| Commit message (Collapse) | Author | Age |
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compile-time warning since
poloidal ID B-field routine is not yet adapted to MP.
From: Christian Reisswig <reisswig@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@215 ac85fae7-cede-4708-beff-ae01c7fa1c26
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make sense
From: Roland Haas <rhaas@caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@210 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@209 ac85fae7-cede-4708-beff-ae01c7fa1c26
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tie Gamma value used to that of eos_omni's gamma law eos
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@208 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@206 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@205 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: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@202 ac85fae7-cede-4708-beff-ae01c7fa1c26
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later on prim2con will of course compute the grid function using vel
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@201 ac85fae7-cede-4708-beff-ae01c7fa1c26
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was used to call the newton solver twice with the very same arguments.
Not sure what the idea was.
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@200 ac85fae7-cede-4708-beff-ae01c7fa1c26
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this is mostly important when we freeze the evolution afterwards
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@199 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@198 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@197 ac85fae7-cede-4708-beff-ae01c7fa1c26
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r_code = r_KS - r0 with r0=1M by default. This avoids placing the
central singularity on the grid.
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@196 ac85fae7-cede-4708-beff-ae01c7fa1c26
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Initial Avec constrained to poloidal at the moment.
From: Tanja Bode <tanja.bode@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@195 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Tanja Bode <tanja.bode@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@194 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@193 ac85fae7-cede-4708-beff-ae01c7fa1c26
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to test inversions in the gr context.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@192 ac85fae7-cede-4708-beff-ae01c7fa1c26
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to make sure Exact's spacetime metric is consistent with the one
internally used by the Bondi solution
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@191 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@190 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@189 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@188 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@187 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@186 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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From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@184 ac85fae7-cede-4708-beff-ae01c7fa1c26
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this is so that there is a proper initial_bvec setting rather than just
"zero".
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@183 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@182 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@181 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@180 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@179 ac85fae7-cede-4708-beff-ae01c7fa1c26
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and improve smoothing of v field.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@178 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@177 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@176 ac85fae7-cede-4708-beff-ae01c7fa1c26
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this avoids having to rely on GRHydro_InitData running after HydroBase's
ZeroBvec routine in order to have non-zero magnetic field
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@173 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@172 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@171 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: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@167 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@166 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@165 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@164 ac85fae7-cede-4708-beff-ae01c7fa1c26
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SmoothedPuncture thorn
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@163 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@162 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@157 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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evolved or not evolved.
From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@154 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@152 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@151 ac85fae7-cede-4708-beff-ae01c7fa1c26
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