_0+a_1 \nonumber \\ +1 & = & -a_{-1}+a_1 \nonumber \\ +0 & = & a_{-1}+a_1 \nonumber +\end{eqnarray} +with the solution $a_{-1}=-1/2, a_0=0, a_1=1/2$. +} + +\frame{\frametitle{Finite Differencing (continued)} +Thus we find that +\begin{equation} +\left. \frac{df}{dx} \right |_{x_i} = \frac{f_{i+1}-f_{i-1}}{2\Delta x} + + O((\Delta x)^2). +\end{equation}\pause +Similarly we find for the second derivative that +\begin{equation} +\left. \frac{d^2f}{dx^2} \right |_{x_i} = \frac{f_{i+1}-2 f_i+f_{i-1}}{(\Delta x)^2} + + O((\Delta x)^2). +\end{equation}\pause +These finite difference operators are second order accurate.\pause + +Higher order accuracy or higher order derivatives require larger stencils.\pause + +Another way of looking at finite differencing operators is through +interpolating polynomials.\pause + +Either approach gives the same coefficients for the same stencil.\pause + +It is also clear from either approach that the error estimates are only +correct if $f$ is smooth enough. +} \end{document}

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[McLachlan]McLachlan branch, master, updated. af04ce2e3d96d19b94dd4b416a6617b649c6da34
by Carpet git repositories 03 Apr '12

03 Apr '12

This is an automated email from the git hooks/post-receive script. It was generated because a ref change was pushed to the repository containing the project "McLachlan". The branch, master has been updated via af04ce2e3d96d19b94dd4b416a6617b649c6da34 (commit) from 6a60c4578abcd30d8fc60904ba275ec2e21133a5 (commit) Those revisions listed above that are new to this repository have not appeared on any other notification email; so we list those revisions in full, below. - Log ----------------------------------------------------------------- commit af04ce2e3d96d19b94dd4b416a6617b649c6da34 Author: Erik Schnetter <schnetter(a)gmail.com> Date: Tue Apr 3 16:05:18 2012 -0400 Regenerate code with current version of Kranc This is necessary so that Pi is correctly vectorized. ----------------------------------------------------------------------- Summary of changes: ML_ADMConstraints/schedule.ccl | 21 ++- ML_ADMConstraints/src/ML_ADMConstraints.cc | 22 +- ML_ADMConstraints/src/make.code.defn | 2 +- ML_ADMConstraints_MP/schedule.ccl | 21 ++- ML_ADMConstraints_MP/src/ML_ADMConstraints_MP.cc | 22 +- ML_ADMConstraints_MP/src/make.code.defn | 2 +- ML_ADMConstraints_O2/schedule.ccl | 21 ++- ML_ADMConstraints_O2/src/ML_ADMConstraints_O2.cc | 22 +- ML_ADMConstraints_O2/src/make.code.defn | 2 +- ML_ADMQuantities/schedule.ccl | 26 ++- ML_ADMQuantities/src/ML_ADMQuantities.cc | 27 ++- ML_ADMQuantities/src/make.code.defn | 2 +- ML_ADMQuantities_MP/schedule.ccl | 26 ++- ML_ADMQuantities_MP/src/ML_ADMQuantities_MP.cc | 27 ++- ML_ADMQuantities_MP/src/make.code.defn | 2 +- ML_ADMQuantities_O2/schedule.ccl | 26 ++- ML_ADMQuantities_O2/src/ML_ADMQuantities_O2.cc | 27 ++- ML_ADMQuantities_O2/src/make.code.defn | 2 +- ML_BSSN/schedule.ccl | 237 +++++++++++++++++++- ML_BSSN/src/ML_BSSN_Advect.cc | 203 +++++------------ ML_BSSN/src/ML_BSSN_Dissipation.cc | 203 +++++------------ ML_BSSN/src/ML_BSSN_InitGamma.cc | 98 +++------ ML_BSSN/src/ML_BSSN_InitRHS.cc | 194 +++++------------ ML_BSSN/src/ML_BSSN_Minkowski.cc | 194 +++++------------ ML_BSSN/src/ML_BSSN_RHS1.cc | 182 +++++---------- ML_BSSN/src/ML_BSSN_RHS2.cc | 112 ++++------ ML_BSSN/src/ML_BSSN_RHSStaticBoundary.cc | 194 +++++------------ ML_BSSN/src/ML_BSSN_boundary.cc | 194 +++++------------ ML_BSSN/src/ML_BSSN_constraints1.cc | 75 +++---- ML_BSSN/src/ML_BSSN_constraints2.cc | 117 ++++------- ML_BSSN/src/ML_BSSN_convertFromADMBase.cc | 160 ++++---------- ML_BSSN/src/ML_BSSN_convertFromADMBaseGamma.cc | 111 +++------ ML_BSSN/src/ML_BSSN_convertToADMBase.cc | 150 ++++--------- .../src/ML_BSSN_convertToADMBaseDtLapseShift.cc | 92 +++----- ...ML_BSSN_convertToADMBaseDtLapseShiftBoundary.cc | 90 +++----- .../ML_BSSN_convertToADMBaseFakeDtLapseShift.cc | 90 +++----- ML_BSSN/src/ML_BSSN_enforce.cc | 98 +++------ ML_BSSN/src/make.code.defn | 2 +- ML_BSSN_MP/schedule.ccl | 237 +++++++++++++++++++- ML_BSSN_MP/src/ML_BSSN_MP_Advect.cc | 203 +++++------------ ML_BSSN_MP/src/ML_BSSN_MP_Dissipation.cc | 203 +++++------------ ML_BSSN_MP/src/ML_BSSN_MP_InitGamma.cc | 98 +++------ ML_BSSN_MP/src/ML_BSSN_MP_InitRHS.cc | 194 +++++------------ ML_BSSN_MP/src/ML_BSSN_MP_Minkowski.cc | 194 +++++------------ ML_BSSN_MP/src/ML_BSSN_MP_RHS1.cc | 182 +++++---------- ML_BSSN_MP/src/ML_BSSN_MP_RHS2.cc | 112 ++++------ ML_BSSN_MP/src/ML_BSSN_MP_RHSStaticBoundary.cc | 194 +++++------------ ML_BSSN_MP/src/ML_BSSN_MP_boundary.cc | 194 +++++------------ ML_BSSN_MP/src/ML_BSSN_MP_constraints1.cc | 75 +++---- ML_BSSN_MP/src/ML_BSSN_MP_constraints2.cc | 117 ++++------- ML_BSSN_MP/src/ML_BSSN_MP_convertFromADMBase.cc | 160 ++++---------- .../src/ML_BSSN_MP_convertFromADMBaseGamma.cc | 111 +++------ ML_BSSN_MP/src/ML_BSSN_MP_convertToADMBase.cc | 150 ++++--------- .../src/ML_BSSN_MP_convertToADMBaseDtLapseShift.cc | 92 +++----- ...BSSN_MP_convertToADMBaseDtLapseShiftBoundary.cc | 90 +++----- .../ML_BSSN_MP_convertToADMBaseFakeDtLapseShift.cc | 90 +++----- ML_BSSN_MP/src/ML_BSSN_MP_enforce.cc | 98 +++------ ML_BSSN_MP/src/make.code.defn | 2 +- ML_BSSN_MP_O8/schedule.ccl | 237 +++++++++++++++++++- ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_Advect.cc | 203 +++++------------ ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_Dissipation.cc | 203 +++++------------ ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_InitGamma.cc | 98 +++------ ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_InitRHS.cc | 194 +++++------------ ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_Minkowski.cc | 194 +++++------------ ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_RHS1.cc | 182 +++++---------- ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_RHS2.cc | 112 ++++------ .../src/ML_BSSN_MP_O8_RHSStaticBoundary.cc | 194 +++++------------ ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_boundary.cc | 194 +++++------------ ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_constraints1.cc | 75 +++---- ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_constraints2.cc | 117 ++++------- .../src/ML_BSSN_MP_O8_convertFromADMBase.cc | 160 ++++---------- .../src/ML_BSSN_MP_O8_convertFromADMBaseGamma.cc | 111 +++------ .../src/ML_BSSN_MP_O8_convertToADMBase.cc | 150 ++++--------- .../ML_BSSN_MP_O8_convertToADMBaseDtLapseShift.cc | 92 +++----- ...N_MP_O8_convertToADMBaseDtLapseShiftBoundary.cc | 90 +++----- ..._BSSN_MP_O8_convertToADMBaseFakeDtLapseShift.cc | 90 +++----- ML_BSSN_MP_O8/src/ML_BSSN_MP_O8_enforce.cc | 98 +++------ ML_BSSN_MP_O8/src/make.code.defn | 2 +- ML_BSSN_O2/schedule.ccl | 237 +++++++++++++++++++- ML_BSSN_O2/src/ML_BSSN_O2_Advect.cc | 203 +++++------------ ML_BSSN_O2/src/ML_BSSN_O2_Dissipation.cc | 203 +++++------------ ML_BSSN_O2/src/ML_BSSN_O2_InitGamma.cc | 98 +++------ ML_BSSN_O2/src/ML_BSSN_O2_InitRHS.cc | 194 +++++------------ ML_BSSN_O2/src/ML_BSSN_O2_Minkowski.cc | 194 +++++------------ ML_BSSN_O2/src/ML_BSSN_O2_RHS1.cc | 182 +++++---------- ML_BSSN_O2/src/ML_BSSN_O2_RHS2.cc | 112 ++++------ ML_BSSN_O2/src/ML_BSSN_O2_RHSStaticBoundary.cc | 194 +++++------------ ML_BSSN_O2/src/ML_BSSN_O2_boundary.cc | 194 +++++------------ ML_BSSN_O2/src/ML_BSSN_O2_constraints1.cc | 75 +++---- ML_BSSN_O2/src/ML_BSSN_O2_constraints2.cc | 117 ++++------- ML_BSSN_O2/src/ML_BSSN_O2_convertFromADMBase.cc | 160 ++++---------- .../src/ML_BSSN_O2_convertFromADMBaseGamma.cc | 111 +++------ ML_BSSN_O2/src/ML_BSSN_O2_convertToADMBase.cc | 150 ++++--------- .../src/ML_BSSN_O2_convertToADMBaseDtLapseShift.cc | 92 +++----- ...BSSN_O2_convertToADMBaseDtLapseShiftBoundary.cc | 90 +++----- .../ML_BSSN_O2_convertToADMBaseFakeDtLapseShift.cc | 90 +++----- ML_BSSN_O2/src/ML_BSSN_O2_enforce.cc | 98 +++------ ML_BSSN_O2/src/make.code.defn | 2 +- ML_BSSN_O8/schedule.ccl | 237 +++++++++++++++++++- ML_BSSN_O8/src/ML_BSSN_O8_Advect.cc | 203 +++++------------ ML_BSSN_O8/src/ML_BSSN_O8_Dissipation.cc | 203 +++++------------ ML_BSSN_O8/src/ML_BSSN_O8_InitGamma.cc | 98 +++------ ML_BSSN_O8/src/ML_BSSN_O8_InitRHS.cc | 194 +++++------------ ML_BSSN_O8/src/ML_BSSN_O8_Minkowski.cc | 194 +++++------------ ML_BSSN_O8/src/ML_BSSN_O8_RHS1.cc | 182 +++++---------- ML_BSSN_O8/src/ML_BSSN_O8_RHS2.cc | 112 ++++------ ML_BSSN_O8/src/ML_BSSN_O8_RHSStaticBoundary.cc | 194 +++++------------ ML_BSSN_O8/src/ML_BSSN_O8_boundary.cc | 194 +++++------------ ML_BSSN_O8/src/ML_BSSN_O8_constraints1.cc | 75 +++---- ML_BSSN_O8/src/ML_BSSN_O8_constraints2.cc | 117 ++++------- ML_BSSN_O8/src/ML_BSSN_O8_convertFromADMBase.cc | 160 ++++---------- .../src/ML_BSSN_O8_convertFromADMBaseGamma.cc | 111 +++------ ML_BSSN_O8/src/ML_BSSN_O8_convertToADMBase.cc | 150 ++++--------- .../src/ML_BSSN_O8_convertToADMBaseDtLapseShift.cc | 92 +++----- ...BSSN_O8_convertToADMBaseDtLapseShiftBoundary.cc | 90 +++----- .../ML_BSSN_O8_convertToADMBaseFakeDtLapseShift.cc | 90 +++----- ML_BSSN_O8/src/ML_BSSN_O8_enforce.cc | 98 +++------ ML_BSSN_O8/src/make.code.defn | 2 +- ML_BSSN_UPW/schedule.ccl | 237 +++++++++++++++++++- ML_BSSN_UPW/src/ML_BSSN_UPW_Advect.cc | 203 +++++------------ ML_BSSN_UPW/src/ML_BSSN_UPW_Dissipation.cc | 203 +++++------------ ML_BSSN_UPW/src/ML_BSSN_UPW_InitGamma.cc | 98 +++------ ML_BSSN_UPW/src/ML_BSSN_UPW_InitRHS.cc | 194 +++++------------ ML_BSSN_UPW/src/ML_BSSN_UPW_Minkowski.cc | 194 +++++------------ ML_BSSN_UPW/src/ML_BSSN_UPW_RHS1.cc | 182 +++++---------- ML_BSSN_UPW/src/ML_BSSN_UPW_RHS2.cc | 112 ++++------ ML_BSSN_UPW/src/ML_BSSN_UPW_RHSStaticBoundary.cc | 194 +++++------------ ML_BSSN_UPW/src/ML_BSSN_UPW_boundary.cc | 194 +++++------------ ML_BSSN_UPW/src/ML_BSSN_UPW_constraints1.cc | 75 +++---- ML_BSSN_UPW/src/ML_BSSN_UPW_constraints2.cc | 117 ++++------- ML_BSSN_UPW/src/ML_BSSN_UPW_convertFromADMBase.cc | 160 ++++---------- .../src/ML_BSSN_UPW_convertFromADMBaseGamma.cc | 111 +++------ ML_BSSN_UPW/src/ML_BSSN_UPW_convertToADMBase.cc | 150 ++++--------- .../ML_BSSN_UPW_convertToADMBaseDtLapseShift.cc | 92 +++----- ...SSN_UPW_convertToADMBaseDtLapseShiftBoundary.cc | 90 +++----- ...ML_BSSN_UPW_convertToADMBaseFakeDtLapseShift.cc | 90 +++----- ML_BSSN_UPW/src/ML_BSSN_UPW_enforce.cc | 98 +++------ ML_BSSN_UPW/src/make.code.defn | 2 +- ML_WaveToy/schedule.ccl | 22 ++- ML_WaveToy/src/WT_Gaussian.cc | 18 +- ML_WaveToy/src/WT_RHS.cc | 20 +- ML_WaveToy/src/make.code.defn | 2 +- ML_hydro/schedule.ccl | 45 ++++- ML_hydro/src/hydro_RHS.cc | 22 +- ML_hydro/src/hydro_con2prim.cc | 24 ++- ML_hydro/src/hydro_prim2con.cc | 23 ++- ML_hydro/src/hydro_soundWave.cc | 26 ++- ML_hydro/src/hydro_vacuum.cc | 19 +- ML_hydro/src/make.code.defn | 2 +- 149 files changed, 6413 insertions(+), 10886 deletions(-) hooks/post-receive -- McLachlan

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[svn:einsteintoolkit] Workshop_Spring_2012/handson_analysis/ (Rev. 28)
by roland.haas＠physics.gatech.edu 03 Apr '12

03 Apr '12

User: rhaas Date: 2012/04/03 01:30 PM Modified: /handson_analysis/ handson_analysis.tex Log: add word "global" to algorithm outline File Changes: Directory: /handson_analysis/ ============================= File [modified]: handson_analysis.tex Delta lines: +3 -2 =================================================================== --- handson_analysis/handson_analysis.tex 2012-04-03 18:06:07 UTC (rev 27) +++ handson_analysis/handson_analysis.tex 2012-04-03 18:30:44 UTC (rev 28) @@ -112,7 +112,7 @@ core\_density[idx] = 0.; \} \end{alltt} -\item<3-> \texttt{CCTK\_ANALYSIS} compute \texttt{sum} reduction on integrand +\item<3-> \texttt{CCTK\_ANALYSIS} compute global \texttt{sum} reduction on integrand \begin{alltt}\color{blue} CCTK\_Reduce(cctkGH, -1, handle\_sum, 1, CCTK\_VARIABLE\_REAL, core\_x, 1, varindex); @@ -121,7 +121,7 @@ \end{frame} \begin{frame}[fragile] - \frametitle{Useful functions} + \frametitle{Useful functions/Notes} \begin{itemize} \item Section C1.7.4 of User Guide \url{http://einsteintoolkit.org/documentation/UsersGuide/UsersGuidech9.html#x13-116000C1.7.4} \item[] @@ -135,6 +135,7 @@ int num\_in\_fields, ...); \end{alltt} + \item Reductions should be called in global mode \end{itemize} \end{frame} \end{document}

1 0

[svn:einsteintoolkit] Workshop_Spring_2012/handson_analysis/ (Rev. 27)
by roland.haas＠physics.gatech.edu 03 Apr '12

03 Apr '12

User: rhaas Date: 2012/04/03 01:06 PM Modified: /handson_analysis/ handson_analysis.tex Log: add prototype of CCTK_Reduce (from UserGuide) to analysis_handson File Changes: Directory: /handson_analysis/ ============================= File [modified]: handson_analysis.tex Delta lines: +20 -1 =================================================================== --- handson_analysis/handson_analysis.tex 2012-04-02 21:39:51 UTC (rev 26) +++ handson_analysis/handson_analysis.tex 2012-04-03 18:06:07 UTC (rev 27) @@ -67,7 +67,8 @@ \begin{block}{Does this fit into code?} Certainly. \begin{itemize} - \item $\int$ $\rightarrow$ $\sum_{i,j,k} \text{grid-points}$ + \item $\int$ $\rightarrow$ + \parbox{.75\linewidth}{\begin{alltt}core\_density\_x[idx] = \ldots;\\\vdots\\CCTK\_Reduce(\ldots,handle\_sum,\ldots,core\_density\_x,\ldots);\end{alltt}} \item $\Heaviside$ $\rightarrow$ \verb|if(...)| \end{itemize} \end{block} @@ -118,4 +119,22 @@ \end{alltt} \end{itemize} \end{frame} + +\begin{frame}[fragile] + \frametitle{Useful functions} + \begin{itemize} + \item Section C1.7.4 of User Guide \url{http://einsteintoolkit.org/documentation/UsersGuide/UsersGuidech9.html#x13-116000C1.7.4} + \item[] + \begin{alltt}\color{blue} +int CCTK\_Reduce(const cGH *GH, + int proc, + int operation\_handle, + int num\_out\_vals, + int type\_out\_vals, + void *out\_vals, + int num\_in\_fields, + ...); + \end{alltt} + \end{itemize} +\end{frame} \end{document}

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[McLachlan]McLachlan branch, cakernel, updated. 5b5b744ad8ec5b7627c84c236f0f3ae4f01b8d07
by Carpet git repositories 03 Apr '12

03 Apr '12

This is an automated email from the git hooks/post-receive script. It was generated because a ref change was pushed to the repository containing the project "McLachlan". The branch, cakernel has been updated via 5b5b744ad8ec5b7627c84c236f0f3ae4f01b8d07 (commit) via 56cea2adf29ca0223b53581313841c86ca8b5ac9 (commit) via 20021c93bc314c539eb061a1c43e8457cd29141c (commit) via d66498b9c4a15bc18549627364a0989af83204d3 (commit) via 581b31365c65653c114ba5befc20f7befe36bf15 (commit) from 7a226e25dcd3d87a753866fa7a1411da98fc27f2 (commit) Those revisions listed above that are new to this repository have not appeared on any other notification email; so we list those revisions in full, below. - Log ----------------------------------------------------------------- commit 5b5b744ad8ec5b7627c84c236f0f3ae4f01b8d07 Author: Ian Hinder <ian.hinder(a)aei.mpg.de> Date: Tue Apr 3 16:02:22 2012 +0200 Regenerate ML_BSSN and ML_BSSN_Host commit 56cea2adf29ca0223b53581313841c86ca8b5ac9 Author: Ian Hinder <ian.hinder(a)aei.mpg.de> Date: Tue Apr 3 16:01:55 2012 +0200 McLachlan_BSSN.m: Compute all derivatives in RHS calculation in separate calculations and gridfunctions commit 20021c93bc314c539eb061a1c43e8457cd29141c Author: Ian Hinder <ian.hinder(a)aei.mpg.de> Date: Tue Apr 3 15:30:07 2012 +0200 Regenerate ML_BSSN and ML_BSSN_Host commit d66498b9c4a15bc18549627364a0989af83204d3 Author: Ian Hinder <ian.hinder(a)aei.mpg.de> Date: Tue Apr 3 15:21:33 2012 +0200 McLachlan_BSSN.m: Calculate mixed second derivatives in a separate calculation and store them in grid functions commit 581b31365c65653c114ba5befc20f7befe36bf15 Author: Ian Hinder <ian.hinder(a)aei.mpg.de> Date: Tue Apr 3 11:13:34 2012 +0200 McLachlan_BSSN.m: Use Kranc for all equation calculation splitting and remove splitting code from McLachlan No change to generated code ----------------------------------------------------------------------- Summary of changes: ML_BSSN/cakernel.ccl | 3417 ++++++++++++++++++-- ML_BSSN/interface.ccl | 666 ++++ ML_BSSN/param.ccl | 1458 ++++++++- ML_BSSN/schedule.ccl | 2102 +++++++++++-- ML_BSSN/src/CaKernel__ML_BSSN_Advect_Arhs.code | 121 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_At11rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_At12rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_At13rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_At22rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_At23rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_At33rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_B1rhs.code | 121 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_B2rhs.code | 121 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_B3rhs.code | 121 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_Xt1rhs.code | 110 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_Xt2rhs.code | 110 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_Xt3rhs.code | 110 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_alpharhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_beta1rhs.code | 110 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_beta2rhs.code | 110 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_beta3rhs.code | 110 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotA.code | 121 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotAt11.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotAt12.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotAt13.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotAt22.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotAt23.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotAt33.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotB1.code | 121 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotB2.code | 121 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotB3.code | 121 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotXt1.code | 110 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotXt2.code | 110 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotXt3.code | 110 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotalpha.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotbeta1.code | 110 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotbeta2.code | 110 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotbeta3.code | 110 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotgt11.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotgt12.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotgt13.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotgt22.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotgt23.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotgt33.code | 111 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dotphi.code | 110 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_dottrK.code | 110 - ML_BSSN/src/CaKernel__ML_BSSN_Advect_gt11rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_gt12rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_gt13rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_gt22rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_gt23rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_gt33rhs.code | 111 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_phirhs.code | 110 + ML_BSSN/src/CaKernel__ML_BSSN_Advect_trKrhs.code | 110 + ML_BSSN/src/CaKernel__ML_BSSN_RHS1.code | 446 ++-- ML_BSSN/src/CaKernel__ML_BSSN_RHS2.code | 526 ++-- .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt11.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt12.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt13.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt21.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt22.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt23.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt31.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt32.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthXt33.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthalpha1.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthalpha11.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthalpha12.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthalpha13.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthalpha2.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthalpha22.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthalpha23.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthalpha3.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthalpha33.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta11.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta111.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta112.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta113.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta12.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta122.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta123.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta13.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta133.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta21.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta211.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta212.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta213.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta22.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta222.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta223.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta23.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta233.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta31.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta311.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta312.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta313.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta32.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta322.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta323.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthbeta33.code | 92 + ...aKernel__ML_BSSN_RHS_DPDstandardNthbeta333.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthgt111.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1111.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1112.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1113.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthgt112.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1122.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1123.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthgt113.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1133.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthgt121.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1211.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1212.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1213.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthgt122.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1222.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1223.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthgt123.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1233.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthgt131.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1311.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1312.code | 92 + ...CaKernel__ML_BSSN_RHS_DPDstandardNthgt1313.code | 92 + .../CaKernel__ML_BSSN_RHS_DPDstandardNthgt132.code | 92 + 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ML_BSSN_Host/src/ML_BSSN_Host_Advect_At23rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_At33rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_B1rhs.cc | 184 ++ ML_BSSN_Host/src/ML_BSSN_Host_Advect_B2rhs.cc | 184 ++ ML_BSSN_Host/src/ML_BSSN_Host_Advect_B3rhs.cc | 184 ++ ML_BSSN_Host/src/ML_BSSN_Host_Advect_Xt1rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_Xt2rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_Xt3rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_alpharhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_beta1rhs.cc | 174 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_beta2rhs.cc | 174 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_beta3rhs.cc | 174 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotA.cc | 184 -- ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotAt11.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotAt12.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotAt13.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotAt22.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotAt23.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotAt33.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotB1.cc | 184 -- ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotB2.cc | 184 -- ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotB3.cc | 184 -- ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotXt1.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotXt2.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotXt3.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotalpha.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotbeta1.cc | 174 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotbeta2.cc | 174 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotbeta3.cc | 174 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotgt11.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotgt12.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotgt13.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotgt22.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotgt23.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotgt33.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dotphi.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_dottrK.cc | 176 - ML_BSSN_Host/src/ML_BSSN_Host_Advect_gt11rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_gt12rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_gt13rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_gt22rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_gt23rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_gt33rhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_phirhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_Advect_trKrhs.cc | 176 + ML_BSSN_Host/src/ML_BSSN_Host_RHS1.cc | 253 +- ML_BSSN_Host/src/ML_BSSN_Host_RHS2.cc | 367 ++- .../src/ML_BSSN_Host_RHS_DPDstandardNthXt11.cc | 159 + .../src/ML_BSSN_Host_RHS_DPDstandardNthXt12.cc | 159 + .../src/ML_BSSN_Host_RHS_DPDstandardNthXt13.cc | 159 + .../src/ML_BSSN_Host_RHS_DPDstandardNthXt21.cc | 159 + .../src/ML_BSSN_Host_RHS_DPDstandardNthXt22.cc | 159 + .../src/ML_BSSN_Host_RHS_DPDstandardNthXt23.cc | 159 + 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ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthgt3333.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi1.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi11.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi12.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi13.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi2.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi22.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi23.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi3.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthphi33.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthtrK1.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthtrK2.cc create mode 100644 ML_BSSN_Host/src/ML_BSSN_Host_RHS_DPDstandardNthtrK3.cc hooks/post-receive -- McLachlan

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