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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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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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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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@157 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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* 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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added.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@134 ac85fae7-cede-4708-beff-ae01c7fa1c26
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