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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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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@161 ac85fae7-cede-4708-beff-ae01c7fa1c26
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Since commit 454e99d6a717433c523ec7074302fc1fc7c01dbe it is not possible
to run SRMHD tests anymore without assigning storage to Tmunu.
This commit change changes advectedloop3D.par to reflect that and suggests
a possible solution in GRHydro/src/GRHydro_RegisterVars.cc. This solution
doesn't work yet due to inadequate scheduling. A trac ticket will be
filed soon to discuss this issue more broadly.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@160 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@159 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@158 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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rather than defining a private parameter of the same name.
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@155 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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including used-defined pressure (to alter wavespeed) and oblique case
From: Josh Faber <jfaberrit@jfaber3.local>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@150 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@149 ac85fae7-cede-4708-beff-ae01c7fa1c26
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Signed-off-by: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@148 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@147 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@146 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@145 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@144 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@143 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Josh Faber <jfaberrit@jafsmamacbook.main.ad.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@142 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@141 ac85fae7-cede-4708-beff-ae01c7fa1c26
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* don't access 2d array as 1d array through second index
* always assign something to rho_guess in Bondi solution
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@140 ac85fae7-cede-4708-beff-ae01c7fa1c26
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* cite paper with description of system
* reverse sense of rotation
* add openmp statements
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@139 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@138 ac85fae7-cede-4708-beff-ae01c7fa1c26
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1) Calculate divergence of B in MoL PseudoEvolution and set its Prolongation="Restrict".
2) Correct the source terms and fluxes for the Bfield and the divergence cleaning field when having a non-flat space-time.
3) Make sure alpha factors match between UpdateCalculation and fluxes definition.
4) Include 1/sqrt(detg) factor in calculation of \epsilon^{\muijk} in the cross product to obtain the Bfield form the vector potential.
From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@137 ac85fae7-cede-4708-beff-ae01c7fa1c26
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From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@136 ac85fae7-cede-4708-beff-ae01c7fa1c26
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* The 2d diagonal boundary conditions are correctly applied
when using multiprocessors.
* The ymin (ymax) surfaces have their points in the region
indsum < minsum (indsum > maxsum) fixed after a first sync
operation. A second sync guarantees the neighbour grid
receives the correct value of the boundary on those regions.
* Mirror symmetries applied at the faces intercepting the upper
right corner assumed cubic local domain. However, rectangular
local domains are common after domain decomposition. This commit
fixes the indexes applying this symmetry for these cases.
* Upper right corner/edge/surface condition should use sten instead
of stenp1. Thanks for catching this Josh!
* Attempt at a 3d diagonal boundary treatment (Josh's commit)
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@135 ac85fae7-cede-4708-beff-ae01c7fa1c26
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added.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@134 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@132 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@128 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@127 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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1) Komissarov's cylindrical explosion test
2) Magnetic monopole test
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@124 ac85fae7-cede-4708-beff-ae01c7fa1c26
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Balsara's and Komissarov's shock tube tests.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@123 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@121 ac85fae7-cede-4708-beff-ae01c7fa1c26
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@120 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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Update initial data routines to properly call out pressures and other
hydro quantities using EOS_Omni rather than now-defunct interfaces.
Add C2P_polytype interface.
Un-hardwire fixed values of gamma for all MHD Con2Prim routines.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@117 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@111 ac85fae7-cede-4708-beff-ae01c7fa1c26
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