From ea70d0ee2becfeabce8fbc261779c571da1572e0 Mon Sep 17 00:00:00 2001 From: cott Date: Sun, 7 Jul 2013 05:34:05 +0000 Subject: * remove option to have different gamma and K for different stars. That's physically impossible. * adjust test par files (will do so with GRHydro next) * modify the way solutions are added so that atmosphere cuts are applied after solutions are added. Otherwise one of the stars will have the atmosphere added to it. This breaks symmetry. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/TOVSolver/trunk@137 1bdb13ef-5d69-4035-bb54-08abeb3aa7f1 --- test/test_two_max.par | 8 ++++---- 1 file changed, 4 insertions(+), 4 deletions(-) (limited to 'test/test_two_max.par') diff --git a/test/test_two_max.par b/test/test_two_max.par index 39761a3..4a2819a 100644 --- a/test/test_two_max.par +++ b/test/test_two_max.par @@ -45,13 +45,13 @@ tovsolver::TOV_Num_Radial = 200000 tovsolver::TOV_Combine_Method = "maximum" tovsolver::TOV_Rho_Central[0] = 0.16e-3 -tovsolver::TOV_Gamma[0] = 2.0 -tovsolver::TOV_K[0] = 100.0 +tovsolver::TOV_Gamma = 2.0 +tovsolver::TOV_K = 100.0 tovsolver::TOV_Position_x[0] = -15.0 tovsolver::TOV_Rho_Central[1] = 0.32e-3 -tovsolver::TOV_Gamma[1] = 2.0 -tovsolver::TOV_K[1] = 100.0 +tovsolver::TOV_Gamma = 2.0 +tovsolver::TOV_K = 100.0 tovsolver::TOV_Position_x[1] = 15.0 IO::out_fileinfo="none" -- cgit v1.2.3