mod_rhd_phys.t

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!> Radiation-Hydrodynamics physics module
!> Module aims at solving the Hydrodynamic equations toghether with
!> the zeroth moment of the radiative transfer equation. A closure is
!> provided by the flux limited diffusion (FLD)-approximation in the mod_fld.t module. See
!> [1]Moens, N., Sundqvist, J. O., El Mellah, I., Poniatowski, L., Teunissen, J., and Keppens, R.,
!> “Radiation-hydrodynamics with MPI-AMRVAC . Flux-limited diffusion”,
!> <i>Astronomy and Astrophysics</i>, vol. 657, 2022. doi:10.1051/0004-6361/202141023.
!> For more information.
!> Another possible closure in the works is the anisotropic flux limited diffusion approximation (AFLD) described in mod_afld.t.
 
module mod_rhd_phys
  use mod_thermal_conduction, only: tc_fluid
  use mod_radiative_cooling, only: rc_fluid
  use mod_thermal_emission, only: te_fluid
  use mod_physics
  use mod_comm_lib, only: mpistop
  implicit none
  private
 
  !> Whether an energy equation is used
  logical, public, protected              :: rhd_energy = .true.
 
  !> Whether thermal conduction is added
  logical, public, protected              :: rhd_thermal_conduction = .false.
  type(tc_fluid), allocatable, public :: tc_fl
  type(te_fluid), allocatable, public :: te_fl_rhd
 
  !> Whether radiative cooling is added
  logical, public, protected              :: rhd_radiative_cooling = .false.
  type(rc_fluid), allocatable, public :: rc_fl
 
  !> Whether dust is added
  logical, public, protected              :: rhd_dust = .false.
 
  !> Whether viscosity is added
  logical, public, protected              :: rhd_viscosity = .false.
 
  !> Whether gravity is added
  logical, public, protected              :: rhd_gravity = .false.
 
  !> Whether particles module is added
  logical, public, protected              :: rhd_particles = .false.
 
  !> Whether rotating frame is activated
  logical, public, protected              :: rhd_rotating_frame = .false.
 
  !> Number of tracer species
  integer, public, protected              :: rhd_n_tracer = 0
 
  !> Index of the density (in the w array)
  integer, public, protected              :: rho_
 
  !> Indices of the momentum density
  integer, allocatable, public, protected :: mom(:)
 
  !> Indices of the tracers
  integer, allocatable, public, protected :: tracer(:)
 
  !> Index of the energy density (-1 if not present)
  integer, public, protected              :: e_
 
  !> Index of the gas pressure (-1 if not present) should equal e_
  integer, public, protected              :: p_
 
  !> Index of the radiation energy
  integer, public, protected              :: r_e
 
  !> Indices of temperature
  integer, public, protected :: te_
 
  !> Index of the cutoff temperature for the TRAC method
  integer, public, protected              :: tcoff_
 
  !> The adiabatic index
  double precision, public                :: rhd_gamma = 5.d0/3.0d0
 
  !> The adiabatic constant
  double precision, public                :: rhd_adiab = 1.0d0
 
  !> The small_est allowed energy
  double precision, protected             :: small_e
 
  !> The smallest allowed radiation energy
  double precision, public, protected             :: small_r_e = 0.d0
 
  !> Whether TRAC method is used
  logical, public, protected              :: rhd_trac = .false.
  integer, public, protected              :: rhd_trac_type = 1
 
  !> Helium abundance over Hydrogen
  double precision, public, protected  :: he_abundance=0.1d0
 
  !> Formalism to treat radiation
  character(len=8), public :: rhd_radiation_formalism = 'fld'
 
  !> In the case of no rhd_energy, how to compute pressure
  character(len=8), public :: rhd_pressure = 'Trad'
 
  !> Treat radiation fld_Rad_force
  logical, public, protected :: rhd_radiation_force = .true.
 
  !> Treat radiation-gas energy interaction
  logical, public, protected :: rhd_energy_interact = .true.
 
  !> Treat radiation energy diffusion
  logical, public, protected :: rhd_radiation_diffusion = .true.
 
  !> Treat radiation advection
  logical, public, protected :: rhd_radiation_advection = .true.
 
  !> Whether plasma is partially ionized
  logical, public, protected :: rhd_partial_ionization = .false.
 
  !> Do a running mean over the radiation pressure when determining dt
  logical, protected :: radio_acoustic_filter = .false.
  integer, protected :: size_ra_filter = 1
 
  !> kb/(m_p mu)* 1/a_rad**4,
  double precision, public :: kbmpmua4
 
  !> Use the speed of light to calculate the timestep, usefull for debugging
  logical :: dt_c = .false.
 
  !> Ionization fraction of H
  !> H_ion_fr = H+/(H+ + H)
  double precision, public, protected  :: h_ion_fr=1d0
  !> Ionization fraction of He
  !> He_ion_fr = (He2+ + He+)/(He2+ + He+ + He)
  double precision, public, protected  :: he_ion_fr=1d0
  !> Ratio of number He2+ / number He+ + He2+
  !> He_ion_fr2 = He2+/(He2+ + He+)
  double precision, public, protected  :: he_ion_fr2=1d0
  ! used for eq of state when it is not defined by units,
  ! the units do not contain terms related to ionization fraction
  ! and it is p = RR * rho * T
  double precision, public, protected  :: rr=1d0
  ! remove the below flag  and assume default value = .false.
  ! when eq state properly implemented everywhere
  ! and not anymore through units
  logical, public, protected :: eq_state_units = .true.
 
  procedure(sub_get_pthermal), pointer :: rhd_get_rfactor   => null()
  ! Public methods
  public :: rhd_phys_init
  public :: rhd_kin_en
  public :: rhd_get_pthermal
  public :: rhd_get_pradiation
  public :: rhd_get_ptot
  public :: rhd_get_csound2
  public :: rhd_to_conserved
  public :: rhd_to_primitive
  public :: rhd_check_params
  public :: rhd_check_w
  public :: rhd_get_tgas
  public :: rhd_get_trad
  public :: rhd_set_mg_bounds
 
contains
 
  !> Read this module's parameters from a file
  subroutine rhd_read_params(files)
    use mod_global_parameters
    character(len=*), intent(in) :: files(:)
    integer                      :: n
 
    namelist /rhd_list/ rhd_energy, rhd_pressure, rhd_n_tracer, rhd_gamma, rhd_adiab, &
    rhd_dust, rhd_thermal_conduction, rhd_radiative_cooling, rhd_viscosity, &
    rhd_gravity, he_abundance, h_ion_fr, he_ion_fr, he_ion_fr2, eq_state_units, &
    si_unit, rhd_particles, rhd_rotating_frame, rhd_trac, &
    rhd_trac_type, rhd_radiation_formalism, &
    rhd_radiation_force, rhd_energy_interact, rhd_radiation_diffusion, &
    rhd_radiation_advection, radio_acoustic_filter, size_ra_filter, dt_c, rhd_partial_ionization
 
    do n = 1, size(files)
       open(unitpar, file=trim(files(n)), status="old")
       read(unitpar, rhd_list, end=111)
111    close(unitpar)
    end do
 
  end subroutine rhd_read_params
 
  !> Write this module's parameters to a snapsoht
  subroutine rhd_write_info(fh)
    use mod_global_parameters
    integer, intent(in)                 :: fh
    integer, parameter                  :: n_par = 1
    double precision                    :: values(n_par)
    character(len=name_len)             :: names(n_par)
    integer, dimension(MPI_STATUS_SIZE) :: st
    integer                             :: er
 
    call mpi_file_write(fh, n_par, 1, mpi_integer, st, er)
 
    names(1) = "gamma"
    values(1) = rhd_gamma
    call mpi_file_write(fh, values, n_par, mpi_double_precision, st, er)
    call mpi_file_write(fh, names, n_par * name_len, mpi_character, st, er)
  end subroutine rhd_write_info
 
  !> Initialize the module
  subroutine rhd_phys_init()
    use mod_global_parameters
    use mod_thermal_conduction
    use mod_radiative_cooling
    use mod_dust, only: dust_init
    use mod_viscosity, only: viscosity_init
    use mod_gravity, only: gravity_init
    use mod_particles, only: particles_init
    use mod_rotating_frame, only:rotating_frame_init
    use mod_fld
    use mod_afld
    use mod_supertimestepping, only: sts_init, add_sts_method,&
            set_conversion_methods_to_head, set_error_handling_to_head
    use mod_ionization_degree
    use mod_usr_methods, only: usr_rfactor
 
    integer :: itr, idir
 
    call rhd_read_params(par_files)
 
    physics_type = "rhd"
    phys_energy  = rhd_energy
    phys_total_energy  = rhd_energy
    phys_gamma = rhd_gamma
 
    phys_trac=rhd_trac
    if(phys_trac) then
      if(ndim .eq. 1) then
        if(rhd_trac_type .gt. 2) then
          rhd_trac_type=1
          if(mype==0) write(*,*) 'WARNING: set rhd_trac_type=1'
        end if
        phys_trac_type=rhd_trac_type
      else
        phys_trac=.false.
        if(mype==0) write(*,*) 'WARNING: set rhd_trac=F when ndim>=2'
      end if
    end if
 
    ! set default gamma for polytropic/isothermal process
    if(.not.rhd_energy) then
      if(rhd_thermal_conduction) then
        rhd_thermal_conduction=.false.
        if(mype==0) write(*,*) 'WARNING: set rhd_thermal_conduction=F when rhd_energy=F'
      end if
      if(rhd_radiative_cooling) then
        rhd_radiative_cooling=.false.
        if(mype==0) write(*,*) 'WARNING: set rhd_radiative_cooling=F when rhd_energy=F'
      end if
    end if
    if(.not.eq_state_units) then
      if(rhd_partial_ionization) then
        rhd_partial_ionization=.false.
        if(mype==0) write(*,*) 'WARNING: set rhd_partial_ionization=F when eq_state_units=F'
      end if
    end if
    use_particles = rhd_particles
 
    allocate(start_indices(number_species),stop_indices(number_species))
 
    ! set the index of the first flux variable for species 1
    start_indices(1)=1
    ! Determine flux variables
    rho_ = var_set_rho()
 
    allocate(mom(ndir))
    mom(:) = var_set_momentum(ndir)
 
    ! Set index of energy variable
    if (rhd_energy) then
       e_ = var_set_energy()
       p_ = e_
    else
       e_ = -1
       p_ = -1
    end if
 
    !> set radiation energy
    r_e = var_set_radiation_energy()
 
    !  set temperature as an auxiliary variable to get ionization degree
    if(rhd_partial_ionization) then
      te_ = var_set_auxvar('Te','Te')
    else
      te_ = -1
    end if
 
    phys_get_dt              => rhd_get_dt
    phys_get_cmax            => rhd_get_cmax
    phys_get_a2max           => rhd_get_a2max
    phys_get_tcutoff         => rhd_get_tcutoff
    phys_get_cbounds         => rhd_get_cbounds
    phys_get_flux            => rhd_get_flux
    phys_add_source_geom     => rhd_add_source_geom
    phys_add_source          => rhd_add_source
    phys_to_conserved        => rhd_to_conserved
    phys_to_primitive        => rhd_to_primitive
    ! phys_ei_to_e             => rhd_ei_to_e
    ! phys_e_to_ei             => rhd_e_to_ei
    phys_check_params        => rhd_check_params
    phys_check_w             => rhd_check_w
    phys_get_pthermal        => rhd_get_pthermal
    phys_write_info          => rhd_write_info
    phys_handle_small_values => rhd_handle_small_values
    phys_set_mg_bounds       => rhd_set_mg_bounds
    phys_get_trad            => rhd_get_trad
    phys_get_tgas            => rhd_get_tgas
 
    ! derive units from basic units
    call rhd_physical_units()
 
    if (rhd_dust) then
        call dust_init(rho_, mom(:), e_)
    endif
 
    !> Initiate radiation-closure module
    select case (rhd_radiation_formalism)
    case('fld')
      call fld_init(he_abundance, rhd_radiation_diffusion, rhd_energy_interact, rhd_gamma)
    case('afld')
      call afld_init(he_abundance, rhd_radiation_diffusion, rhd_gamma)
    case default
      call mpistop('Radiation formalism unknown')
    end select
 
    allocate(tracer(rhd_n_tracer))
 
    ! Set starting index of tracers
    do itr = 1, rhd_n_tracer
       tracer(itr) = var_set_fluxvar("trc", "trp", itr, need_bc=.false.)
    end do
 
    ! set number of variables which need update ghostcells
    nwgc=nwflux+nwaux
 
    ! set the index of the last flux variable for species 1
    stop_indices(1)=nwflux
 
    if(rhd_trac) then
      tcoff_ = var_set_wextra()
      iw_tcoff=tcoff_
    else
      tcoff_ = -1
    end if
 
    ! choose Rfactor in ideal gas law
    if(rhd_partial_ionization) then
      rhd_get_rfactor=>rfactor_from_temperature_ionization
      phys_update_temperature => rhd_update_temperature
    else if(associated(usr_rfactor)) then
      rhd_get_rfactor=>usr_rfactor
    else
      rhd_get_rfactor=>rfactor_from_constant_ionization
    end if
 
    ! initialize thermal conduction module
    if (rhd_thermal_conduction) then
      if (.not. rhd_energy) &
           call mpistop("thermal conduction needs rhd_energy=T")
 
      call sts_init()
      call tc_init_params(rhd_gamma)
 
      allocate(tc_fl)
      call tc_get_hd_params(tc_fl,tc_params_read_rhd)
      tc_fl%get_temperature_from_conserved => rhd_get_temperature_from_etot
      call add_sts_method(rhd_get_tc_dt_rhd,rhd_sts_set_source_tc_rhd,e_,1,e_,1,.false.)
      call set_conversion_methods_to_head(rhd_e_to_ei, rhd_ei_to_e)
      call set_error_handling_to_head(rhd_tc_handle_small_e)
      tc_fl%get_temperature_from_eint => rhd_get_temperature_from_eint
      tc_fl%get_rho => rhd_get_rho
      tc_fl%e_ = e_
    end if
 
    ! Initialize radiative cooling module
    if (rhd_radiative_cooling) then
      if (.not. rhd_energy) &
           call mpistop("radiative cooling needs rhd_energy=T")
      call radiative_cooling_init_params(rhd_gamma,he_abundance)
      allocate(rc_fl)
      call radiative_cooling_init(rc_fl,rc_params_read)
      rc_fl%get_rho => rhd_get_rho
      rc_fl%get_pthermal => rhd_get_pthermal
      rc_fl%get_var_Rfactor => rhd_get_rfactor
      rc_fl%e_ = e_
      rc_fl%Tcoff_ = tcoff_
    end if
    allocate(te_fl_rhd)
    te_fl_rhd%get_rho=> rhd_get_rho
    te_fl_rhd%get_pthermal=> rhd_get_pthermal
    te_fl_rhd%get_var_Rfactor => rhd_get_rfactor
{^ifthreed
    phys_te_images => rhd_te_images
}
    ! Initialize viscosity module
    if (rhd_viscosity) call viscosity_init(phys_wider_stencil)
 
    ! Initialize gravity module
    if (rhd_gravity) call gravity_init()
 
    ! Initialize rotating_frame module
    if (rhd_rotating_frame) call rotating_frame_init()
 
    ! Initialize particles module
    if (rhd_particles) then
       call particles_init()
    end if
 
    ! Check whether custom flux types have been defined
    if (.not. allocated(flux_type)) then
       allocate(flux_type(ndir, nw))
       flux_type = flux_default
    else if (any(shape(flux_type) /= [ndir, nw])) then
       call mpistop("phys_check error: flux_type has wrong shape")
    end if
 
    nvector      = 1 ! No. vector vars
    allocate(iw_vector(nvector))
    iw_vector(1) = mom(1) - 1
 
    !> Usefull constante
    kbmpmua4 = unit_pressure**(-3.d0/4.d0)*unit_density*const_kb/(const_mp*fld_mu)*const_rad_a**(-1.d0/4.d0)
    ! initialize ionization degree table
    if(rhd_partial_ionization) call ionization_degree_init()
  end subroutine rhd_phys_init
 
{^ifthreed
  subroutine rhd_te_images()
    use mod_global_parameters
    use mod_thermal_emission
    select case(convert_type)
      case('EIvtiCCmpi','EIvtuCCmpi')
        call get_euv_image(unitconvert,te_fl_rhd)
      case('ESvtiCCmpi','ESvtuCCmpi')
        call get_euv_spectrum(unitconvert,te_fl_rhd)
      case('SIvtiCCmpi','SIvtuCCmpi')
        call get_sxr_image(unitconvert,te_fl_rhd)
      case default
        call mpistop("Error in synthesize emission: Unknown convert_type")
      end select
  end subroutine rhd_te_images
}
!!start th cond
  ! wrappers for STS functions in thermal_conductivity module
  ! which take as argument the tc_fluid (defined in the physics module)
  subroutine  rhd_sts_set_source_tc_rhd(ixI^L,ixO^L,w,x,wres,fix_conserve_at_step,my_dt,igrid,nflux)
    use mod_global_parameters
    use mod_fix_conserve
    use mod_thermal_conduction, only: sts_set_source_tc_hd
    integer, intent(in) :: ixi^l, ixo^l, igrid, nflux
    double precision, intent(in) ::  x(ixi^s,1:ndim)
    double precision, intent(inout) ::  wres(ixi^s,1:nw), w(ixi^s,1:nw)
    double precision, intent(in) :: my_dt
    logical, intent(in) :: fix_conserve_at_step
    call sts_set_source_tc_hd(ixi^l,ixo^l,w,x,wres,fix_conserve_at_step,my_dt,igrid,nflux,tc_fl)
  end subroutine rhd_sts_set_source_tc_rhd
 
 
  function rhd_get_tc_dt_rhd(w,ixI^L,ixO^L,dx^D,x) result(dtnew)
    !Check diffusion time limit dt < dx_i**2/((gamma-1)*tc_k_para_i/rho)
    !where                      tc_k_para_i=tc_k_para*B_i**2/B**2
    !and                        T=p/rho
    use mod_global_parameters
    use mod_thermal_conduction, only: get_tc_dt_hd
 
    integer, intent(in) :: ixi^l, ixo^l
    double precision, intent(in) :: dx^d, x(ixi^s,1:ndim)
    double precision, intent(in) :: w(ixi^s,1:nw)
    double precision :: dtnew
 
    dtnew=get_tc_dt_hd(w,ixi^l,ixo^l,dx^d,x,tc_fl)
  end function rhd_get_tc_dt_rhd
 
 
  subroutine rhd_tc_handle_small_e(w, x, ixI^L, ixO^L, step)
    ! move this in a different  routine as in mhd if needed in more places
    use mod_global_parameters
    use mod_small_values
 
    integer, intent(in)             :: ixi^l,ixo^l
    double precision, intent(inout) :: w(ixi^s,1:nw)
    double precision, intent(in)    :: x(ixi^s,1:ndim)
    integer, intent(in)    :: step
 
    integer :: idir
    logical :: flag(ixi^s,1:nw)
    character(len=140) :: error_msg
 
    flag=.false.
    where(w(ixo^s,e_)<small_e) flag(ixo^s,e_)=.true.
    if(any(flag(ixo^s,e_))) then
      select case (small_values_method)
      case ("replace")
        where(flag(ixo^s,e_)) w(ixo^s,e_)=small_e
      case ("average")
        call small_values_average(ixi^l, ixo^l, w, x, flag, e_)
      case default
        ! small values error shows primitive variables
        w(ixo^s,e_)=w(ixo^s,e_)*(rhd_gamma - 1.0d0)
        do idir = 1, ndir
           w(ixo^s, iw_mom(idir)) = w(ixo^s, iw_mom(idir))/w(ixo^s,rho_)
        end do
        write(error_msg,"(a,i3)") "Thermal conduction step ", step
        call small_values_error(w, x, ixi^l, ixo^l, flag, error_msg)
      end select
    end if
  end subroutine rhd_tc_handle_small_e
 
    ! fill in tc_fluid fields from namelist
    subroutine tc_params_read_rhd(fl)
      use mod_global_parameters, only: unitpar,par_files
      use mod_global_parameters, only: unitpar
      type(tc_fluid), intent(inout) :: fl
      integer                      :: n
      logical :: tc_saturate=.false.
      double precision :: tc_k_para=0d0
 
      namelist /tc_list/ tc_saturate, tc_k_para
 
      do n = 1, size(par_files)
         open(unitpar, file=trim(par_files(n)), status="old")
         read(unitpar, tc_list, end=111)
111      close(unitpar)
      end do
      fl%tc_saturate = tc_saturate
      fl%tc_k_para = tc_k_para
 
    end subroutine tc_params_read_rhd
 
  subroutine rhd_get_rho(w,x,ixI^L,ixO^L,rho)
    use mod_global_parameters
    integer, intent(in)           :: ixi^l, ixo^l
    double precision, intent(in)  :: w(ixi^s,1:nw),x(ixi^s,1:ndim)
    double precision, intent(out) :: rho(ixi^s)
 
    rho(ixo^s) = w(ixo^s,rho_)
 
  end subroutine rhd_get_rho
 
!!end th cond
!!rad cool
  subroutine rc_params_read(fl)
    use mod_global_parameters, only: unitpar,par_files
    use mod_constants, only: bigdouble
    use mod_basic_types, only: std_len
    type(rc_fluid), intent(inout) :: fl
    integer                      :: n
    ! list parameters
    integer :: ncool = 4000
 
    !> Name of cooling curve
    character(len=std_len)  :: coolcurve='JCcorona'
 
    !> Fixed temperature not lower than tlow
    logical    :: tfix=.false.
 
    !> Lower limit of temperature
    double precision   :: tlow=bigdouble
 
    !> Add cooling source in a split way (.true.) or un-split way (.false.)
    logical    :: rc_split=.false.
 
 
    namelist /rc_list/ coolcurve, ncool, tlow, tfix, rc_split
 
    do n = 1, size(par_files)
      open(unitpar, file=trim(par_files(n)), status="old")
      read(unitpar, rc_list, end=111)
111     close(unitpar)
    end do
 
    fl%ncool=ncool
    fl%coolcurve=coolcurve
    fl%tlow=tlow
    fl%Tfix=tfix
    fl%rc_split=rc_split
  end subroutine rc_params_read
!! end rad cool
 
  subroutine rhd_check_params
    use mod_global_parameters
    use mod_dust, only: dust_check_params
 
    if (.not. rhd_energy .and. rhd_pressure == 'adiabatic') then
       if (rhd_gamma <= 0.0d0) call mpistop ("Error: rhd_gamma <= 0")
       if (rhd_adiab < 0.0d0) call mpistop  ("Error: rhd_adiab < 0")
       small_pressure= rhd_adiab*small_density**rhd_gamma
    elseif (rhd_pressure == 'Tcond') then
      small_pressure = smalldouble
    else
       if (rhd_gamma <= 0.0d0 .or. rhd_gamma == 1.0d0) &
            call mpistop ("Error: rhd_gamma <= 0 or rhd_gamma == 1.0")
       small_e = small_pressure/(rhd_gamma - 1.0d0)
    end if
 
    small_r_e = small_pressure/(rhd_gamma - 1.0d0)
 
    if (rhd_dust) call dust_check_params()
 
    ! if (rhd_radiation_diffusion .and. (.not. use_imex_scheme) ) &
    if (rhd_radiation_diffusion .and. (.not. use_imex_scheme) .and. ((rhd_radiation_formalism .eq. 'fld') .or. (rhd_radiation_formalism .eq. 'afld')) ) &
    call mpistop("Use an IMEX scheme when doing FLD")
 
    if (use_multigrid) call rhd_set_mg_bounds()
 
  end subroutine rhd_check_params
 
  !> Set the boundaries for the diffusion of E
  subroutine rhd_set_mg_bounds
    use mod_global_parameters
    use mod_multigrid_coupling
    use mod_usr_methods
 
    integer :: ib
 
    ! Set boundary conditions for the multigrid solver
    do ib = 1, 2*ndim
       select case (typeboundary(r_e, ib))
       case (bc_symm)
          ! d/dx u = 0
          mg%bc(ib, mg_iphi)%bc_type = mg_bc_neumann
          mg%bc(ib, mg_iphi)%bc_value = 0.0_dp
       case (bc_asymm)
          ! u = 0
          mg%bc(ib, mg_iphi)%bc_type = mg_bc_dirichlet
          mg%bc(ib, mg_iphi)%bc_value = 0.0_dp
       case (bc_cont)
          ! d/dx u = 0
          ! mg%bc(iB, mg_iphi)%bc_type = mg_bc_continuous
          mg%bc(ib, mg_iphi)%bc_type = mg_bc_neumann
          mg%bc(ib, mg_iphi)%bc_value = 0.0_dp
       case (bc_periodic)
          ! Nothing to do here
       case (bc_noinflow)
          call usr_special_mg_bc(ib)
       case (bc_special)
          call usr_special_mg_bc(ib)
       case default
          call mpistop("divE_multigrid warning: unknown b.c. ")
       end select
    end do
  end subroutine rhd_set_mg_bounds
 
  subroutine rhd_physical_units
    use mod_global_parameters
    double precision :: mp,kb
    double precision :: a,b
    ! Derive scaling units
    if(si_unit) then
      mp=mp_si
      kb=kb_si
    else
      mp=mp_cgs
      kb=kb_cgs
    end if
    if(eq_state_units) then
      a=1d0+4d0*he_abundance
      if(rhd_partial_ionization) then
        b=1d0+h_ion_fr+he_abundance*(he_ion_fr*(he_ion_fr2+1d0)+1d0)
      else
        b=2d0+3d0*he_abundance
      end if
      rr=1d0
    else
      a=1d0
      b=1d0
      rr=(1d0+h_ion_fr+he_abundance*(he_ion_fr*(he_ion_fr2+1d0)+1d0))/(1d0+4d0*he_abundance)
    end if
    if(unit_density/=1.d0 .or. unit_numberdensity/=1.d0) then
      if(unit_density/=1.d0) then
        unit_numberdensity=unit_density/(a*mp)
      else if(unit_numberdensity/=1.d0) then
        unit_density=a*mp*unit_numberdensity
      end if
      if(unit_temperature/=1.d0) then
        unit_pressure=b*unit_numberdensity*kb*unit_temperature
        unit_velocity=sqrt(unit_pressure/unit_density)
        if(unit_length/=1.d0) then
          unit_time=unit_length/unit_velocity
        else if(unit_time/=1.d0) then
          unit_length=unit_velocity*unit_time
        end if
      else if(unit_pressure/=1.d0) then
        unit_temperature=unit_pressure/(b*unit_numberdensity*kb)
        unit_velocity=sqrt(unit_pressure/unit_density)
        if(unit_length/=1.d0) then
          unit_time=unit_length/unit_velocity
        else if(unit_time/=1.d0) then
          unit_length=unit_velocity*unit_time
        end if
      else if(unit_velocity/=1.d0) then
        unit_pressure=unit_density*unit_velocity**2
        unit_temperature=unit_pressure/(b*unit_numberdensity*kb)
        if(unit_length/=1.d0) then
          unit_time=unit_length/unit_velocity
        else if(unit_time/=1.d0) then
          unit_length=unit_velocity*unit_time
        end if
      else if(unit_time/=1.d0) then
        unit_velocity=unit_length/unit_time
        unit_pressure=unit_density*unit_velocity**2
        unit_temperature=unit_pressure/(b*unit_numberdensity*kb)
      end if
    else if(unit_temperature/=1.d0) then
      ! units of temperature and velocity are dependent
      if(unit_pressure/=1.d0) then
        unit_numberdensity=unit_pressure/(b*unit_temperature*kb)
        unit_density=a*mp*unit_numberdensity
        unit_velocity=sqrt(unit_pressure/unit_density)
        if(unit_length/=1.d0) then
          unit_time=unit_length/unit_velocity
        else if(unit_time/=1.d0) then
          unit_length=unit_velocity*unit_time
        end if
      end if
    else if(unit_pressure/=1.d0) then
      if(unit_velocity/=1.d0) then
        unit_density=unit_pressure/unit_velocity**2
        unit_numberdensity=unit_density/(a*mp)
        unit_temperature=unit_pressure/(b*unit_numberdensity*kb)
        if(unit_length/=1.d0) then
          unit_time=unit_length/unit_velocity
        else if(unit_time/=1.d0) then
          unit_length=unit_velocity*unit_time
        end if
      else if(unit_time/=0.d0) then
        unit_velocity=unit_length/unit_time
        unit_density=unit_pressure/unit_velocity**2
        unit_numberdensity=unit_density/(a*mp)
        unit_temperature=unit_pressure/(b*unit_numberdensity*kb)
      end if
    end if
 
    !> Units for radiative flux and opacity
    unit_radflux = unit_velocity*unit_pressure
    unit_opacity = one/(unit_density*unit_length)
 
  end subroutine rhd_physical_units
 
  !> Returns logical argument flag where values are ok
  subroutine rhd_check_w(primitive, ixI^L, ixO^L, w, flag)
    use mod_global_parameters
    use mod_dust, only: dust_check_w
 
    logical, intent(in)          :: primitive
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, nw)
    logical, intent(inout)       :: flag(ixi^s,1:nw)
    double precision             :: tmp(ixi^s)
 
    flag=.false.
 
    if (rhd_energy) then
       if (primitive) then
          where(w(ixo^s, e_) < small_pressure) flag(ixo^s,e_) = .true.
       else
          tmp(ixo^s) = (rhd_gamma - 1.0d0)*(w(ixo^s, e_) - &
               rhd_kin_en(w, ixi^l, ixo^l))
          where(tmp(ixo^s) < small_pressure) flag(ixo^s,e_) = .true.
       endif
    end if
 
    where(w(ixo^s, rho_) < small_density) flag(ixo^s,rho_) = .true.
 
    where(w(ixo^s, r_e) < small_r_e) flag(ixo^s,r_e) = .true.
 
    if(rhd_dust) call dust_check_w(ixi^l,ixo^l,w,flag)
 
  end subroutine rhd_check_w
 
  !> Transform primitive variables into conservative ones
  subroutine rhd_to_conserved(ixI^L, ixO^L, w, x)
    use mod_global_parameters
    use mod_dust, only: dust_to_conserved
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(inout) :: w(ixi^s, nw)
    double precision, intent(in)    :: x(ixi^s, 1:ndim)
    double precision                :: invgam
    integer                         :: idir, itr
 
    !!if (fix_small_values) then
    !!  call rhd_handle_small_values(.true., w, x, ixI^L, ixO^L, 'rhd_to_conserved')
    !!end if
 
    if (rhd_energy) then
       invgam = 1.d0/(rhd_gamma - 1.0d0)
       ! Calculate total energy from pressure and kinetic energy
       w(ixo^s, e_) = w(ixo^s, e_) * invgam + &
            0.5d0 * sum(w(ixo^s, mom(:))**2, dim=ndim+1) * w(ixo^s, rho_)
    end if
 
    ! Convert velocity to momentum
    do idir = 1, ndir
       w(ixo^s, mom(idir)) = w(ixo^s, rho_) * w(ixo^s, mom(idir))
    end do
 
    if (rhd_dust) then
      call dust_to_conserved(ixi^l, ixo^l, w, x)
    end if
 
  end subroutine rhd_to_conserved
 
  !> Transform conservative variables into primitive ones
  subroutine rhd_to_primitive(ixI^L, ixO^L, w, x)
    use mod_global_parameters
    use mod_dust, only: dust_to_primitive
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(inout) :: w(ixi^s, nw)
    double precision, intent(in)    :: x(ixi^s, 1:ndim)
    integer                         :: itr, idir
    double precision                :: inv_rho(ixo^s)
 
    if (fix_small_values) then
      call rhd_handle_small_values(.false., w, x, ixi^l, ixo^l, 'rhd_to_primitive')
    end if
 
    inv_rho = 1.0d0 / w(ixo^s, rho_)
 
    if (rhd_energy) then
       ! Compute pressure
       w(ixo^s, e_) = (rhd_gamma - 1.0d0) * (w(ixo^s, e_) - &
            rhd_kin_en(w, ixi^l, ixo^l, inv_rho))
    end if
 
    ! Convert momentum to velocity
    do idir = 1, ndir
       w(ixo^s, mom(idir)) = w(ixo^s, mom(idir)) * inv_rho
    end do
 
    ! Convert dust momentum to dust velocity
    if (rhd_dust) then
      call dust_to_primitive(ixi^l, ixo^l, w, x)
    end if
 
  end subroutine rhd_to_primitive
 
  !> Transform internal energy to total energy
  subroutine rhd_ei_to_e(ixI^L,ixO^L,w,x)
    use mod_global_parameters
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(inout) :: w(ixi^s, nw)
    double precision, intent(in)    :: x(ixi^s, 1:ndim)
 
    ! Calculate total energy from internal and kinetic energy
    w(ixo^s,e_)=w(ixo^s,e_)&
               +rhd_kin_en(w,ixi^l,ixo^l)
 
  end subroutine rhd_ei_to_e
 
  !> Transform total energy to internal energy
  subroutine rhd_e_to_ei(ixI^L,ixO^L,w,x)
    use mod_global_parameters
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(inout) :: w(ixi^s, nw)
    double precision, intent(in)    :: x(ixi^s, 1:ndim)
 
    ! Calculate ei = e - ek
    w(ixo^s,e_)=w(ixo^s,e_)&
                -rhd_kin_en(w,ixi^l,ixo^l)
 
  end subroutine rhd_e_to_ei
 
  subroutine e_to_rhos(ixI^L, ixO^L, w, x)
    use mod_global_parameters
 
    integer, intent(in)          :: ixi^l, ixo^l
    double precision             :: w(ixi^s, nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
 
    if (rhd_energy) then
       w(ixo^s, e_) = (rhd_gamma - 1.0d0) * w(ixo^s, rho_)**(1.0d0 - rhd_gamma) * &
            (w(ixo^s, e_) - rhd_kin_en(w, ixi^l, ixo^l))
    else
       call mpistop("energy from entropy can not be used with -eos = iso !")
    end if
  end subroutine e_to_rhos
 
  subroutine rhos_to_e(ixI^L, ixO^L, w, x)
    use mod_global_parameters
 
    integer, intent(in)          :: ixi^l, ixo^l
    double precision             :: w(ixi^s, nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
 
    if (rhd_energy) then
       w(ixo^s, e_) = w(ixo^s, rho_)**(rhd_gamma - 1.0d0) * w(ixo^s, e_) &
            / (rhd_gamma - 1.0d0) + rhd_kin_en(w, ixi^l, ixo^l)
    else
       call mpistop("entropy from energy can not be used with -eos = iso !")
    end if
  end subroutine rhos_to_e
 
  !> Calculate v_i = m_i / rho within ixO^L
  subroutine rhd_get_v(w, x, ixI^L, ixO^L, idim, v)
    use mod_global_parameters
    integer, intent(in)           :: ixi^l, ixo^l, idim
    double precision, intent(in)  :: w(ixi^s, nw), x(ixi^s, 1:ndim)
    double precision, intent(out) :: v(ixi^s)
 
    v(ixo^s) = w(ixo^s, mom(idim)) / w(ixo^s, rho_)
  end subroutine rhd_get_v
 
  !> Calculate cmax_idim = csound + abs(v_idim) within ixO^L
  subroutine rhd_get_cmax(w, x, ixI^L, ixO^L, idim, cmax)
    use mod_global_parameters
    use mod_usr_methods, only: usr_set_pthermal
    use mod_dust, only: dust_get_cmax_prim
 
    integer, intent(in)                       :: ixi^l, ixo^l, idim
    ! w in primitive form
    double precision, intent(in)              :: w(ixi^s, nw), x(ixi^s, 1:ndim)
    double precision, intent(inout)           :: cmax(ixi^s)
 
    if(rhd_energy) then
      cmax(ixo^s)=dabs(w(ixo^s,mom(idim)))+dsqrt(rhd_gamma*w(ixo^s,p_)/w(ixo^s,rho_))
    else
      if (.not. associated(usr_set_pthermal)) then
        select case (rhd_pressure)
         case ('Trad')
          cmax(ixo^s) = (w(ixo^s,r_e)*unit_pressure/const_rad_a)**0.25d0&
          /unit_temperature*w(ixo^s, rho_)
         case ('adiabatic')
          cmax(ixo^s) = rhd_adiab * w(ixo^s, rho_)**rhd_gamma
         case ('Tcond') !> Thermal conduction?!
          cmax(ixo^s) = (rhd_gamma-1.d0)*w(ixo^s,r_e)
         case default
          call mpistop('rhd_pressure unknown, use Trad or adiabatic')
         end select
      else
         call usr_set_pthermal(w,x,ixi^l,ixo^l,cmax)
      end if
      cmax(ixo^s)=dabs(w(ixo^s,mom(idim)))+dsqrt(rhd_gamma*cmax(ixo^s)/w(ixo^s,rho_))
    end if
 
    if (rhd_dust) then
      call dust_get_cmax_prim(w, x, ixi^l, ixo^l, idim, cmax)
    end if
  end subroutine rhd_get_cmax
 
  subroutine rhd_get_a2max(w,x,ixI^L,ixO^L,a2max)
    use mod_global_parameters
 
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, nw), x(ixi^s,1:ndim)
    double precision, intent(inout) :: a2max(ndim)
    double precision :: a2(ixi^s,ndim,nw)
    integer :: gxo^l,hxo^l,jxo^l,kxo^l,i,j
 
    a2=zero
    do i = 1,ndim
      !> 4th order
      hxo^l=ixo^l-kr(i,^d);
      gxo^l=hxo^l-kr(i,^d);
      jxo^l=ixo^l+kr(i,^d);
      kxo^l=jxo^l+kr(i,^d);
      a2(ixo^s,i,1:nw)=dabs(-w(kxo^s,1:nw)+16.d0*w(jxo^s,1:nw)&
        -30.d0*w(ixo^s,1:nw)+16.d0*w(hxo^s,1:nw)-w(gxo^s,1:nw))
      a2max(i)=maxval(a2(ixo^s,i,1:nw))/12.d0/dxlevel(i)**2
    end do
  end subroutine rhd_get_a2max
 
  !> get adaptive cutoff temperature for TRAC (Johnston 2019 ApJL, 873, L22)
  subroutine rhd_get_tcutoff(ixI^L,ixO^L,w,x,tco_local,Tmax_local)
    use mod_global_parameters
    integer, intent(in) :: ixi^l,ixo^l
    double precision, intent(in) :: x(ixi^s,1:ndim)
    double precision, intent(inout) :: w(ixi^s,1:nw)
    double precision, intent(out) :: tco_local, tmax_local
 
    double precision, parameter :: trac_delta=0.25d0
    double precision :: tmp1(ixi^s),te(ixi^s),lts(ixi^s)
    double precision :: ltr(ixi^s),ltrc,ltrp,tcoff(ixi^s)
    integer :: jxo^l,hxo^l
    integer :: jxp^l,hxp^l,ixp^l
    logical :: lrlt(ixi^s)
 
    {^ifoned
    call rhd_get_temperature_from_etot(w,x,ixi^l,ixi^l,te)
 
    tco_local=zero
    tmax_local=maxval(te(ixo^s))
    select case(rhd_trac_type)
    case(0)
      w(ixi^s,tcoff_)=3.d5/unit_temperature
    case(1)
      hxo^l=ixo^l-1;
      jxo^l=ixo^l+1;
      lts(ixo^s)=0.5d0*dabs(te(jxo^s)-te(hxo^s))/te(ixo^s)
      lrlt=.false.
      where(lts(ixo^s) > trac_delta)
        lrlt(ixo^s)=.true.
      end where
      if(any(lrlt(ixo^s))) then
        tco_local=maxval(te(ixo^s), mask=lrlt(ixo^s))
      end if
    case(2)
      !> iijima et al. 2021, LTRAC method
      ltrc=1.5d0
      ltrp=2.5d0
      ixp^l=ixo^l^ladd1;
      hxo^l=ixo^l-1;
      jxo^l=ixo^l+1;
      hxp^l=ixp^l-1;
      jxp^l=ixp^l+1;
      lts(ixp^s)=0.5d0*abs(te(jxp^s)-te(hxp^s))/te(ixp^s)
      ltr(ixp^s)=max(one, (exp(lts(ixp^s))/ltrc)**ltrp)
      w(ixo^s,tcoff_)=te(ixo^s)*&
        (0.25*(ltr(jxo^s)+two*ltr(ixo^s)+ltr(hxo^s)))**0.4d0
    case default
      call mpistop("mrhd_trac_type not allowed for 1D simulation")
    end select
    }
  end subroutine rhd_get_tcutoff
 
  !> Calculate cmax_idim = csound + abs(v_idim) within ixO^L
  subroutine rhd_get_cbounds(wLC, wRC, wLp, wRp, x, ixI^L, ixO^L, idim,Hspeed,cmax, cmin)
    use mod_global_parameters
    use mod_dust, only: dust_get_cmax
    use mod_variables
 
    integer, intent(in)             :: ixi^l, ixo^l, idim
    ! conservative left and right status
    double precision, intent(in)    :: wlc(ixi^s, nw), wrc(ixi^s, nw)
    ! primitive left and right status
    double precision, intent(in)    :: wlp(ixi^s, nw), wrp(ixi^s, nw)
    double precision, intent(in)    :: x(ixi^s, 1:ndim)
    double precision, intent(inout) :: cmax(ixi^s,1:number_species)
    double precision, intent(inout), optional :: cmin(ixi^s,1:number_species)
    double precision, intent(in)    :: hspeed(ixi^s,1:number_species)
 
    double precision :: wmean(ixi^s,nw)
    double precision, dimension(ixI^S) :: umean, dmean, csoundl, csoundr, tmp1,tmp2,tmp3
    integer :: ix^d
 
    select case(boundspeed)
    case (1)
      ! This implements formula (10.52) from "Riemann Solvers and Numerical
      ! Methods for Fluid Dynamics" by Toro.
 
      tmp1(ixo^s)=dsqrt(wlp(ixo^s,rho_))
      tmp2(ixo^s)=dsqrt(wrp(ixo^s,rho_))
      tmp3(ixo^s)=1.d0/(dsqrt(wlp(ixo^s,rho_))+dsqrt(wrp(ixo^s,rho_)))
      umean(ixo^s)=(wlp(ixo^s,mom(idim))*tmp1(ixo^s)+wrp(ixo^s,mom(idim))*tmp2(ixo^s))*tmp3(ixo^s)
 
      if(rhd_energy) then
        csoundl(ixo^s)=rhd_gamma*wlp(ixo^s,p_)/wlp(ixo^s,rho_)
        csoundr(ixo^s)=rhd_gamma*wrp(ixo^s,p_)/wrp(ixo^s,rho_)
      else
        select case (rhd_pressure)
        case ('Trad')
          csoundl(ixo^s)=rhd_gamma*kbmpmua4*wlp(ixo^s,r_e)**(1.d0/4)
          csoundr(ixo^s)=rhd_gamma*kbmpmua4*wrp(ixo^s,r_e)**(1.d0/4)
        case ('adiabatic')
          csoundl(ixo^s)=rhd_gamma*rhd_adiab*wlp(ixo^s,rho_)**(rhd_gamma-one)
          csoundr(ixo^s)=rhd_gamma*rhd_adiab*wrp(ixo^s,rho_)**(rhd_gamma-one)
        end select
      end if
 
      dmean(ixo^s) = (tmp1(ixo^s)*csoundl(ixo^s)+tmp2(ixo^s)*csoundr(ixo^s)) * &
           tmp3(ixo^s) + 0.5d0*tmp1(ixo^s)*tmp2(ixo^s)*tmp3(ixo^s)**2 * &
           (wrp(ixo^s,mom(idim))-wlp(ixo^s,mom(idim)))**2
 
      dmean(ixo^s)=dsqrt(dmean(ixo^s))
      if(present(cmin)) then
        cmin(ixo^s,1)=umean(ixo^s)-dmean(ixo^s)
        cmax(ixo^s,1)=umean(ixo^s)+dmean(ixo^s)
        if(h_correction) then
          {do ix^db=ixomin^db,ixomax^db\}
            cmin(ix^d,1)=sign(one,cmin(ix^d,1))*max(abs(cmin(ix^d,1)),hspeed(ix^d,1))
            cmax(ix^d,1)=sign(one,cmax(ix^d,1))*max(abs(cmax(ix^d,1)),hspeed(ix^d,1))
          {end do\}
        end if
      else
        cmax(ixo^s,1)=dabs(umean(ixo^s))+dmean(ixo^s)
      end if
 
      if (rhd_dust) then
        wmean(ixo^s,1:nwflux)=0.5d0*(wlc(ixo^s,1:nwflux)+wrc(ixo^s,1:nwflux))
        call dust_get_cmax(wmean, x, ixi^l, ixo^l, idim, cmax, cmin)
      end if
 
    case (2)
      wmean(ixo^s,1:nwflux)=0.5d0*(wlc(ixo^s,1:nwflux)+wrc(ixo^s,1:nwflux))
      tmp1(ixo^s)=wmean(ixo^s,mom(idim))/wmean(ixo^s,rho_)
      call rhd_get_csound2(wmean,x,ixi^l,ixo^l,csoundr)
      csoundr(ixo^s) = dsqrt(csoundr(ixo^s))
 
      if(present(cmin)) then
        cmax(ixo^s,1)=max(tmp1(ixo^s)+csoundr(ixo^s),zero)
        cmin(ixo^s,1)=min(tmp1(ixo^s)-csoundr(ixo^s),zero)
        if(h_correction) then
          {do ix^db=ixomin^db,ixomax^db\}
            cmin(ix^d,1)=sign(one,cmin(ix^d,1))*max(abs(cmin(ix^d,1)),hspeed(ix^d,1))
            cmax(ix^d,1)=sign(one,cmax(ix^d,1))*max(abs(cmax(ix^d,1)),hspeed(ix^d,1))
          {end do\}
        end if
      else
        cmax(ixo^s,1)=dabs(tmp1(ixo^s))+csoundr(ixo^s)
      end if
 
      if (rhd_dust) then
        call dust_get_cmax(wmean, x, ixi^l, ixo^l, idim, cmax, cmin)
      end if
    case (3)
      ! Miyoshi 2005 JCP 208, 315 equation (67)
      if(rhd_energy) then
        csoundl(ixo^s)=rhd_gamma*wlp(ixo^s,p_)/wlp(ixo^s,rho_)
        csoundr(ixo^s)=rhd_gamma*wrp(ixo^s,p_)/wrp(ixo^s,rho_)
      else
        select case (rhd_pressure)
        case ('Trad')
          csoundl(ixo^s)=rhd_gamma*kbmpmua4*wlp(ixo^s,r_e)**(1.d0/4)
          csoundr(ixo^s)=rhd_gamma*kbmpmua4*wrp(ixo^s,r_e)**(1.d0/4)
        case ('adiabatic')
          csoundl(ixo^s)=rhd_gamma*rhd_adiab*wlp(ixo^s,rho_)**(rhd_gamma-one)
          csoundr(ixo^s)=rhd_gamma*rhd_adiab*wrp(ixo^s,rho_)**(rhd_gamma-one)
        end select
      end if
      csoundl(ixo^s)=max(dsqrt(csoundl(ixo^s)),dsqrt(csoundr(ixo^s)))
      if(present(cmin)) then
        cmin(ixo^s,1)=min(wlp(ixo^s,mom(idim)),wrp(ixo^s,mom(idim)))-csoundl(ixo^s)
        cmax(ixo^s,1)=max(wlp(ixo^s,mom(idim)),wrp(ixo^s,mom(idim)))+csoundl(ixo^s)
        if(h_correction) then
          {do ix^db=ixomin^db,ixomax^db\}
            cmin(ix^d,1)=sign(one,cmin(ix^d,1))*max(abs(cmin(ix^d,1)),hspeed(ix^d,1))
            cmax(ix^d,1)=sign(one,cmax(ix^d,1))*max(abs(cmax(ix^d,1)),hspeed(ix^d,1))
          {end do\}
        end if
      else
        cmax(ixo^s,1)=max(wlp(ixo^s,mom(idim)),wrp(ixo^s,mom(idim)))+csoundl(ixo^s)
      end if
      if (rhd_dust) then
        wmean(ixo^s,1:nwflux)=0.5d0*(wlc(ixo^s,1:nwflux)+wrc(ixo^s,1:nwflux))
        call dust_get_cmax(wmean, x, ixi^l, ixo^l, idim, cmax, cmin)
      end if
    end select
 
  end subroutine rhd_get_cbounds
 
  !> Calculate the square of the thermal sound speed csound2 within ixO^L.
  !> csound2=gamma*p/rho
  subroutine rhd_get_csound2(w,x,ixI^L,ixO^L,csound2)
    use mod_global_parameters
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(in)    :: w(ixi^s,nw)
    double precision, intent(in)    :: x(ixi^s,1:ndim)
    double precision, intent(out)   :: csound2(ixi^s)
 
    call rhd_get_ptot(w,x,ixi^l,ixo^l,csound2)
    csound2(ixo^s)=max(rhd_gamma,4.d0/3.d0)*csound2(ixo^s)/w(ixo^s,rho_)
    !> Turner & Stone 2001
 
  end subroutine rhd_get_csound2
 
  !> Calculate thermal pressure=(gamma-1)*(e-0.5*m**2/rho) within ixO^L
  subroutine rhd_get_pthermal(w, x, ixI^L, ixO^L, pth)
    use mod_global_parameters
    use mod_usr_methods, only: usr_set_pthermal
    use mod_small_values, only: trace_small_values
 
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, 1:nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
    double precision, intent(out):: pth(ixi^s)
    integer                      :: iw, ix^d
 
    if (rhd_energy) then
       pth(ixi^s) = (rhd_gamma - 1.d0) * (w(ixi^s, e_) - &
            0.5d0 * sum(w(ixi^s, mom(:))**2, dim=ndim+1) / w(ixi^s, rho_))
    else
       if (.not. associated(usr_set_pthermal)) then
         select case (rhd_pressure)
          case ('Trad')
           pth(ixi^s) = (w(ixi^s,r_e)*unit_pressure/const_rad_a)**0.25d0&
           /unit_temperature*w(ixi^s, rho_)
          case ('adiabatic')
           pth(ixi^s) = rhd_adiab * w(ixi^s, rho_)**rhd_gamma
          case ('Tcond') !> Thermal conduction?!
           pth(ixi^s) = (rhd_gamma-1.d0)*w(ixi^s,r_e)
          case default
           call mpistop('rhd_pressure unknown, use Trad or adiabatic')
          end select
       else
          call usr_set_pthermal(w,x,ixi^l,ixo^l,pth)
       end if
    end if
 
    if (fix_small_values) then
      {do ix^db= ixo^lim^db\}
         if(pth(ix^d)<small_pressure) then
            pth(ix^d)=small_pressure
         endif
      {enddo^d&\}
    else if (check_small_values) then
      {do ix^db= ixo^lim^db\}
         if(pth(ix^d)<small_pressure) then
           write(*,*) "Error: small value of gas pressure",pth(ix^d),&
                " encountered when call rhd_get_pthermal"
           write(*,*) "Iteration: ", it, " Time: ", global_time
           write(*,*) "Location: ", x(ix^d,:)
           write(*,*) "Cell number: ", ix^d
           do iw=1,nw
             write(*,*) trim(cons_wnames(iw)),": ",w(ix^d,iw)
           end do
           ! use erroneous arithmetic operation to crash the run
           if(trace_small_values) write(*,*) dsqrt(pth(ix^d)-bigdouble)
           write(*,*) "Saving status at the previous time step"
           crash=.true.
         end if
      {enddo^d&\}
    end if
 
  end subroutine rhd_get_pthermal
 
  !> Calculate radiation pressure within ixO^L
  subroutine rhd_get_pradiation(w, x, ixI^L, ixO^L, prad)
    use mod_global_parameters
    use mod_fld
    use mod_afld
 
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, 1:nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
    double precision, intent(out):: prad(ixo^s, 1:ndim, 1:ndim)
 
    select case (rhd_radiation_formalism)
    case('fld')
      call fld_get_radpress(w, x, ixi^l, ixo^l, prad, nghostcells)
    case('afld')
      call afld_get_radpress(w, x, ixi^l, ixo^l, prad, nghostcells)
    case default
      call mpistop('Radiation formalism unknown')
    end select
  end subroutine rhd_get_pradiation
 
  !> calculates the sum of the gas pressure and max Prad tensor element
  subroutine rhd_get_ptot(w, x, ixI^L, ixO^L, ptot)
    use mod_global_parameters
 
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, 1:nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
    double precision             :: pth(ixi^s)
    double precision             :: prad_tensor(ixo^s, 1:ndim, 1:ndim)
    double precision             :: prad_max(ixo^s)
    double precision, intent(out):: ptot(ixi^s)
    integer :: ix^d
 
    call rhd_get_pthermal(w, x, ixi^l, ixo^l, pth)
    call rhd_get_pradiation(w, x, ixi^l, ixo^l, prad_tensor)
 
    {do ix^d = ixomin^d,ixomax^d\}
      prad_max(ix^d) = maxval(prad_tensor(ix^d,:,:))
    {enddo\}
 
    !> filter cmax
    if (radio_acoustic_filter) then
      call rhd_radio_acoustic_filter(x, ixi^l, ixo^l, prad_max)
    endif
 
    ptot(ixo^s) = pth(ixo^s) + prad_max(ixo^s)
 
  end subroutine rhd_get_ptot
 
  !> Filter peaks in cmax due to radiation energy density, used for debugging
  subroutine rhd_radio_acoustic_filter(x, ixI^L, ixO^L, prad_max)
    use mod_global_parameters
 
    integer, intent(in)                       :: ixi^l, ixo^l
    double precision, intent(in)              :: x(ixi^s, 1:ndim)
    double precision, intent(inout)           :: prad_max(ixo^s)
 
    double precision :: tmp_prad(ixi^s)
    integer :: ix^d, filter, idim
 
    if (size_ra_filter .lt. 1) call mpistop("ra filter of size < 1 makes no sense")
    if (size_ra_filter .gt. nghostcells) call mpistop("ra filter of size < nghostcells makes no sense")
 
    tmp_prad(ixi^s) = zero
    tmp_prad(ixo^s) = prad_max(ixo^s)
 
    do filter = 1,size_ra_filter
      do idim = 1,ndim
        ! {do ix^D = ixOmin^D+filter,ixOmax^D-filter\}
        {do ix^d = ixomin^d,ixomax^d\}
            prad_max(ix^d) = min(tmp_prad(ix^d),tmp_prad(ix^d+filter*kr(idim,^d)))
            prad_max(ix^d) = min(tmp_prad(ix^d),tmp_prad(ix^d-filter*kr(idim,^d)))
        {enddo\}
      enddo
    enddo
  end subroutine rhd_radio_acoustic_filter
 
  !> Calculate temperature=p/rho when in e_ the  total energy is stored
  subroutine rhd_get_temperature_from_etot(w, x, ixI^L, ixO^L, res)
    use mod_global_parameters
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, 1:nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
    double precision, intent(out):: res(ixi^s)
 
    double precision :: r(ixi^s)
 
    call rhd_get_rfactor(w,x,ixi^l,ixo^l,r)
    call rhd_get_pthermal(w, x, ixi^l, ixo^l, res)
    res(ixo^s)=res(ixo^s)/(r(ixo^s)*w(ixo^s,rho_))
  end subroutine rhd_get_temperature_from_etot
 
 
  !> Calculate temperature=p/rho when in e_ the  internal energy is stored
  subroutine rhd_get_temperature_from_eint(w, x, ixI^L, ixO^L, res)
    use mod_global_parameters
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, 1:nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
    double precision, intent(out):: res(ixi^s)
    double precision :: r(ixi^s)
 
    call rhd_get_rfactor(w,x,ixi^l,ixo^l,r)
    res(ixo^s) = (rhd_gamma - 1.0d0) * w(ixo^s, e_)/(w(ixo^s,rho_)*r(ixo^s))
  end subroutine rhd_get_temperature_from_eint
 
  !> Calculates gas temperature
  subroutine rhd_get_tgas(w, x, ixI^L, ixO^L, tgas)
    use mod_global_parameters
 
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, 1:nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
    double precision             :: pth(ixi^s)
    double precision, intent(out):: tgas(ixi^s)
 
    call rhd_get_pthermal(w, x, ixi^l, ixo^l, pth)
    tgas(ixi^s) = pth(ixi^s)/w(ixi^s,rho_)
 
  end subroutine rhd_get_tgas
 
  !> Calculates radiation temperature
  subroutine rhd_get_trad(w, x, ixI^L, ixO^L, trad)
    use mod_global_parameters
    use mod_constants
 
    integer, intent(in)          :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s, 1:nw)
    double precision, intent(in) :: x(ixi^s, 1:ndim)
    double precision, intent(out):: trad(ixi^s)
 
    trad(ixi^s) = (w(ixi^s,r_e)*unit_pressure&
    /const_rad_a)**(1.d0/4.d0)/unit_temperature
 
  end subroutine rhd_get_trad
 
 
  !these are very similar to the subroutines without 1, used in mod_thermal_conductivity
  !but no check on whether energy variable is present
  subroutine rhd_ei_to_e1(ixI^L,ixO^L,w,x)
    use mod_global_parameters
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(inout) :: w(ixi^s, nw)
    double precision, intent(in)    :: x(ixi^s, 1:ndim)
 
    ! Calculate total energy from internal and kinetic energy
    w(ixo^s,e_)=w(ixo^s,e_)&
                 +rhd_kin_en(w,ixi^l,ixo^l)
 
  end subroutine rhd_ei_to_e1
 
  !> Transform total energy to internal energy
  !but no check on whether energy variable is present
  subroutine rhd_e_to_ei1(ixI^L,ixO^L,w,x)
    use mod_global_parameters
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(inout) :: w(ixi^s, nw)
    double precision, intent(in)    :: x(ixi^s, 1:ndim)
 
    ! Calculate ei = e - ek
    w(ixo^s,e_)=w(ixo^s,e_)&
                  -rhd_kin_en(w,ixi^l,ixo^l)
 
  end subroutine rhd_e_to_ei1
 
  ! Calculate flux f_idim[iw]
  subroutine rhd_get_flux_cons(w, x, ixI^L, ixO^L, idim, f)
    use mod_global_parameters
    use mod_dust, only: dust_get_flux
 
    integer, intent(in)             :: ixi^l, ixo^l, idim
    double precision, intent(in)    :: w(ixi^s, 1:nw), x(ixi^s, 1:ndim)
    double precision, intent(out)   :: f(ixi^s, nwflux)
    double precision                :: pth(ixi^s), v(ixi^s),frame_vel(ixi^s)
    integer                         :: idir, itr
 
    call rhd_get_pthermal(w, x, ixi^l, ixo^l, pth)
    call rhd_get_v(w, x, ixi^l, ixo^l, idim, v)
 
    f(ixo^s, rho_) = v(ixo^s) * w(ixo^s, rho_)
 
    ! Momentum flux is v_i*m_i, +p in direction idim
    do idir = 1, ndir
       f(ixo^s, mom(idir)) = v(ixo^s) * w(ixo^s, mom(idir))
    end do
 
    f(ixo^s, mom(idim)) = f(ixo^s, mom(idim)) + pth(ixo^s)
 
    if(rhd_energy) then
      ! Energy flux is v_i*(e + p)
      f(ixo^s, e_) = v(ixo^s) * (w(ixo^s, e_) + pth(ixo^s))
    end if
 
    if (rhd_radiation_advection) then
      f(ixo^s, r_e) = v(ixo^s) * w(ixo^s,r_e)
    else
      f(ixo^s, r_e) = zero
    endif
 
    do itr = 1, rhd_n_tracer
       f(ixo^s, tracer(itr)) = v(ixo^s) * w(ixo^s, tracer(itr))
    end do
 
    ! Dust fluxes
    if (rhd_dust) then
      call dust_get_flux(w, x, ixi^l, ixo^l, idim, f)
    end if
 
  end subroutine rhd_get_flux_cons
 
  ! Calculate flux f_idim[iw]
  subroutine rhd_get_flux(wC, w, x, ixI^L, ixO^L, idim, f)
    use mod_global_parameters
    use mod_dust, only: dust_get_flux_prim
 
    integer, intent(in)             :: ixi^l, ixo^l, idim
    ! conservative w
    double precision, intent(in)    :: wc(ixi^s, 1:nw)
    ! primitive w
    double precision, intent(in)    :: w(ixi^s, 1:nw)
    double precision, intent(in)    :: x(ixi^s, 1:ndim)
    double precision, intent(out)   :: f(ixi^s, nwflux)
    double precision                :: pth(ixi^s),frame_vel(ixi^s)
    integer                         :: idir, itr
 
    if (rhd_energy) then
       pth(ixo^s) = w(ixo^s,p_)
    else
       call rhd_get_pthermal(wc, x, ixi^l, ixo^l, pth)
    end if
 
    f(ixo^s, rho_) = w(ixo^s,mom(idim)) * w(ixo^s, rho_)
 
    ! Momentum flux is v_i*m_i, +p in direction idim
    do idir = 1, ndir
       f(ixo^s, mom(idir)) = w(ixo^s,mom(idim)) * wc(ixo^s, mom(idir))
    end do
 
    f(ixo^s, mom(idim)) = f(ixo^s, mom(idim)) + pth(ixo^s)
 
    if(rhd_energy) then
      ! Energy flux is v_i*(e + p)
      f(ixo^s, e_) = w(ixo^s,mom(idim)) * (wc(ixo^s, e_) + w(ixo^s,p_))
    end if
 
    if (rhd_radiation_advection) then
      f(ixo^s, r_e) = w(ixo^s,mom(idim)) * wc(ixo^s,r_e)
    else
      f(ixo^s, r_e) = zero
    endif
 
    do itr = 1, rhd_n_tracer
       f(ixo^s, tracer(itr)) = w(ixo^s,mom(idim)) * w(ixo^s, tracer(itr))
    end do
 
    ! Dust fluxes
    if (rhd_dust) then
      call dust_get_flux_prim(w, x, ixi^l, ixo^l, idim, f)
    end if
 
  end subroutine rhd_get_flux
 
  !> Add geometrical source terms to w
  !>
  !> Notice that the expressions of the geometrical terms depend only on ndir,
  !> not ndim. Eg, they are the same in 2.5D and in 3D, for any geometry.
  !>
  subroutine rhd_add_source_geom(qdt, dtfactor, ixI^L, ixO^L, wCT, wprim, w, x)
    use mod_global_parameters
    use mod_usr_methods, only: usr_set_surface, usr_set_pthermal
    use mod_rotating_frame, only: rotating_frame_add_source
    use mod_dust, only: dust_n_species, dust_mom, dust_rho
    use mod_geometry
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(in)    :: qdt, dtfactor, x(ixi^s, 1:ndim)
    double precision, intent(inout) :: wct(ixi^s, 1:nw), wprim(ixi^s,1:nw), w(ixi^s, 1:nw)
    ! to change and to set as a parameter in the parfile once the possibility to
    ! solve the equations in an angular momentum conserving form has been
    ! implemented (change tvdlf.t eg)
    double precision :: pth(ixi^s), source(ixi^s), minrho
    integer                         :: iw,idir, h1x^l{^nooned, h2x^l}
    integer :: mr_,mphi_ ! Polar var. names
    integer :: irho, ifluid, n_fluids
    double precision :: exp_factor(ixi^s), del_exp_factor(ixi^s), exp_factor_primitive(ixi^s)
 
    if (rhd_dust) then
       n_fluids = 1 + dust_n_species
    else
       n_fluids = 1
    end if
 
    select case (coordinate)
 
    case(cartesian_expansion)
      !the user provides the functions of exp_factor and del_exp_factor
      if(associated(usr_set_surface)) call usr_set_surface(ixi^l,x,block%dx,exp_factor,del_exp_factor,exp_factor_primitive)
      if(rhd_energy) then
        source(ixo^s) =wprim(ixo^s, p_)
      else
        if(.not. associated(usr_set_pthermal)) then
          source(ixo^s)=rhd_adiab * wprim(ixo^s, rho_)**rhd_gamma
        else
          call usr_set_pthermal(wct,x,ixi^l,ixo^l,source)
        end if
      end if
      source(ixo^s) = source(ixo^s)*del_exp_factor(ixo^s)/exp_factor(ixo^s)
      w(ixo^s,mom(1)) = w(ixo^s,mom(1)) + qdt*source(ixo^s)
 
    case (cylindrical)
      if ((rhd_radiation_formalism .eq. 'fld') .or. (rhd_radiation_formalism .eq. 'afld')) then
       call mpistop("Diffusion term not implemented yet with cylkindrical geometries")
      end if
 
       do ifluid = 0, n_fluids-1
          ! s[mr]=(pthermal+mphi**2/rho)/radius
          if (ifluid == 0) then
            ! gas
            irho  = rho_
            mr_   = mom(r_)
            if(phi_>0) mphi_ = mom(phi_)
            if(rhd_energy) then
              source(ixo^s) =wprim(ixo^s, p_)
            else
              if(.not. associated(usr_set_pthermal)) then
                source(ixo^s)=rhd_adiab * wprim(ixo^s, rho_)**rhd_gamma
              else
                call usr_set_pthermal(wct,x,ixi^l,ixo^l,source)
              end if
            end if
            minrho = 0.0d0
          else
             ! dust : no pressure
             irho  = dust_rho(ifluid)
             mr_   = dust_mom(r_, ifluid)
             if(phi_>0) mphi_ = dust_mom(phi_, ifluid)
             source(ixi^s) = zero
             minrho = 0.0d0
          end if
          if (phi_ > 0) then
            source(ixo^s) = source(ixo^s) + wprim(ixo^s, mphi_)**2 * wprim(ixo^s, irho)
            w(ixo^s, mr_) = w(ixo^s, mr_) + qdt * source(ixo^s) / x(ixo^s, r_)
         ! s[mphi]=(-vphi*vr*rho)/radius
            source(ixo^s) = -wprim(ixo^s, mphi_) * wprim(ixo^s, mr_) * wprim(ixo^s, irho)
            w(ixo^s, mphi_) = w(ixo^s, mphi_) + qdt * source(ixo^s) / x(ixo^s, r_)
          else
            ! s[mr]=2pthermal/radius
            w(ixo^s, mr_) = w(ixo^s, mr_) + qdt * source(ixo^s) / x(ixo^s, r_)
          end if
       end do
    case (spherical)
 
       if ((rhd_radiation_formalism .eq. 'fld') .or. (rhd_radiation_formalism .eq. 'afld')) then
        call mpistop("Diffusion term not implemented yet with spherical geometries")
       end if
 
       if (rhd_dust) then
          call mpistop("Dust geom source terms not implemented yet with spherical geometries")
       end if
       mr_   = mom(r_)
       if(phi_>0) mphi_ = mom(phi_)
       h1x^l=ixo^l-kr(1,^d); {^nooned h2x^l=ixo^l-kr(2,^d);}
       ! s[mr]=((vtheta**2+vphi**2)*rho+2*p)/r
       if(rhd_energy) then
         pth(ixo^s) =wprim(ixo^s, p_)
       else
         if(.not. associated(usr_set_pthermal)) then
           pth(ixo^s)=rhd_adiab * wprim(ixo^s, rho_)**rhd_gamma
         else
           call usr_set_pthermal(wct,x,ixi^l,ixo^l,pth)
         end if
       end if
       source(ixo^s) = pth(ixo^s) * x(ixo^s, 1) &
            *(block%surfaceC(ixo^s, 1) - block%surfaceC(h1x^s, 1)) &
            /block%dvolume(ixo^s)
       do idir = 2, ndir
         source(ixo^s) = source(ixo^s) + wprim(ixo^s, mom(idir))**2 * wprim(ixo^s, rho_)
       end do
       w(ixo^s, mr_) = w(ixo^s, mr_) + qdt * source(ixo^s) / x(ixo^s, 1)
 
       {^nooned
       ! s[mtheta]=-(vr*vtheta*rho)/r+cot(theta)*(vphi**2*rho+p)/r
       source(ixo^s) = pth(ixo^s) * x(ixo^s, 1) &
            * (block%surfaceC(ixo^s, 2) - block%surfaceC(h2x^s, 2)) &
            / block%dvolume(ixo^s)
       if (ndir == 3) then
          source(ixo^s) = source(ixo^s) + (wprim(ixo^s, mom(3))**2 * wprim(ixo^s, rho_)) / tan(x(ixo^s, 2))
       end if
       source(ixo^s) = source(ixo^s) - (wprim(ixo^s, mom(2)) * wprim(ixo^s, mr_)) * wprim(ixo^s, rho_)
       w(ixo^s, mom(2)) = w(ixo^s, mom(2)) + qdt * source(ixo^s) / x(ixo^s, 1)
 
       if (ndir == 3) then
         ! s[mphi]=-(vphi*vr/rho)/r-cot(theta)*(vtheta*vphi/rho)/r
         source(ixo^s) = -(wprim(ixo^s, mom(3)) * wprim(ixo^s, mr_)) * wprim(ixo^s, rho_)&
                        - (wprim(ixo^s, mom(2)) * wprim(ixo^s, mom(3))) * wprim(ixo^s, rho_) / tan(x(ixo^s, 2))
         w(ixo^s, mom(3)) = w(ixo^s, mom(3)) + qdt * source(ixo^s) / x(ixo^s, 1)
       end if
       }
    end select
 
    if (rhd_rotating_frame) then
       if (rhd_dust) then
          call mpistop("Rotating frame not implemented yet with dust")
       else
          call rotating_frame_add_source(qdt,dtfactor,ixi^l,ixo^l,wprim,w,x)
       end if
    end if
 
  end subroutine rhd_add_source_geom
 
  ! w[iw]= w[iw]+qdt*S[wCT, qtC, x] where S is the source based on wCT within ixO
  subroutine rhd_add_source(qdt,dtfactor,ixI^L,ixO^L,wCT,wCTprim,w,x,qsourcesplit,active)
    use mod_global_parameters
    use mod_radiative_cooling, only: radiative_cooling_add_source
    use mod_dust, only: dust_add_source, dust_mom, dust_rho, dust_n_species
    use mod_viscosity, only: viscosity_add_source
    use mod_usr_methods, only: usr_gravity
    use mod_gravity, only: gravity_add_source, grav_split
 
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(in)    :: qdt,dtfactor
    double precision, intent(in)    :: wct(ixi^s, 1:nw),wctprim(ixi^s,1:nw),x(ixi^s, 1:ndim)
    double precision, intent(inout) :: w(ixi^s, 1:nw)
    logical, intent(in)             :: qsourcesplit
    logical, intent(inout)          :: active
 
    double precision :: gravity_field(ixi^s, 1:ndim)
    integer :: idust, idim
 
    if(rhd_dust) then
      call dust_add_source(qdt,ixi^l,ixo^l,wct,w,x,qsourcesplit,active)
    end if
 
    if(rhd_radiative_cooling) then
      call radiative_cooling_add_source(qdt,ixi^l,ixo^l,wct,wctprim,w,x,&
           qsourcesplit,active, rc_fl)
    end if
 
    if(rhd_viscosity) then
      call viscosity_add_source(qdt,ixi^l,ixo^l,wct,wctprim,w,x,&
           rhd_energy,qsourcesplit,active)
    end if
 
    if (rhd_gravity) then
      call gravity_add_source(qdt,ixi^l,ixo^l,wct,wctprim,w,x,&
           rhd_energy,qsourcesplit,active)
 
      if (rhd_dust .and. qsourcesplit .eqv. grav_split) then
         active = .true.
 
         call usr_gravity(ixi^l, ixo^l, wct, x, gravity_field)
         do idust = 1, dust_n_species
            do idim = 1, ndim
               w(ixo^s, dust_mom(idim, idust)) = w(ixo^s, dust_mom(idim, idust)) &
                    + qdt * gravity_field(ixo^s, idim) * wct(ixo^s, dust_rho(idust))
            end do
         end do
      end if
    end if
 
    !> This is where the radiation force and heating/cooling are added/
    call rhd_add_radiation_source(qdt,ixi^l,ixo^l,wct,w,x,qsourcesplit,active)
 
    if(rhd_partial_ionization) then
      if(.not.qsourcesplit) then
        active = .true.
        call rhd_update_temperature(ixi^l,ixo^l,wct,w,x)
      end if
    end if
 
  end subroutine rhd_add_source
 
  subroutine rhd_add_radiation_source(qdt,ixI^L,ixO^L,wCT,w,x,qsourcesplit,active)
    use mod_constants
    use mod_global_parameters
    use mod_usr_methods
    use mod_fld!, only: fld_get_diffcoef_central, get_fld_rad_force, get_fld_energy_interact
    use mod_afld!, only: afld_get_diffcoef_central, get_afld_rad_force, get_afld_energy_interact
 
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(in)    :: qdt, x(ixi^s,1:ndim)
    double precision, intent(in)    :: wct(ixi^s,1:nw)
    double precision, intent(inout) :: w(ixi^s,1:nw)
    logical, intent(in) :: qsourcesplit
    logical, intent(inout) :: active
    double precision :: cmax(ixi^s)
 
    select case(rhd_radiation_formalism)
    case('fld')
      if(fld_diff_scheme .eq. 'mg') call fld_get_diffcoef_central(w, wct, x, ixi^l, ixo^l)
      !> radiation force
      if(rhd_radiation_force) call get_fld_rad_force(qdt,ixi^l,ixo^l,wct,w,x,&
        rhd_energy,qsourcesplit,active)
      call rhd_handle_small_values(.true., w, x, ixi^l, ixo^l, 'fld_e_interact')
    case('afld')
      if (fld_diff_scheme .eq. 'mg') call afld_get_diffcoef_central(w, wct, x, ixi^l, ixo^l)
      !> radiation force
      if (rhd_radiation_force) call get_afld_rad_force(qdt,ixi^l,ixo^l,wct,w,x,&
        rhd_energy,qsourcesplit,active)
      call rhd_handle_small_values(.true., w, x, ixi^l, ixo^l, 'fld_e_interact')
      !> photon tiring, heating and cooling
      if (rhd_energy) then
      if (rhd_energy_interact) call get_afld_energy_interact(qdt,ixi^l,ixo^l,wct,w,x,&
        rhd_energy,qsourcesplit,active)
      endif
    case default
      call mpistop('Radiation formalism unknown')
    end select
 
    ! ! !>  NOT necessary for calculation, just want to know the grid-dependent-timestep
    ! call rhd_get_cmax(w, x, ixI^L, ixO^L, 2, cmax)
    ! w(ixI^S,i_test) = cmax(ixI^S)
  end subroutine rhd_add_radiation_source
 
  subroutine rhd_get_dt(w, ixI^L, ixO^L, dtnew, dx^D, x)
    use mod_global_parameters
    use mod_dust, only: dust_get_dt
    use mod_viscosity, only: viscosity_get_dt
    use mod_gravity, only: gravity_get_dt
    use mod_fld, only: fld_radforce_get_dt
    use mod_afld, only: afld_radforce_get_dt
 
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(in)    :: dx^d, x(ixi^s, 1:^nd)
    double precision, intent(in)    :: w(ixi^s, 1:nw)
    double precision, intent(inout) :: dtnew
 
    dtnew = bigdouble
 
    if (.not. dt_c) then
 
      if(rhd_dust) then
        call dust_get_dt(w, ixi^l, ixo^l, dtnew, dx^d, x)
      end if
 
      if(rhd_radiation_force) then
        select case(rhd_radiation_formalism)
        case('fld')
          call fld_radforce_get_dt(w,ixi^l,ixo^l,dtnew,dx^d,x)
        case('afld')
          call afld_radforce_get_dt(w,ixi^l,ixo^l,dtnew,dx^d,x)
        case default
          call mpistop('Radiation formalism unknown')
        end select
      endif
 
      if(rhd_viscosity) then
        call viscosity_get_dt(w,ixi^l,ixo^l,dtnew,dx^d,x)
      end if
 
      if(rhd_gravity) then
        call gravity_get_dt(w,ixi^l,ixo^l,dtnew,dx^d,x)
      end if
    else
      {^ifoned dtnew = dx1*unit_velocity/const_c}
      {^nooned dtnew = min(dx^d*unit_velocity/const_c)}
    endif
 
  end subroutine rhd_get_dt
 
  function rhd_kin_en(w, ixI^L, ixO^L, inv_rho) result(ke)
    use mod_global_parameters, only: nw, ndim
    integer, intent(in)                    :: ixi^l, ixo^l
    double precision, intent(in)           :: w(ixi^s, nw)
    double precision                       :: ke(ixo^s)
    double precision, intent(in), optional :: inv_rho(ixo^s)
 
    if (present(inv_rho)) then
       ke = 0.5d0 * sum(w(ixo^s, mom(:))**2, dim=ndim+1) * inv_rho
    else
       ke = 0.5d0 * sum(w(ixo^s, mom(:))**2, dim=ndim+1) / w(ixo^s, rho_)
    end if
  end function rhd_kin_en
 
  function rhd_inv_rho(w, ixI^L, ixO^L) result(inv_rho)
    use mod_global_parameters, only: nw, ndim
    integer, intent(in)           :: ixi^l, ixo^l
    double precision, intent(in)  :: w(ixi^s, nw)
    double precision              :: inv_rho(ixo^s)
 
    ! Can make this more robust
    inv_rho = 1.0d0 / w(ixo^s, rho_)
  end function rhd_inv_rho
 
  subroutine rhd_handle_small_values(primitive, w, x, ixI^L, ixO^L, subname)
    ! handles hydro (density,pressure,velocity) bootstrapping
    ! any negative dust density is flagged as well (and throws an error)
    ! small_values_method=replace also for dust
    use mod_global_parameters
    use mod_small_values
    use mod_dust, only: dust_n_species, dust_mom, dust_rho
    logical, intent(in)             :: primitive
    integer, intent(in)             :: ixi^l,ixo^l
    double precision, intent(inout) :: w(ixi^s,1:nw)
    double precision, intent(in)    :: x(ixi^s,1:ndim)
    character(len=*), intent(in)    :: subname
 
    integer :: n,idir
    logical :: flag(ixi^s,1:nw)
 
    call rhd_check_w(primitive, ixi^l, ixo^l, w, flag)
 
    if (any(flag)) then
      select case (small_values_method)
      case ("replace")
        where(flag(ixo^s,rho_)) w(ixo^s,rho_) = small_density
        do idir = 1, ndir
          if(small_values_fix_iw(mom(idir))) then
            where(flag(ixo^s,rho_)) w(ixo^s, mom(idir)) = 0.0d0
          end if
        end do
 
        if (small_values_fix_iw(r_e)) then
          where(flag(ixo^s,r_e)) w(ixo^s,r_e) = small_r_e
        end if
 
        if(rhd_energy)then
          if(small_values_fix_iw(e_)) then
            if(primitive) then
              where(flag(ixo^s,rho_)) w(ixo^s, p_) = small_pressure
            else
              where(flag(ixo^s,rho_)) w(ixo^s, e_) = small_e + rhd_kin_en(w,ixi^l,ixo^l)
            endif
          end if
        endif
 
        if(rhd_energy) then
          if(primitive) then
            where(flag(ixo^s,e_)) w(ixo^s,p_) = small_pressure
          else
            where(flag(ixo^s,e_))
              ! Add kinetic energy
              w(ixo^s,e_) = small_e + rhd_kin_en(w,ixi^l,ixo^l)
            end where
          end if
        end if
 
        if(rhd_dust)then
           do n=1,dust_n_species
              where(flag(ixo^s,dust_rho(n))) w(ixo^s,dust_rho(n)) = 0.0d0
              do idir = 1, ndir
                  where(flag(ixo^s,dust_rho(n))) w(ixo^s,dust_mom(idir,n)) = 0.0d0
              enddo
           enddo
        endif
      case ("average")
        if(primitive)then
           ! averaging for all primitive fields, including dust
           call small_values_average(ixi^l, ixo^l, w, x, flag)
        else
           ! do averaging of density
           call small_values_average(ixi^l, ixo^l, w, x, flag, rho_)
           if(rhd_energy) then
             ! do averaging of pressure
             w(ixi^s,p_)=(rhd_gamma-1.d0)*(w(ixi^s,e_) &
              -0.5d0*sum(w(ixi^s, mom(:))**2, dim=ndim+1)/w(ixi^s,rho_))
             call small_values_average(ixi^l, ixo^l, w, x, flag, p_)
             w(ixi^s,e_)=w(ixi^s,p_)/(rhd_gamma-1.d0) &
               +0.5d0*sum(w(ixi^s, mom(:))**2, dim=ndim+1)/w(ixi^s,rho_)
           end if
           ! do averaging of radiation energy
           call small_values_average(ixi^l, ixo^l, w, x, flag, r_e)
           if(rhd_dust)then
              do n=1,dust_n_species
                 where(flag(ixo^s,dust_rho(n))) w(ixo^s,dust_rho(n)) = 0.0d0
                 do idir = 1, ndir
                    where(flag(ixo^s,dust_rho(n))) w(ixo^s,dust_mom(idir,n)) = 0.0d0
                 enddo
              enddo
          endif
        endif
      case default
        if(.not.primitive) then
          !convert w to primitive
          ! Calculate pressure = (gamma-1) * (e-ek)
          if(rhd_energy) then
            w(ixo^s,p_)=(rhd_gamma-1.d0)*(w(ixo^s,e_)-rhd_kin_en(w,ixi^l,ixo^l))
          end if
          ! Convert gas momentum to velocity
          do idir = 1, ndir
            w(ixo^s, mom(idir)) = w(ixo^s, mom(idir))/w(ixo^s,rho_)
          end do
        end if
        ! NOTE: dust entries may still have conserved values here
        call small_values_error(w, x, ixi^l, ixo^l, flag, subname)
      end select
    end if
  end subroutine rhd_handle_small_values
 
  subroutine rfactor_from_temperature_ionization(w,x,ixI^L,ixO^L,Rfactor)
    use mod_global_parameters
    use mod_ionization_degree
    integer, intent(in) :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s,1:nw)
    double precision, intent(in) :: x(ixi^s,1:ndim)
    double precision, intent(out):: rfactor(ixi^s)
 
    double precision :: iz_h(ixo^s),iz_he(ixo^s)
 
    call ionization_degree_from_temperature(ixi^l,ixo^l,w(ixi^s,te_),iz_h,iz_he)
    ! assume the first and second ionization of Helium have the same degree
    rfactor(ixo^s)=(1.d0+iz_h(ixo^s)+0.1d0*(1.d0+iz_he(ixo^s)*(1.d0+iz_he(ixo^s))))/2.3d0
 
  end subroutine rfactor_from_temperature_ionization
 
  subroutine rfactor_from_constant_ionization(w,x,ixI^L,ixO^L,Rfactor)
    use mod_global_parameters
    integer, intent(in) :: ixi^l, ixo^l
    double precision, intent(in) :: w(ixi^s,1:nw)
    double precision, intent(in) :: x(ixi^s,1:ndim)
    double precision, intent(out):: rfactor(ixi^s)
 
    rfactor(ixo^s)=rr
 
  end subroutine rfactor_from_constant_ionization
 
  subroutine rhd_update_temperature(ixI^L,ixO^L,wCT,w,x)
    use mod_global_parameters
    use mod_ionization_degree
 
    integer, intent(in)             :: ixi^l, ixo^l
    double precision, intent(in)    :: wct(ixi^s,1:nw), x(ixi^s,1:ndim)
    double precision, intent(inout) :: w(ixi^s,1:nw)
 
    double precision :: iz_h(ixo^s),iz_he(ixo^s), pth(ixi^s)
 
    call ionization_degree_from_temperature(ixi^l,ixo^l,wct(ixi^s,te_),iz_h,iz_he)
 
    call rhd_get_pthermal(w,x,ixi^l,ixo^l,pth)
 
    w(ixo^s,te_)=(2.d0+3.d0*he_abundance)*pth(ixo^s)/(w(ixo^s,rho_)*(1.d0+iz_h(ixo^s)+&
     he_abundance*(iz_he(ixo^s)*(iz_he(ixo^s)+1.d0)+1.d0)))
 
  end subroutine rhd_update_temperature
 
end module mod_rhd_phys