aboutsummaryrefslogtreecommitdiff
path: root/schedule.ccl
Commit message (Collapse)AuthorAge
* GRHydro_InitData: Reschedule to make things work with multipatch. Spit out a ↵rhaas2013-07-06
| | | | | | | | | | 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
* GRHydro_Init_Data: add routine to force boundary data to Bondirhaas2013-03-28
| | | | | | 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
* GRHydro: add parameters to set Bondi solution only in certain range.rhaas2013-03-28
| | | | | | 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
* GRHydro_InitData: Add basic vector potential supportrhaas2013-01-11
| | | | | | | | 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
* Get rid of (some) tab charactersrhaas2012-09-17
| | | | | | | | | | | | | * 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
* * add a hot shocktube to run shocktube tests with the nuclear EOSrhaas2012-09-04
| | | | | | 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
* GRHydro_InitData: extent initial_Bvecrhaas2012-09-04
| | | | | | | | 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
* Changes to make GRHydro MHD work with nuclear/hot equation of state:rhaas2012-09-04
| | | | | | | | | | | | | | | | | | 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
* Introduce a better treatment of the shocktube boundaries.rhaas2012-08-09
| | | | | | | | | | | | | | | | | | | | | | * 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
* Snapshot of ET GRHydro_InitData rev. 132 with a poloidal magnetic field routinerhaas2012-08-09
| | | | | | added. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@134 ac85fae7-cede-4708-beff-ae01c7fa1c26
* RIT MHD dev:bmundim2011-04-27
| | | | | | | 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
* RIT MHD dev:bmundim2010-12-25
| | | | | | | | | | | | | | 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
* Add the magnetized routine versions for prim2con2prim bmundim2010-10-08
| | | | | | | | | | 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
* file/parameter string replacement from whisky to GRHydrobmundim2010-05-03
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@106 ac85fae7-cede-4708-beff-ae01c7fa1c26
* update from public Whisky versionknarf2010-01-11
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@12 ac85fae7-cede-4708-beff-ae01c7fa1c26
* This is a _temporary_ repository to be able to start to work on theknarf2009-11-18
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
generated by cgit v1.2.3 (git 2.39.1) at 2024-05-17 12:21:21 +0000