| Commit message (Collapse) | Author | Age |
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@216 ac85fae7-cede-4708-beff-ae01c7fa1c26
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* Tested successfully pointwisely. It still needs to be tested on evolution.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@204 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Josh Faber <jfaberrit@jfaber3.local>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@185 ac85fae7-cede-4708-beff-ae01c7fa1c26
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* There are still a lot of committed tab characters in the code.
I will try to slowly clean that up. Meanwhile, please teach your
text editor to transform tab characters into equivalent blank spaces
before saving file to disk. This avoids code looking unformatted
to other users due to different personal or default text editor settings
for tab characters..
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@168 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Christian Ott <cott@bethe.tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@156 ac85fae7-cede-4708-beff-ae01c7fa1c26
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1) Switch to EOSOmni pointwise C2P routine and modify where necessary.
2) Modify Con2PrimM.F90 to allow for the evolution of temperature and adjust the wrapper routine.
3) Create EigenProblemM_hot pointwise routine and call that from HLLEM.F90 when temperature is evolved.
Additionally adjust HLLEM where necessary.
4) Adjust InterfacesM.h to incorporate the newly created functions.
5) Fix a loop problem (not taking into account constraint transport) in PPM reconstruction of Y_e
6) Introduce Prim2ConM_hot and call this pointwise routine from Prim2ConM.F90 when temperature is evolved.
Additionally also make this routine available to initial data routine in GRHydro_InitData
7) Adjust loops in GRHydro_PoloidalMagFieldM.F90 to not set boundary points it cannot set but instead call boundary group afterwards! Pay attention as this will not work with boundary conditions set to "none" in MHD case anymore but is the correct thing to do.
8) Allow StarMapper to extend HydroBase::initial_hydro = "starmapper".
9) Smaller fixes.
From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@153 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@131 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@126 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@125 ac85fae7-cede-4708-beff-ae01c7fa1c26
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EOS Omni interface.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@119 ac85fae7-cede-4708-beff-ae01c7fa1c26
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Add #include "cctk_Functions.h" and DECLARE_CCTK_FUNCTIONS
to GRHydro_C2P2CM.F90.
Solve several issues of rank mismatch in the EOS Omni
interface.
Initialize the velocities at GRHydro_C2P2CM.F90 since
GRHydro_Con2PrimM_pt.c uses past values as initial guess
for its Newton-Raphson procedure. These unitialized values
were causing C2P2CM to fail from time to time, since it
would access memory positions with very large numerical
values, i.e. v>>1. C2P2CM test always passes now.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@118 ac85fae7-cede-4708-beff-ae01c7fa1c26
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and vice versa.
Add the magnetized version for the ShockTube routine.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@114 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@113 ac85fae7-cede-4708-beff-ae01c7fa1c26
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* correct syntax in F90 files
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@112 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@106 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@89 ac85fae7-cede-4708-beff-ae01c7fa1c26
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code right now. I have put in the public version of Whisky to start from.
Everybody with commit rights should get commit messages (and the other
way around). It should not be a problem to add people to that list, just
ask. I don't want to get into political problems because someone feels
excluded, but I also don't want to give everyone access per se.
Frank
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@3 ac85fae7-cede-4708-beff-ae01c7fa1c26
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