[Commits] [svn:einsteintoolkit] IllinoisGRMHD/ (Rev. 4)

zachetie at gmail.com zachetie at gmail.com
Tue Oct 1 18:25:17 CDT 2013


User: zetienne
Date: 2013/10/01 06:25 PM

Removed:
 /
  configuration.ccl, interface.ccl, param.ccl, schedule.ccl
 /doc/
 /src/

Log:
 Move to trunk.

File Changes:

Directory: /
============

File [removed]: configuration.ccl
Delta lines: +0 -9
===================================================================
--- configuration.ccl	2013-10-01 22:26:48 UTC (rev 3)
+++ configuration.ccl	2013-10-01 23:25:16 UTC (rev 4)
@@ -1,9 +0,0 @@
-# Configuration definition for thorn IllinoisGRMHD
-PROVIDES IllinoisGRMHD
-{
-  SCRIPT
-  LANG
-}
-
-# A list of thorns that must be compiled with this one. (Incomplete, but okay if you use the appropriate ThornList)
-REQUIRES CartGrid3D excision bssn

File [removed]: interface.ccl
Delta lines: +0 -138
===================================================================
--- interface.ccl	2013-10-01 22:26:48 UTC (rev 3)
+++ interface.ccl	2013-10-01 23:25:16 UTC (rev 4)
@@ -1,138 +0,0 @@
-# Interface definition for thorn IllinoisGRMHD
-
-implements: IllinoisGRMHD
-inherits: grid
-
-USES INCLUDE: Symmetry.h
-friend: BSSN
-friend: lapse
-friend: shift
-friend: excision
-friend: fisheye
-
-protected:
-
-#vvvvvvvv EVOLVED VARIABLES vvvvvvvv#
-cctk_real grmhd_conservatives type = GF TAGS='prolongation="Lag3"' Timelevels=3
-{
-  rho_star,tau,mhd_st_x,mhd_st_y,mhd_st_z
-} "Evolved mhd variables"
-
-# These variables are semi-staggered:
-# Ax is defined on the semi-staggered grid (i,j+1/2,k+1/2)
-cctk_real em_Ax type = GF Timelevels=3 tags='Prolongation="STAGGER011"'
-{
-  Ax
-} "x-component of the vector potential, evolved when constrained_transport_scheme==3"
-# Ay is defined on the semi-staggered grid (i+1/2,j,k+1/2)
-cctk_real em_Ay type = GF Timelevels=3 tags='Prolongation="STAGGER101"'
-{
-  Ay
-} "y-component of the vector potential, evolved when constrained_transport_scheme==3"
-# Az is defined on the semi-staggered grid (i+1/2,j+1/2,k)
-cctk_real em_Az type = GF Timelevels=3 tags='Prolongation="STAGGER110"'
-{
-  Az
-} "z-component of the vector potential, evolved when constrained_transport_scheme==3"
-
-# psi6phi is defined on the staggered grid (i+1/2,j+1/2,k+1/2)
-cctk_real em_psi6phi type = GF Timelevels=3 tags='Prolongation="STAGGER111"'
-{
-  psi6phi 
-} "\sqrt{\gamma} \Phi, where Phi is the em scalar potential"
-#^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^#
-
-
-#vvvvvvv PRIMITIVE VARIABLES vvvvvvv#
-cctk_real grmhd_primitives_allbutBi type = GF TAGS='InterpNumTimelevels=1 prolongation="none"'
-{
-  rho_b,P,vx,vy,vz,u0
-}
-cctk_real grmhd_primitives_Bi type = GF TAGS='InterpNumTimelevels=1 prolongation="none"'
-{
-  Bx,By,Bz,Bx_stagger,By_stagger,Bz_stagger
-}
-#^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^#
-
-#vvvvvvv EQUATION OF STATE VARIABLES vvvvvvv#
-REAL eos_params_arrays1 TYPE=ARRAY DISTRIB=CONSTANT DIM=1 SIZE=10
-{
-  rho_tab,P_tab,eps_tab
-} "eos_parameters"
-
-REAL eos_params_arrays2 TYPE=ARRAY DISTRIB=CONSTANT DIM=1 SIZE=11
-{
-  k_tab,gamma_tab
-} "eos_parameters"
-
-REAL eos_params_scalar TYPE = SCALAR 
-{
-  n_poly
-} "polytropic index"
-#^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^#
-
-
-private:
-
-#vvvvvvv TEMPORARY VARIABLES FOR RECONSTRUCTION vvvvvvv#
-cctk_real grmhd_primitives_reconstructed_temps type = GF TAGS='Checkpoint="no"'
-{
-  ftilde_gf,temporary,
-  rho_br,Pr,vxr,vyr,vzr,Bxr,Byr,Bzr,Bx_staggerr,By_staggerr,Bz_staggerr,
-  rho_bl,Pl,vxl,vyl,vzl,Bxl,Byl,Bzl,Bx_staggerl,By_staggerl,Bz_staggerl,
-  vxrr,vxrl,vyrr,vyrl,vzrr,vzrl,vxlr,vxll,vylr,vyll,vzlr,vzll
-}
-#^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^#
-
-#vvvvvvv RHS VARIABLES vvvvvvv#
-cctk_real grmhd_conservatives_rhs type = GF TAGS='Checkpoint="no"'
-{
-  rho_star_rhs,tau_rhs,st_x_rhs,st_y_rhs,st_z_rhs
-}
-
-cctk_real em_Ax_rhs type = GF TAGS='Checkpoint="no"'
-{ 
-  Ax_rhs 
-}
-cctk_real em_Ay_rhs type = GF TAGS='Checkpoint="no"'
-{
-  Ay_rhs 
-}
-cctk_real em_Az_rhs type = GF TAGS='Checkpoint="no"'
-{ 
-  Az_rhs 
-}
-cctk_real em_psi6phi_rhs type = GF TAGS='Checkpoint="no"'
-{
-  psi6phi_rhs 
-}
-#^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^#
-
-#vvvvvvv TEMPORARY VARIABLES USEFUL FOR A-FIELD EVOLUTION vvvvvvv#
-cctk_real grmhd_cmin_cmax_temps type = GF TAGS='Checkpoint="no"'
-{
-  cmin_x,cmax_x,
-  cmin_y,cmax_y,
-  cmin_z,cmax_z
-}
-#^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^#
-
-#vvvvvvv TEMPORARY VARIABLES USEFUL FOR FLUX COMPUTATION vvvvvvv#
-cctk_real grmhd_flux_temps type = GF TAGS='Checkpoint="no"'
-{
-  rho_star_flux,tau_flux,st_x_flux,st_y_flux,st_z_flux
-}
-#^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^#
-
-#vvvvvvv T^{\mu \nu}, stored to avoid expensive recomputation vvvvvvv#
-cctk_real TUPmunu type = GF TAGS='Checkpoint="no"'
-{
-  TUPtt,TUPtx,TUPty,TUPtz,TUPxx,TUPxy,TUPxz,TUPyy,TUPyz,TUPzz
-}
-
-###########################################################################
-# Following needed for MoL (timestepping):
-CCTK_INT FUNCTION MoLRegisterEvolvedGroup(CCTK_INT IN EvolvedIndex, \
-                                          CCTK_INT IN RHSIndex)
-REQUIRES FUNCTION MoLRegisterEvolvedGroup
-###########################################################################

File [removed]: param.ccl
Delta lines: +0 -103
===================================================================
--- param.ccl	2013-10-01 22:26:48 UTC (rev 3)
+++ param.ccl	2013-10-01 23:25:16 UTC (rev 4)
@@ -1,103 +0,0 @@
-# Parameter definitions for thorn IllinoisGRMHD
-shares: bssn
-USES KEYWORD zero_out_matter_source_terms
-
-#########################################################
-# Timestepping (MoL) stuff
-shares: MethodOfLines
-
-USES CCTK_INT MoL_Num_Evolved_Vars
-
-restricted:
-CCTK_INT IllinoisGRMHD_MaxNumEvolvedVars "The maximum number of evolved variables used by BSSN" ACCUMULATOR-BASE=MethodofLines::MoL_Num_Evolved_Vars
-{
-  9:9           :: "Just 9: rho_star,tau,mhd_st_x,mhd_st_y,mhd_st_z,Ax,Ay,Az, and psi6phi"
-} 9
-#########################################################
-
-restricted:
-
-#########################################################
-# CONSERV TO PRIMS PARAMETERS
-INT tau_stildefix_enable "tau<0 fix in primitive_vars_hybrid2 to reduce number of Font fixes, especially in puncture+matter evolutions" STEERABLE=ALWAYS
-{
- 0:3 :: "zero (disable), one (enable everywhere), or two (enable only where Psi6 > 50.0 [i.e., inside the horizon, where B's are set to zero], or three (kludge: set B=0 if tau<0 inside horizon))"
-} 0
-
-REAL tau_atm "Parameter used only when tau_stildefix_enable==1.  Should be set by your initial data thorn!  If you need to change this parameter mid-run, you'll need to set STEERABLE=ALWAYS!"
-{
- 0:* :: "Positive"
-} 100.000
-
-REAL rho_b_atm "Atmosphere value of rho_b.  Should be set by your initial data thorn!  If you need to change this parameter mid-run, you'll need to set STEERABLE=ALWAYS!" STEERABLE=ALWAYS
-{
- *:* :: "Allow for negative values.  This enables us to debug the code and verify if rho_b_atm is properly set."
-} 100.000
-
-INT conserv_to_prims_debug "0: no, 1: yes" STEERABLE=ALWAYS
-{
- 0:1 :: "zero (no) or one (yes)"
-} 0
-
-REAL Psi6threshold "Where Psi^6 > Psi6threshold, we assume we're inside the horizon in the primitives solver, and certain limits are relaxed or imposed" STEERABLE=ALWAYS
-{
- *:* :: "Can set to anything"
-} 1e100
-#########################################################
-
-#########################################################
-# EQUATION OF STATE PARAMS, LOOK FOR MORE IN interface.ccl!
-INT neos "number of parameters in EOS table. If you want to increase from the default max value, you MUST also set eos_params_arrays1 and eos_params_arrays2 in interface.ccl to be consistent!"
-{
- 1:10 :: "Any integer between 1 and 10"
-} 1
-
-REAL gamma_th "thermal gamma parameter"
-{
- *:* :: "Any real"
-} 1.3
-
-REAL K_poly "initial polytropic constant"
-{
- 0:* :: "Positive"
-} 1.0
-#########################################################
-
-#########################################################
-# BOUNDARY CONDITION PARAMS
-INT Matter_BC "Chosen Matter boundary condition: OUTFLOW = 1,FREEZE = 2,COPY = 3,LINEAR = 4,QUADRATIC = 5,PLANAR = 6"
-{
- *:* :: "Any integer"
-} 1
-
-INT EM_BC "EM field boundary condition"
-{
- 1:5 :: "COPY=1, FREEZE=2, EXTRAP=3, QUAD=4, PLANAR=5"
-} 1
-
-REAL Sym_Bz "Symmetry parameter across z axis for magnetic fields = +/- 1"
-{
- -1.0:1.0 :: "Set to +1 or -1."
-} 1.0
-#########################################################
-
-###############################################################################################
-
-private:
-
-#########################################################
-# EVOLUTION PARAMS
-REAL damp_lorenz "Damping factor for Lorenz gauge. Has units of 1/length = 1/M. Try using the same value as used for the eta parameter, or smaller! Brian tried 0.1 with ADM mass of 1." STEERABLE=ALWAYS
-{
- *:* :: "any real"
-} 0.0
-#########################################################
-
-#########################################################
-# SANITY CHECK, 
-#   (to ensure equation of state is properly set up)
-INT really_want_gamma_th_of_1_point_3 "Show gamma_th error message if gamma_th has not been reset from its default value (of 1.3).  You must set gamma_th to the appropriate value in your initial data thorn or your .par file!"
-{
- 0:1 :: "zero (no) or one (yes)"
-} 0
-#########################################################

File [removed]: schedule.ccl
Delta lines: +0 -190
===================================================================
--- schedule.ccl	2013-10-01 22:26:48 UTC (rev 3)
+++ schedule.ccl	2013-10-01 23:25:16 UTC (rev 4)
@@ -1,190 +0,0 @@
-# Scheduler setup for IllinoisGRMHD
-
-STORAGE: bssn::BSSN_vars[3], bssn::BSSN_rhs, have_global_bdry
-STORAGE: bssn::BSSN_diag_restrict, bssn::BSSN_gupij, bssn::BSSN_matter, bssn::BSSN_aux_restrict2, phi_derivs, bssn::BSSN_aux_private,bssn::BSSN_AH
-STORAGE: bssn::BSSN_refbd[3]
-
-STORAGE: lapse::lapse_vars[3]
-STORAGE: shift::shift_vars[3]
-STORAGE: grmhd_conservatives[3],em_Ax[3],em_Ay[3],em_Az[3],em_psi6phi[3] 
-STORAGE: grmhd_primitives_allbutBi,grmhd_primitives_Bi,grmhd_primitives_reconstructed_temps,grmhd_conservatives_rhs,em_Ax_rhs,em_Ay_rhs,em_Az_rhs,em_psi6phi_rhs,grmhd_cmin_cmax_temps,grmhd_flux_temps,TUPmunu
-STORAGE: eos_params_arrays1,eos_params_arrays2,eos_params_scalar
-STORAGE: fisheye::fisheye_vars
-STORAGE: excision::excision_int_gfs
-
-####################
-# RUN INITIALLY ONLY
-schedule IllinoisGRMHD_RegisterVars in MoL_Register after BSSN_RegisterVars after lapse_RegisterVars
-{
-  LANG: C
-  OPTIONS: META
-} "Register evolved, rhs variables in IllinoisGRMHD for MoL"
-
-# Tells the symmetry thorn how to apply symmetries on each gridfunction:
-schedule IllinoisGRMHD_InitSymBound at BASEGRID after Lapse_InitSymBound
-{
-  LANG: C
-} "Schedule symmetries"
-
-schedule compute_B_and_Bstagger_from_A in ABE_PostInitial as compute_b after postid after empostid after lapsepostid
-{
-  OPTIONS: GLOBAL,loop-local
-  SYNC: grmhd_primitives_Bi
-  LANG: C
-} "Compute B and B_stagger from A SYNC: grmhd_primitives_Bi"
-
-#FIXME:
-# Probably want to add this, so that initial data thorns don't need to set conservative variables...
-#schedule driver_prims_to_conserv in ABE_PostInitial as p2c after compute_b
-#{
-#  OPTIONS: GLOBAL,loop-local
-#  LANG: C
-#} "Compute conservative variables from primitive variables. This is simple and algebraic, unlike the inverse operation!"
-
-schedule IllinoisGRMHD_PostInitialData in ABE_PostInitial as mhdpostid after compute_b after p2c
-{
-  LANG: C
-  OPTIONS: GLOBAL,loop-local
-} "Compute post-initialdata quantities"
-####################
-
-####################
-# RHS EVALUATION
-schedule driver_evaluate_MHD_rhs in MoL_CalcRHS as IllinoisGRMHD_RHS_eval after bssn_rhs after shift_rhs
-{
-  LANG: C
-#FIXME: Not sure these SYNC's are necessary...
-  SYNC: grmhd_conservatives,em_Ax,em_Ay,em_Az,em_psi6phi
-} "Evaluate RHSs of GR Hydro & GRMHD equations"
-####################
-
-
-##############################################
-# AFTER TIMELEVEL SWITCH, RECOMPUTE PRIMITIVES
-
-schedule GROUP IllinoisGRMHD_Recompute_Primitives_MoLPostStep at CCTK_EVOL after MoL_Evolution
-{
-} "Recompute MHD primitive variables right after flipping gridfunction timelevels. We must do this because primitives are defined only on 1 timelevel and conservs on 3."
-
-schedule IllinoisGRMHD_InitSymBound in IllinoisGRMHD_Recompute_Primitives_MoLPostStep as mhd_mol_post_step before compute_b_poststep
-{
-  OPTIONS: LEVEL,LOOP-LOCAL
-  SYNC: grmhd_conservatives,em_Ax,em_Ay,em_Az,em_psi6phi
-  LANG: C
-} "Schedule symmetries"
-
-schedule compute_B_and_Bstagger_from_A in IllinoisGRMHD_Recompute_Primitives_MoLPostStep as compute_b_poststep
-{
-  SYNC: grmhd_primitives_Bi
-  LANG: C
-} "Compute B and B_stagger from A"
-
-schedule conserv_to_prims in IllinoisGRMHD_Recompute_Primitives_MoLPostStep as mhd_conserv2prims_poststep after compute_b_poststep
-{
-  LANG: C
-} "Compute primitive variables from conservatives. This is non-trivial, requiring a Newton-Raphson root-finder."
-##############################################
-
-
-##########################################################
-# AFTER REGRID, COMPUTE B FROM A & RE-SOLVE FOR PRIMITIVES
-
-schedule IllinoisGRMHD_InitSymBound at CCTK_POSTREGRID as prolong_stuff after MoL_PostStep after fish_postregrid_update before compute_B_postregrid
-{
- OPTIONS: LEVEL,LOOP-LOCAL
-  SYNC: grmhd_conservatives,em_Ax,em_Ay,em_Az,em_psi6phi
-  LANG: C
-} "Schedule symmetries -- Actually just a placeholder function to ensure prolongation / processor syncs are done BEFORE the primitives solver."
-
-schedule compute_B_and_Bstagger_from_A at CCTK_POSTREGRID as compute_B_postregrid after fish_postregrid_update
-{
-  OPTIONS: LEVEL,LOOP-LOCAL
-  SYNC: grmhd_primitives_Bi
-  LANG: C
-} "Compute B and B_stagger from A"
-
-schedule conserv_to_prims at CCTK_POSTREGRID as mhd_conserv2prims_postregrid after compute_B_postregrid before bssn_postregrid before MaskZero
-{
-  OPTIONS: LEVEL,LOOP-LOCAL
-  LANG: C
-} "Compute primitive variables from conservatives. This is non-trivial, requiring a Newton-Raphson root-finder."
-##########################################################
-
-
-##########################################################
-# AFTER RESTRICT, COMPUTE B FROM A & RE-SOLVE FOR PRIMITIVES
-
-schedule IllinoisGRMHD_InitSymBound at CCTK_POSTRESTRICT as post_restrict_SYNCs before compute_B_postrestrict after fish_postregrid_update0 after MoL_PostStep
-{
-  OPTIONS: LEVEL,LOOP-LOCAL
-  SYNC: grmhd_conservatives,em_Ax,em_Ay,em_Az,em_psi6phi
-  LANG: C
-} "Schedule symmetries -- Actually just a placeholder function to ensure prolongation / processor syncs are done BEFORE the primitives solver."
-
-schedule compute_B_and_Bstagger_from_A at CCTK_POSTRESTRICT as compute_B_postrestrict after fish_update
-{
-  OPTIONS: LEVEL,LOOP-LOCAL
-  SYNC: grmhd_primitives_Bi
-  LANG: C
-} "Compute B and B_stagger from A"
-
-schedule conserv_to_prims at CCTK_POSTRESTRICT as mhd_conserv2prims_postrestrict after compute_B_postrestrict before bssn_postregrid
-{
-  OPTIONS: LEVEL,LOOP-LOCAL
-  LANG: C
-} "Compute primitive variables from conservatives. This is non-trivial, requiring a Newton-Raphson root-finder."
-##########################################################
-
-####################################################
-# APPLY BOUNDARY CONDITIONS & RE-SOLVE FOR PRIMITIVES
-schedule IllinoisGRMHD_InitSymBound in ABE_PostStep as poststep_SYNCs before A_bc after iter_count_update after lapse_postbc after shift_update_bc
-{
-  OPTIONS: LEVEL,LOOP-LOCAL
-  SYNC: grmhd_conservatives,em_Ax,em_Ay,em_Az,em_psi6phi
-  LANG: C
-} "Schedule symmetries -- Actually just a placeholder function to ensure prolongation / processor syncs are done BEFORE the primitives solver."
-
-# Since compute_B_and_Bstagger_from_A depends on Bi's being defined everywhere, we must first
-#  apply boundary conditions to Ai's:
-if(Matter_BC!=2 && EM_BC!=2) {
-# I removed this ugly bit of FORTRAN code, as it seems more reasonable to simply move to the nice BC interface in ET.
-#		schedule IllinoisGRMHD_driver_bcs_on_A in ABE_PostStep as A_bc after iter_count_update after lapse_postbc after shift_update_bc after poststep_SYNCs
-#	     	{
-#	     	  SYNC: em_Ax,em_Ay,em_Az,em_psi6phi
-#	     	  LANG:   FORTRAN
-#	     	} "Apply BC on Ai"
-		schedule output_BC_error as BC_error after iter_count_update after lapse_postbc after shift_update_bc after poststep_SYNCs
-		{
-		  LANG: C
-		} "Output error if BC type is set to something other than FROZEN, until we are able to use the nice ET boundary condition interface"
-} else 	     	{
-	     	schedule apply_frozen_boundary_condition in ABE_PostStep as A_bc after iter_count_update after lapse_postbc after shift_update_bc after poststep_SYNCs
-	     	{
-	     	  SYNC: grmhd_conservatives,em_Ax,em_Ay,em_Az,em_psi6phi
-	     	  LANG:   C
-	     	} "Apply FROZEN BCs on Ai AND conservatives!"
-}
-
-schedule compute_B_and_Bstagger_from_A in ABE_PostStep as compute_b after A_bc
-{
-  SYNC: grmhd_primitives_Bi
-  LANG: C
-} "Compute B and B_stagger from A"
-
-schedule conserv_to_prims in ABE_PostStep as conserv2prims after compute_b
-{
-  LANG: C
-} "Compute primitive variables from conservatives. This is non-trivial, requiring a Newton-Raphson root-finder."
-
-# I removed this ugly bit of FORTRAN code, as it seems more reasonable to simply move to the nice BC interface in ET.
-#if(Matter_BC!=2 && EM_BC!=2) {
-#		schedule IllinoisGRMHD_driver_bcs in ABE_PostStep as mhd_bc after conserv2prims
-#		{
-#		  #Note that the SYNC's here are only processor syncs, and are only intended for the coarsest level; no prolongation is done inside the MoL substepping!
-#		  SYNC: grmhd_primitives_allbutBi
-#		  # Eventually we'll want to try applying BCs on conservatives only. For now, BCs are applied to prims, then we recompute conservs
-#		  SYNC: grmhd_conservatives,em_Ax,em_Ay,em_Az,em_psi6phi
-#		  LANG:   FORTRAN
-#		} "Update boundaries on GRMHD conservatives"
-#}
-####################################################



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