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authorschnetter <schnetter@0a4070d5-58f5-498f-b6c0-2693e757fa0f>2005-07-22 23:11:25 +0000
committerschnetter <schnetter@0a4070d5-58f5-498f-b6c0-2693e757fa0f>2005-07-22 23:11:25 +0000
commit3342f675f08cb92660676f50ad3eb4a6231c44d3 (patch)
treeab6ebf0267e1fc75102558d952c696a57d7630c5
parentf6290b709fba33db2fc3b4b3e2a73cc7ec9e8432 (diff)
Update future ideas
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/IDAxiBrillBH/trunk@80 0a4070d5-58f5-498f-b6c0-2693e757fa0f
-rw-r--r--doc/TODO4
1 files changed, 3 insertions, 1 deletions
diff --git a/doc/TODO b/doc/TODO
index 948a31e..054a564 100644
--- a/doc/TODO
+++ b/doc/TODO
@@ -5,7 +5,7 @@ This thorn works with non-unigrid Cactus, but it doesn't work very
efficiently: it does the 2D elliptic setup and solve all over again
for each local Cactus (3D) grid. It would be more efficient to move the
2D elliptic stuff out into a separately scheduled routine which would
-be done once (for Carpet, it would be scheduled in level or global
+be done once (for Carpet, it would be scheduled in global
mode), and have only the interpolation to the 3D grid done for each
local Cactus grid.
@@ -26,3 +26,5 @@ computed eta value will fall outside the internal grid.
It would be nice if this restriction could be lifted (eg allowing
a grid point at the origin). Maybe some sort of interpolation in real
space (instead of in eta-space) to fill in the hole at the origin?
+Maybe an extrapolation that can lead outside the eta grid? Maybe use
+the unperturbed black hole data outside the eta grid?