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/*@@
@file GRHydro_UpdateMaskM.F90
@date Sep 2, 2010
@author
@desc
Alter the update terms if inside the atmosphere or excision region
@enddesc
@@*/
#include "cctk.h"
#include "cctk_Parameters.h"
#include "cctk_Arguments.h"
#include "GRHydro_Macros.h"
#include "SpaceMask.h"
!!$ We don't need to adapt GRHydroUpdateAtmosphereMask, GRHydro_SetupMask, or
!!$ since we need to evolve Bvec in the atmosphere
!!$ In GRHydro_AtmosphereResetM, we just need to switch the P2C calls to MHD
/*@@
@routine GRHydro_AtmosphereResetM
@date Sep 2, 2010
@author Joshua Faber, Scott Noble, Bruno Mundim, Ian Hawke
@desc
After MoL has evolved, if a point is supposed to be reset then do so.
@enddesc
@calls
@calledby
@history
@endhistory
@@*/
subroutine GRHydro_AtmosphereResetM(CCTK_ARGUMENTS)
implicit none
DECLARE_CCTK_ARGUMENTS
DECLARE_CCTK_PARAMETERS
CCTK_INT :: i, j, k
CCTK_REAL :: det, psi4pt
do k = 1, cctk_lsh(3)
do j = 1, cctk_lsh(2)
do i = 1, cctk_lsh(1)
if ( atmosphere_mask(i, j, k) .eq. 1) then
rho(i,j,k) = GRHydro_rho_min
vel(i,j,k,1) = 0.0d0
vel(i,j,k,2) = 0.0d0
vel(i,j,k,3) = 0.0d0
det = SPATIAL_DETERMINANT(gxx(i,j,k), gxy(i,j,k), gxz(i,j,k), \
gyy(i,j,k), gyz(i,j,k), gzz(i,j,k))
call prim2conpolytypeM(GRHydro_polytrope_handle, &
gxx(i,j,k), gxy(i,j,k), gxz(i,j,k), &
gyy(i,j,k), gyz(i,j,k), gzz(i,j,k), det, &
dens(i,j,k), scon(i,j,k,1), scon(i,j,k,2), scon(i,j,k,3), &
tau(i,j,k), Bcons(i,j,k,1),Bcons(i,j,k,2),Bcons(i,j,k,3),&
rho(i,j,k), vel(i,j,k,1), vel(i,j,k,2), &
vel(i,j,k,3), eps(i,j,k), press(i,j,k), &
Bvec(i,j,k,1),Bvec(i,j,k,2),Bvec(i,j,k,3),w_lorentz(i,j,k))
if (wk_atmosphere .eq. 0) then
atmosphere_mask(i, j, k) = 0
end if
end if
end do
end do
end do
!!$ call GRHydro_BoundariesM(CCTK_PASS_FTOF)
end subroutine GRHydro_AtmosphereResetM
subroutine GRHydro_InitialAtmosphereResetM(CCTK_ARGUMENTS)
implicit none
DECLARE_CCTK_ARGUMENTS
DECLARE_CCTK_PARAMETERS
CCTK_INT :: i, j, k
CCTK_REAL :: det, psi4pt
CCTK_INT :: eos_handle
! begin EOS Omni vars
integer :: n,keytemp,anyerr,keyerr(1)
real*8 :: xpress,xeps,xtemp,xye
n=1;keytemp=0;anyerr=0;keyerr(1)=0
xpress=0.0d0;xye=0.0d0;xeps=0.0d0;xtemp=0.0d0
! end EOS Omni vars
eos_handle = GRHydro_polytrope_handle
do k = 1, cctk_lsh(3)
do j = 1, cctk_lsh(2)
do i = 1, cctk_lsh(1)
if (rho(i,j,k) .le. GRHydro_rho_min) then
rho(i,j,k) = GRHydro_rho_min
vel(i,j,k,1) = 0.0d0
vel(i,j,k,2) = 0.0d0
vel(i,j,k,3) = 0.0d0
call EOS_Omni_press(eos_handle,keytemp,GRHydro_eos_rf_prec,n,&
rho(i,j,k),eps(i,j,k),xtemp,xye,press(i,j,k),keyerr,anyerr)
call EOS_Omni_EpsFromPress(eos_handle,keytemp,GRHydro_eos_rf_prec,n,&
rho(i,j,k),xeps,xtemp,xye,press(i,j,k),eps(i,j,k),keyerr,anyerr)
det = SPATIAL_DETERMINANT(gxx(i,j,k), gxy(i,j,k), gxz(i,j,k), \
gyy(i,j,k), gyz(i,j,k), gzz(i,j,k))
call prim2conpolytypeM(eos_handle, &
gxx(i,j,k), gxy(i,j,k), gxz(i,j,k), &
gyy(i,j,k), gyz(i,j,k), gzz(i,j,k), det, &
dens(i,j,k), scon(i,j,k,1), scon(i,j,k,2), scon(i,j,k,3), &
tau(i,j,k), Bcons(i,j,k,1),Bcons(i,j,k,2),Bcons(i,j,k,3),&
rho(i,j,k), vel(i,j,k,1), vel(i,j,k,2), &
vel(i,j,k,3), eps(i,j,k), press(i,j,k), &
Bvec(i,j,k,1),Bvec(i,j,k,2),Bvec(i,j,k,3),w_lorentz(i,j,k))
end if
if (timelevels .gt. 1) then
if (rho_p(i,j,k) .le. GRHydro_rho_min) then
rho_p(i,j,k) = GRHydro_rho_min
vel_p(i,j,k,1) = 0.0d0
vel_p(i,j,k,2) = 0.0d0
vel_p(i,j,k,3) = 0.0d0
call EOS_Omni_press(eos_handle,keytemp,GRHydro_eos_rf_prec,n,&
rho_p(i,j,k),eps_p(i,j,k),xtemp,xye,press_p(i,j,k),keyerr,anyerr)
call EOS_Omni_EpsFromPress(eos_handle,keytemp,GRHydro_eos_rf_prec,n,&
rho_p(i,j,k),xeps,xtemp,xye,press_p(i,j,k),eps_p(i,j,k),keyerr,anyerr)
det = SPATIAL_DETERMINANT(gxx_p(i,j,k), gxy_p(i,j,k), gxz_p(i,j,k), \
gyy_p(i,j,k), gyz_p(i,j,k), gzz_p(i,j,k))
call prim2conpolytypeM(eos_handle, &
gxx_p(i,j,k), gxy_p(i,j,k), gxz_p(i,j,k), &
gyy_p(i,j,k), gyz_p(i,j,k), gzz_p(i,j,k), det, &
dens_p(i,j,k), scon_p(i,j,k,1), scon_p(i,j,k,2), scon_p(i,j,k,3), &
tau_p(i,j,k), Bcons_p(i,j,k,1),Bcons_p(i,j,k,2),Bcons_p(i,j,k,3),&
rho_p(i,j,k), vel_p(i,j,k,1), vel_p(i,j,k,2), &
vel_p(i,j,k,3), eps_p(i,j,k), press_p(i,j,k), &
Bvec_p(i,j,k,1),Bvec_p(i,j,k,2),Bvec_p(i,j,k,3),w_lorentz_p(i,j,k))
endif
end if
if (timelevels .gt. 2) then
if (rho_p_p(i,j,k) .le. GRHydro_rho_min) then
rho_p_p(i,j,k) = GRHydro_rho_min
vel_p_p(i,j,k,1) = 0.0d0
vel_p_p(i,j,k,2) = 0.0d0
vel_p_p(i,j,k,3) = 0.0d0
call EOS_Omni_press(eos_handle,keytemp,GRHydro_eos_rf_prec,n,&
rho_p_p(i,j,k),eps_p_p(i,j,k),xtemp,xye,press_p_p(i,j,k),keyerr,anyerr)
call EOS_Omni_EpsFromPress(eos_handle,keytemp,GRHydro_eos_rf_prec,n,&
rho_p_p(i,j,k),xeps,xtemp,xye,press_p_p(i,j,k),eps_p_p(i,j,k),keyerr,anyerr)
det = SPATIAL_DETERMINANT(gxx_p_p(i,j,k), gxy_p_p(i,j,k), gxz_p_p(i,j,k), \
gyy_p_p(i,j,k), gyz_p_p(i,j,k), gzz_p_p(i,j,k))
call prim2conpolytypeM(eos_handle, &
gxx_p_p(i,j,k), gxy_p_p(i,j,k), gxz_p_p(i,j,k), &
gyy_p_p(i,j,k), gyz_p_p(i,j,k), gzz_p_p(i,j,k), det, &
dens_p_p(i,j,k), scon_p_p(i,j,k,1), scon_p_p(i,j,k,2), scon_p_p(i,j,k,3), &
tau_p_p(i,j,k), Bcons_p_p(i,j,k,1),Bcons_p_p(i,j,k,2),Bcons_p_p(i,j,k,3),&
rho_p_p(i,j,k), vel_p_p(i,j,k,1), vel_p_p(i,j,k,2), &
vel_p_p(i,j,k,3), eps_p_p(i,j,k), press_p_p(i,j,k), &
Bvec_p_p(i,j,k,1),Bvec_p_p(i,j,k,2),Bvec_p_p(i,j,k,3),w_lorentz_p_p(i,j,k))
endif
endif
end do
end do
end do
write(*,*) " GRHydro_InitialAtmosphereReset"
!!$ call GRHydro_BoundariesM(CCTK_PASS_FTOF)
end subroutine GRHydro_InitialAtmosphereResetM
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