THalofit Class

module: NonLinear file: halofit

Subroutines

conc_bull(this, z, cosm, lut)
- THalofit :: this
- real(dl) intent(in) :: z
- HM_cosmology :: cosm
- HM_tables :: lut
GetNonLinRatios(this, State, CAMB_Pk)

Fill the CAMB_Pk%nonlin_scaling array with sqrt(non-linear power/linear power) for each redshift and wavenumber This implementation uses Halofit $ use omp_lib, only: omp_set_num_threads
- THalofit :: this
- TCAMBdata :: State
- MatterPowerData target :: CAMB_Pk
halofit(this, hf, rk, rn, plin, pnl, pq, ph, rknl, rncur)
- THalofit :: this
- THalofit_zparams intent(in) :: hf
- real(dl) :: rk
- real(dl) :: rn
- real(dl) :: plin
- real(dl) :: pnl
- real(dl) :: pq
- real(dl) :: ph
- real(dl) :: rknl
- real(dl) :: rncur
halomod(this, p1h, p2h, pfull, plin, k, cosm, lut)
- THalofit :: this
- real(dl) intent(out) :: p1h
- real(dl) intent(out) :: p2h
- real(dl) intent(out) :: pfull
- real(dl) intent(in) :: plin
- real(dl) intent(in) :: k
- HM_cosmology intent(in) :: cosm
- HM_tables intent(in) :: lut
halomod_init(this, imead, z, reuse, cosm, lut)
- THalofit :: this
- integer intent(in) :: imead
- real(dl) intent(in) :: z
- logical intent(in), optional :: reuse
- HM_cosmology :: cosm
- HM_tables :: lut
HMcode(this, State, CAMB_Pk)

AM - A CAMB derived type that I need
- THalofit :: this
- CAMBdata :: State
- MatterPowerData :: CAMB_Pk
ReadParams(this, Ini)
- THalofit :: this
- TIniFile intent(in) :: Ini
SelfPointer(cptr, P)
- c_ptr :: cptr
- TPythonInterfacedClass pointer :: P
write_parameters(this, z, cosm, lut)
- THalofit :: this
- real(dl) intent(in) :: z
- HM_cosmology intent(in) :: cosm
- HM_tables intent(in) :: lut
zcoll_bull(this, z, cosm, lut)
- THalofit :: this
- real(dl) intent(in) :: z
- HM_cosmology :: cosm
- HM_tables :: lut

Functions

real(dl)
alpha(lut)

Two- to one-halo transition smoothing from Mead et al. (2015; arXiv 1505.07833)
- HM_tables intent(in) :: lut
real(dl)
As(lut, cosm)

Halo concentration pre-factor from Bullock et al. (2001) relation
- HM_tables intent(in) :: lut
- HM_cosmology intent(in) :: cosm
real(dl)
delta_c(z, cosm, lut)

Function for the linear collapse density
- real(dl) intent(in) :: z
- HM_cosmology intent(in) :: cosm
- HM_tables intent(in) :: lut
real(dl)
Delta_v(z, cosm, lut)

Function for the virialised overdensity
- real(dl) intent(in) :: z
- HM_cosmology intent(in) :: cosm
- HM_tables intent(in) :: lut
real(dl)
eta(cosm, lut)

Function eta that puffs halo profiles
- HM_cosmology intent(in) :: cosm
- HM_tables intent(in) :: lut
real(dl)
fdamp(lut)

Linear power damping function from Mead et al. (2015; arXiv 1505.07833)
- HM_tables intent(in) :: lut
real(dl)
kstar(lut)

Function k* that cuts off the 1-halo term at large scales
- HM_tables intent(in) :: lut
real(dl)
p_1h(k, lut, cosm)

Calculates the 1-halo term
- real(dl) intent(in) :: k
- HM_tables intent(in) :: lut
- HM_cosmology intent(in) :: cosm
real(dl)
p_2h(k, plin, lut, cosm)

Calculates the 2-halo term
- real(dl) intent(in) :: k
- real(dl) intent(in) :: plin
- HM_tables intent(in) :: lut
- HM_cosmology intent(in) :: cosm
character(len=:) allocatable
PythonClass()

Properties

integer :: halofit_version
real(dl) :: HMcode_A_baryon
real(dl) :: HMcode_eta_baryon
real(dl) :: HMcode_logT_AGN
real(dl) :: HMcode_wiggle_max_fnu

Tree Diagrams

TPythonInterfacedClass
- TCambComponent
  - TNonLinearModel
    - THalofit