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lenspen.f90
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!Lensing the C_l using the deflection angle from the computed lensing potential
!power spectrum.
!lensing_method=1: using an accurate curved-sky correlation function method
!lensing_method=2: using the flat-sky lower order result of astro-ph/9505109
! and astro-ph/9803150 as in CMBFAST
!lensing_method=3: using inaccurate full sky harmonic method of astro-ph/0001303
!The flat sky result is accurate to about 0.1% in TT, and 0.4% in EE and is
!about a factor of two faster than lensing_method=1.
!lensing_method=3 is only present for comparison and is not recommended in any regime
!Set accurate_BB=T if you want BB accurately by integrating the full angular range
!otherwise it saves a large amount of time by only integrating the small scales
!accute_BB only does *not* include any non-linear corrections or ensure you have
!chosen sufficiently high l_max and k_max, so does not neccessarily give an accurate
!result
!Uses the un-lensed Cls and the computed lensing potential power spectrum.
!Usual values of k_max are fine for all but the lensed BB Cls
!To get the lensed BB accurate around l=1000 you need to go to l_max >2000, and
!higher for higher l. Since this probes small scales in the lensing power spectrum you
!also need to go to higher k_max - for concordance models something like
!k_eta_max_scalar=10000. At l>1000 you can expect to need higher k_max, and for
!non-linear evolution to cause a significant error.
!Correlation function routines by AL+AC Nov 2004 with flat-sky borrowings from CMBFAST
!Curved sky results use the method of astro-ph/xxx.
!Full sky harmonic lensing routines by Gayoung Chon and AC.
!Ref: astro-ph/0001303 by W. Hu.
!For better derivations see also astro-ph/0301064 and astro-ph/0301031
!Adapted for CAMB and optimized by AL.
!Uses f90 version of "J1-RECURSION OF 3J-COEFFICIENTS" by K. Schulten and R.G. Gordon
!obtainable from the CPC program library (www.cpc.cs.qub.ac.uk).
!March 2006: fixed problem with l_max when generating with tensors (thanks Chad Fendt)
module lensing
use Precision
use ModelParams
use AmlUtils
implicit none
integer, parameter :: lensing_method_curv_corr=1,lensing_method_flat_corr=2, &
lensing_method_harmonic=3
integer :: lensing_method = lensing_method_curv_corr
private
logical :: lensing_includes_tensors = .false.
!flat method stores
real(dl), parameter :: dbessel = 0.05_dl
real(dl), dimension(:), allocatable :: Bess0, ddBess0
real(dl), dimension(:), allocatable :: Bess2, ddBess2
real(dl), dimension(:), allocatable :: Bess4, ddBess4
real(dl), dimension(:), allocatable :: Bess6, ddBess6
integer, parameter :: lensed_convolution_margin = 100
!Number of L less than L max at which the lensed power spectrum is calculated
!Harmonic method stores
integer :: lmax_donelnfa = 0
real(dl), dimension(:), allocatable :: lnfa
public lens_Cls, lensing_includes_tensors, lensing_method, lensing_method_flat_corr,&
lensing_method_curv_corr,lensing_method_harmonic, BessI, bessj0
contains
subroutine lens_Cls
use lvalues
!Must set l again in case computed tessors (thanks to Chad)
call initlval(lSamp,CP%Max_l)
if (lensing_method == lensing_method_curv_corr) then
call CorrFuncFullSky()
elseif (lensing_method == lensing_method_flat_corr) then
call CorrFuncFlatSky()
elseif (lensing_method == lensing_method_harmonic) then
call BadHarmonic
else
stop 'Unknown lensing method'
end if
end subroutine lens_Cls
subroutine CorrFuncFullSky
integer :: lmax_extrap
lmax_extrap = CP%Max_l - lensed_convolution_margin + 450
if (HighAccuracyDefault) lmax_extrap=lmax_extrap+300
lmax_extrap = min(lmax_extrap_highl,lmax_extrap)
call CorrFuncFullSkyImpl(max(lmax_extrap,CP%max_l))
end subroutine CorrFuncFullSky
subroutine CorrFuncFullSkyImpl(lmax)
!Accurate curved sky correlation function method
!Uses non-perturbative isotropic term with 2nd order expansion in C_{gl,2}
!Neglects C_{gl}(theta) terms (very good approx)
use ModelParams
use ModelData
use lvalues
implicit none
integer, intent(in) :: lmax
integer l, i, in
integer :: npoints
real(dl) corr(4), Cg2, sigmasq, theta
real(dl) dtheta
real(dl) llp1,fac, fac1,fac2,fac3, rootllp1, rootfac1, rootfac2, rootfac3
integer max_lensed_ix
real(dl) P(lmax),dP(lmax)
real(dl) sinth,halfsinth, x, T2,T4
real(dl) roots(-1:lmax+4), lfacs(lmax), lfacs2(lmax), lrootfacs(lmax)
real(dl) d_11(lmax),d_m11(lmax)
real(dl) d_22(lmax),d_2m2(lmax),d_20(lmax)
real(dl) Cphil3(lmin:lmax), CTT(lmin:lmax), CTE(lmin:lmax),CEE(lmin:lmax)
real(dl) ls(lmax)
real(dl) xl(lmax),ddcontribs(lmax,4),corrcontribs(lmax,4)
real(dl), allocatable, dimension(:,:,:) :: lens_contrib(:,:,:)
integer thread_ix
real(dl) pmm, pmmp1
real(dl) d4m4,d11,dm11,d2m2,d22,d20,d23,d2m3,d33,d3m3,d04,d1m2,d12,d13,d1m3,d2m4
real(dl) sinfac, Cg2sq
real(dl) X000,X022,X220,X121,X132,X242
real(dl) dX000,dX022
real(sp) timeprev
integer interp_fac
integer j,jmax
integer llo, lhi
real(dl) a0,b0,ho, sc
logical :: short_integral_range
integer, parameter :: slow_highL = 5000 !Lmax at which to do full range to prevent ringing etc
logical, parameter :: approx = .false.
!$ integer OMP_GET_THREAD_NUM, OMP_GET_MAX_THREADS
!$ external OMP_GET_THREAD_NUM, OMP_GET_MAX_THREADS
if (lensing_includes_tensors) stop 'Haven''t implemented tensor lensing'
max_lensed_ix = lSamp%l0-1
! do while(lSamp%l(max_lensed_ix) > CP%Max_l -250)
do while(lSamp%l(max_lensed_ix) > CP%Max_l - lensed_convolution_margin)
max_lensed_ix = max_lensed_ix -1
end do
lmax_lensed = lSamp%l(max_lensed_ix)
if (allocated(Cl_lensed)) deallocate(Cl_lensed)
allocate(Cl_lensed(lmin:lmax_lensed,CP%InitPower%nn,1:4))
Cl_Lensed = 0
npoints = CP%Max_l * 2
short_integral_range = .not. CP%AccurateBB .and. CP%Max_l<=slow_highL
if (.not. short_integral_range ) npoints = npoints * 2
dtheta = pi / npoints
if (short_integral_range) then
npoints = int(npoints /32 *min(32._dl,AccuracyBoost))
!OK for TT, EE, TE but inaccurate for low l BB
!this induces high frequency ringing on very small scales
end if
if (DebugMsgs) timeprev=GetTestTime()
if (.not. short_integral_range) then
!There is an odd serious problem with interpolating if you do a large
!angular range.
interp_fac =1
else
interp_fac = max(1,nint(10/AccuracyBoost))
end if
jmax = 0
do l=lmin,lmax
if (l<=15 .or. mod(l-15,interp_fac)==interp_fac/2) then
jmax =jmax+1
ls(jmax)=l
xl(jmax)=l
end if
lfacs(l) = real(l*(l+1),dl)
lfacs2(l) = real((l+2)*(l-1),dl)
lrootfacs(l) = sqrt(lfacs(l)*lfacs2(l))
end do
roots(-1)=0 !just so dipole doesn't screw up
do l=0,lmax+4
roots(l) = sqrt(real(l,dl))
end do
thread_ix = 1
!$ thread_ix = OMP_GET_MAX_THREADS()
allocate(lens_contrib(4,lmax_lensed,thread_ix))
do in = 1, CP%InitPower%nn
Cphil3=0
! print*, 'Hi Renee initialising Cphil3 now'
do l=lmin,CP%Max_l
! (2*l+1)l(l+1)/4pi C_phi_phi: Cl_scalar(l,1,C_Phi) is l^4 C_phi_phi
Cphil3(l) = Cl_scalar(l,in,C_Phi)*(2*l+1)*(l+1)/real(l,dl)**3/(4*pi)
fac = (2*l+1)/(4*pi) * 2*pi/(l*(l+1))
CTT(l) = Cl_scalar(l,in,C_Temp)*fac
CEE(l) = Cl_scalar(l,in,C_E)*fac
CTE(l) = Cl_scalar(l,in,C_Cross)*fac
! write(888,*) l, Cphil3(l)
end do
if (Cphil3(10) > 1e-7) then
write(*,*) 'strange lensing here, we are resetting it'
write(*,*) CP%h0
do l=lmin, CP%Max_l
! write(999,*) l, Cphil3(l)
Cphil3(l) =0
enddo
! write (*,*) 'You need to normalize realistically to use lensing.'
! write (*,*) 'see http://cosmocoffee.info/viewtopic.php?t=94'
! stop
end if
if (lmax > CP%Max_l) then
l=CP%Max_l
sc = (2*l+1)/(4*pi) * 2*pi/(l*(l+1))
fac2=CTT(CP%Max_l)/(sc*highL_CL_template(CP%Max_l, C_Temp))
fac=Cphil3(CP%Max_l)/(sc*highL_CL_template(CP%Max_l, C_Phi))
do l=CP%Max_l+1, lmax
!Fill in tail from template
sc = (2*l+1)/(4*pi) * 2*pi/(l*(l+1))
Cphil3(l) = highL_CL_template(l, C_Phi)*fac*sc
CTT(l) = highL_CL_template(l, C_Temp)*fac2*sc
CEE(l) = highL_CL_template(l, C_E)*fac2 *sc
CTE(l) = highL_CL_template(l, C_Cross)*fac2*sc
if (Cphil3(CP%Max_l+1) > 1e-7) then
write (*,*) 'You need to normalize the high-L template so it is dimensionless'
stop
end if
end do
end if
lens_contrib=0
!uncomment second line for PGF90 workaround
!$OMP PARALLEL DO DEFAULT(PRIVATE), &
!OMP PRIVATE(P,dP,d11,dm11,d22,d2m2,d20,corrcontribs,ddcontribs),&
!$OMP SHARED(lfacs,lfacs2,lrootfacs,Cphil3,CTT,CTE,CEE,lens_contrib, lmax), &
!$OMP SHARED(dtheta,CP,lmax_lensed,roots, npoints,interp_fac,jmax,ls,xl,short_integral_range)
do i=1,npoints-1
theta = i * dtheta
x = cos(theta)
sinth = sin(theta)
halfsinth = sinth/2
pmm=1
pmmp1=x
Cg2=0
sigmasq=0
if (lmin==1) then
d_11(1) = cos(theta/2)**2
d_m11(1) = sin(theta/2)**2
sigmasq = sigmasq + (1-d_11(1))*Cphil3(lmin)
Cg2 = Cg2 + d_m11(1)*Cphil3(lmin)
P(1) = x
d_22(1)=0
d_2m2(1)=0
d_20(1)=0
end if
do l=2,lmax
P(l)= ((2*l-1)* x *pmmp1 - (l-1)*Pmm)/ l
dP(l) = l*(pmmp1-x*P(l))/sinth**2
Pmm=pmmp1
pmmp1=P(l)
llp1 = lfacs(l)
fac1 = (1-x)
fac2 = (1+x)
fac = fac1/fac2
d_11(l) = fac1*dP(l)/llp1 + P(l)
d_m11(l) = fac2*dP(l)/llp1 - P(l)
sigmasq = sigmasq + (1-d_11(l))*Cphil3(l)
Cg2 = Cg2 + d_m11(l)*Cphil3(l)
d_22(l) = ( ((4*x-8)/fac2 + llp1)*P(l) &
+ 4*fac*( fac2 + (x - 2)/llp1)*dP(l) )/ lfacs2(l)
d_2m2(l) = ( (llp1- (4*x+8)/fac1) *P(l) &
+4/fac*( -fac1 + (x+2)/llp1) *dP(l) )/lfacs2(l)
d_20(l) = (2*x*dP(l) - llp1*P(l) ) / lrootfacs(l)
end do
do j=1,jmax
l =ls(j)
fac1 = (1-x)
fac2 = (1+x)
llp1 = lfacs(l)
rootllp1 = roots(l)*roots(l+1)
rootfac1 = roots(l+2)*roots(l-1)
rootfac2 = roots(l+3)*roots(l-2)
llp1=lfacs(l)
dm11=d_m11(l)
d11=d_11(l)
if (l<2) then
d2m2=0
d22=0
d20=0
d1m2 = 0
d12 = 0
else
d2m2=d_2m2(l)
d22=d_22(l)
d20=d_20(l)
d1m2 = sinth/rootfac1*(dP(l) -2/fac1*dm11)
d12 = sinth/rootfac1*(dP(l) -2/fac2*d11)
end if
if (l<3) then
d1m3=0
d2m3=0
d3m3=0
d13 =0
d23 =0
d33 =0
else
sinfac=4/sinth
d1m3 = (-(x+0.5_dl)*d1m2*sinfac - lfacs2(l)*dm11/rootfac1 )/rootfac2
d2m3 = (-fac2*d2m2*sinfac - rootfac1*d1m2)/rootfac2
d3m3 = (-(x+1.5_dl)*d2m3*sinfac - rootfac1*d1m3)/rootfac2
d13 = ((x-0.5_dl)*d12*sinfac - lfacs2(l)*d11/rootfac1 ) /rootfac2
d23 = (-fac1*d22*sinfac + rootfac1*d12 ) / rootfac2
d33 = (-(x-1.5_dl)*d23*sinfac - rootfac1*d13)/rootfac2
end if
if (l<4) then
d04=0
d2m4=0
d4m4=0
rootfac3=0
else
rootfac3=roots(l-3)*roots(l+4)
d04=( (-llp1 + (18*x**2 + 6)/sinth**2 )*d20 -&
6*x*lfacs2(l)*dP(l)/lrootfacs(l) ) / (rootfac2*rootfac3)
d2m4= (-(6*x+4)*d2m3/sinth - rootfac2*d2m2 ) / rootfac3
d4m4 = (-7/5._dl*(llp1-6)*d2m2 + &
12/5._dl*( -llp1+(9*x+26)/fac1)*d3m3 ) / (llp1-12)
end if
!Non perturbative isotropic integrals
!these are approx, but extremely good approximations
X000 = exp(-llp1*sigmasq/4)
if (approx) then
X022 = X000
X220 = rootllp1**2/4*X000
X121 = -0.5_dl*rootllp1*X000
X132 = -0.5_dl*rootllp1*X000
X242 = 0.25_dl*rootllp1**2*X022
dX000 = -llp1/4*X000
dX022 = -llp1/4*X022
else
X022 = X000*(1+sigmasq) !exp(-(llp1-4)*sigmasq/4)
X220 = lrootfacs(l)/4*X000
X121 = -0.5_dl*rootfac1*X000
X132 = -0.5_dl*rootfac2*X000
X242 = 0.25_dl*rootfac2*rootfac3*X022
dX000 = -llp1/4*X000
dX022 = (1-llp1/4)*X022
end if
!second order
!TT
fac1 = dX000**2
fac3 = X220**2
Cg2sq = Cg2**2
!Here we drop terms in Cgt which are down by powers of l
!Approx good to 1e-4 level
fac = ( (X000**2-1) + Cg2sq*fac1)*P(l)+ Cg2sq*fac3*d2m2 &
+ 8/llp1* fac1*Cg2*dm11
corrcontribs(j,1)= CTT(l) * fac
fac2=(Cg2*dX022)**2+(X022**2-1)
!Q+U
fac = 2*Cg2*X121*X132*d13 + fac2*d22 +Cg2sq*X242*X220*d04
corrcontribs(j,2)= CEE(l) * fac
!Q-U
fac = ( fac3*P(l) + X242**2*d4m4)*Cg2sq/2 &
+ Cg2*(X121**2*dm11+ X132**2*d3m3) + fac2*d2m2
corrcontribs(j,3)= CEE(l) * fac
!TE
fac = (X000*X022-1)*d20+ &
2*dX000*Cg2*(X121*d11 + X132*d1m3)/rootllp1 &
+ Cg2sq*(X220/2*d2m4*X242 +( fac3/2 + dX022*dX000)*d20)
corrcontribs(j,4)= CTE(l) * fac
end do
do j=1,4
corr(j) = sum(corrcontribs(1:14,j))+interp_fac*sum(corrcontribs(15:jmax,j))
end do
if (short_integral_range .and. i>npoints-20) &
corr=corr*exp(-(i-npoints+20)**2/150.0) !taper the end to help prevent ringing
!Interpolate contributions
!Increasing interp_fac and using this seems to be slower than above
if (.false.) then
if (abs(sum(corrcontribs(1:jmax,1)))>1e-11) print *,i,sum(corrcontribs(1:jmax,1))
do j=1,4
call spline(xl,corrcontribs(1,j),jmax,1d30,1d30,ddcontribs(1,j))
end do
corr=0
llo=1
do l=lmin,lmax
if ((l > ls(llo+1)).and.(llo < jmax)) then
llo=llo+1
end if
lhi=llo+1
ho=ls(lhi)-ls(llo)
a0=(ls(lhi)-l)/ho
b0=(l-ls(llo))/ho
fac1 = ho**2/6
fac2 = (b0**3-b0)*fac1
fac1 = (a0**3-a0)*fac1
corr(1) = Corr(1)+ a0*corrcontribs(llo,1)+ b0*corrcontribs(lhi,1)+ &
fac1* ddcontribs(llo,1) +fac2*ddcontribs(lhi,1)
corr(2) = Corr(2)+ a0*corrcontribs(llo,2)+ b0*corrcontribs(lhi,2)+ &
fac1* ddcontribs(llo,2) +fac2*ddcontribs(lhi,2)
corr(3) = Corr(3)+ a0*corrcontribs(llo,3)+ b0*corrcontribs(lhi,3)+ &
fac1* ddcontribs(llo,3) +fac2*ddcontribs(lhi,3)
corr(4) = Corr(4)+ a0*corrcontribs(llo,4)+ b0*corrcontribs(lhi,4)+ &
fac1* ddcontribs(llo,4) +fac2*ddcontribs(lhi,4)
end do
end if
!$ thread_ix = OMP_GET_THREAD_NUM()+1
do l=lmin, lmax_lensed
!theta factors were put in earlier (already in corr)
lens_contrib(C_Temp, l, thread_ix)= lens_contrib(C_Temp,l, thread_ix) + &
corr(1)*P(l)*sinth
T2 = corr(2)* d_22(l)
T4 = corr(3)* d_2m2(l)
lens_contrib(CT_E, l, thread_ix)= lens_contrib(CT_E,l, thread_ix) + &
(T2+T4)*halfsinth
lens_contrib(CT_B, l, thread_ix)= lens_contrib(CT_B,l, thread_ix) + &
(T2-T4)*halfsinth
lens_contrib(CT_Cross, l, thread_ix)= lens_contrib(CT_Cross,l, thread_ix) + &
corr(4)*d_20(l)*sinth
end do
end do
!$OMP END PARALLEL DO
do l=lmin, lmax_lensed
!sign from d(cos theta) = -sin theta dtheta
fac = l*(l+1)/OutputDenominator*dtheta *2*pi
Cl_lensed(l,in,CT_Temp) = sum(lens_contrib(CT_Temp,l,:))*fac &
+ Cl_scalar(l,in,C_Temp)
Cl_lensed(l,in,CT_E) = sum(lens_contrib(CT_E,l,:))*fac &
+ Cl_scalar(l,in,C_E)
Cl_lensed(l,in,CT_B) = sum(lens_contrib(CT_B,l,:))*fac
Cl_lensed(l,in,CT_Cross) = sum(lens_contrib(CT_Cross,l,:))*fac &
+ Cl_scalar(l,in,C_Cross)
end do
end do !loop over different initial power spectra
deallocate(lens_contrib)
if (DebugMsgs) write(*,*) GetTestTime()-timeprev, 'Time for corr lensing'
end subroutine CorrFuncFullSkyImpl
subroutine CorrFuncFlatSky
!Do flat sky approx partially non-perturbative lensing, lensing_method=2
use ModelParams
use ModelData
use lvalues
integer l, i
integer :: npoints
real(dl) Cgl2, sigmasq, theta
real(dl) dtheta
real(dl) dbessfac, fac, fac1,fac2, C2term, expsig, corr(4)
real(sp) timeprev
real(dl) Bessel0(lmin:CP%Max_l),Bessel2(lmin:CP%Max_l)
real(dl) Bessel4(lmin:CP%Max_l),Bessel6(lmin:CP%Max_l)
real(dl) Cphil3(lmin:CP%Max_l), CTT(lmin:CP%Max_l), CTE(lmin:CP%Max_l),CEE(lmin:CP%Max_l)
integer max_lensed_ix
integer b_lo
integer in
real(dl) T2,T4,a0, b0
real(dl) lfacs(CP%Max_l)
real(dl), allocatable, dimension(:,:,:) :: lens_contrib(:,:,:)
integer thread_ix
!$ integer OMP_GET_THREAD_NUM, OMP_GET_MAX_THREADS
!$ external OMP_GET_THREAD_NUM, OMP_GET_MAX_THREADS
if (lensing_includes_tensors) stop 'Haven''t implemented tensor lensing'
max_lensed_ix = lSamp%l0-1
do while(lSamp%l(max_lensed_ix) > CP%Max_l -250)
max_lensed_ix = max_lensed_ix -1
end do
lmax_lensed = lSamp%l(max_lensed_ix)
if (allocated(Cl_lensed)) deallocate(Cl_lensed)
allocate(Cl_lensed(lmin:lmax_lensed,CP%InitPower%nn,1:4))
Cl_Lensed = 0
npoints = CP%Max_l * 2
if (CP%AccurateBB) npoints = npoints * 2
dtheta = pi / npoints
if (.not. CP%AccurateBB) then
npoints = int(npoints /32 *min(32._dl,AccuracyBoost))
!OK for TT, EE, TE but inaccurate for low l BB
!this induces high frequency ringing on very small scales
end if
call GetBessels(npoints*dtheta*CP%Max_l)
if (DebugMsgs) timeprev=GetTestTime()
dbessfac = dbessel**2/6
thread_ix = 1
!$ thread_ix = OMP_GET_MAX_THREADS()
allocate(lens_contrib(4,lmax_lensed,thread_ix))
do in = 1, CP%InitPower%nn
do l=lmin,CP%Max_l
! l^3 C_phi_phi/2/pi: Cl_scalar(l,1,C_Phi) is l^4 C_phi_phi
Cphil3(l) = Cl_scalar(l,in,C_Phi)/l /(2*pi)
fac = l/(2*pi)*2*pi/(l*(l+1))
CTT(l) = Cl_scalar(l,in,C_Temp)*fac
CEE(l) = Cl_scalar(l,in,C_E)*fac
CTE(l) = Cl_scalar(l,in,C_Cross)*fac
lfacs(l) = l**2*0.5_dl
end do
if (Cphil3(10) > 1e-7) then
write (*,*) 'You need to normalize realistically to use lensing.'
write (*,*) 'see http://cosmocoffee.info/viewtopic.php?t=94'
stop
end if
lens_contrib=0
!$OMP PARALLEL DO DEFAULT(SHARED), &
!$OMP PRIVATE(theta, sigmasq,cgl2,b_lo,a0,b0,fac,fac1,fac2), &
!$OMP PRIVATE(Bessel0,Bessel2,Bessel4,Bessel6), &
!$OMP PRIVATE(corr,expsig,C2term,T2,T4,i,l, thread_ix)
do i=1,npoints-1
theta = i * dtheta
sigmasq =0
Cgl2=0
fac = theta /dbessel
do l=lmin,CP%Max_l
!Interpolate the Bessel functions, and compute sigma^2 and C_{gl,2}
b0 = l*fac
b_lo = int(b0) +1
a0= b_lo - b0
b0= 1._dl - a0
fac1 = a0*b0*dbessfac
fac2 = fac1*(a0-2)
fac1 = fac1*(b0-2)
Bessel0(l) = a0*Bess0(b_lo)+ b0*Bess0(b_lo+1) +fac1*ddBess0(b_lo) &
+fac2*ddBess0(b_lo+1)
sigmasq = sigmasq + (1-Bessel0(l))*Cphil3(l)
Bessel2(l) = a0*Bess2(b_lo)+ b0*Bess2(b_lo+1) +fac1*ddBess2(b_lo) &
+fac2*ddBess2(b_lo+1)
Cgl2 = Cgl2 + Bessel2(l)*Cphil3(l)
Bessel4(l) = a0*Bess4(b_lo)+ b0*Bess4(b_lo+1) +fac1*ddBess4(b_lo) &
+fac2*ddBess4(b_lo+1)
Bessel6(l) = a0*Bess6(b_lo)+ b0*Bess6(b_lo+1) +fac1*ddBess6(b_lo) &
+fac2*ddBess6(b_lo+1)
end do
!Get difference between lensed and unlensed correlation function
corr = 0
do l=lmin,CP%Max_l
!For 2nd order perturbative result use
! expsig = 1 -sigmasq*l**2/2._dl
! C2term = l**2*Cgl2/2._dl
fac = sigmasq*lfacs(l)
expsig = exp(-fac)
C2term = Cgl2*lfacs(l)
!Put theta factor later in here
fac1 = expsig*theta
fac2 = C2term*fac1
fac1 = fac1 - theta !we want expsig-1 to get lensing difference
fac = fac1*Bessel0(l) + fac2*Bessel2(l)
!TT
corr(1) = corr(1) + CTT(l) * fac
!Q + U
corr(2) = corr(2) + CEE(l) * fac
fac2 = fac2*0.5_dl
!Q-U
corr(3) = corr(3) + CEE(l) * &
(fac1*Bessel4(l) + fac2*(Bessel2(l)+Bessel6(l)))
!Cross
corr(4) = corr(4) + CTE(l) * &
(fac1*Bessel2(l) + fac2*(Bessel0(l)+Bessel4(l)))
end do
!$ thread_ix = OMP_GET_THREAD_NUM()+1
do l=lmin, lmax_lensed
!theta factors were put in earlier (already in corr)
lens_contrib(C_Temp, l, thread_ix)= lens_contrib(C_Temp,l, thread_ix) + &
corr(1)*Bessel0(l)
T2 = corr(2)*Bessel0(l)
T4 = corr(3)*Bessel4(l)
lens_contrib(CT_E,l,thread_ix) = lens_contrib(CT_E,l, thread_ix) + T2+T4
lens_contrib(CT_B,l,thread_ix) = lens_contrib(CT_B,l, thread_ix) + T2-T4
lens_contrib(CT_Cross,l, thread_ix) = lens_contrib(CT_Cross,l, thread_ix) + &
corr(4)*Bessel2(l)
end do
end do
!$OMP END PARALLEL DO
do l=lmin, lmax_lensed
fac = l*(l+1)* 2*pi/OutputDenominator*dtheta
Cl_lensed(l,in,CT_Temp) = sum(lens_contrib(CT_Temp,l,:))*fac &
+ Cl_scalar(l,in,CT_Temp)
Cl_lensed(l,in,CT_Cross) = sum(lens_contrib(CT_Cross,l,:))*fac &
+Cl_scalar(l,in,C_Cross)
fac = fac /2 !(factor of 1/2 should have been in T2+/-T4 above
Cl_lensed(l,in,CT_E) = sum(lens_contrib(CT_E,l,:))*fac &
+ Cl_scalar(l,in,CT_E)
Cl_lensed(l,in,CT_B) = sum(lens_contrib(CT_B,l,:))*fac
end do
end do !loop over different initial power spectra
deallocate(lens_contrib)
if (DebugMsgs) write(*,*) GetTestTime()-timeprev, 'Time for corr lensing'
end subroutine CorrFuncFlatSky
subroutine BadHarmonic
use ModelParams
use ModelData
use lvalues
use InitialPower
integer maxl, i, in, almin, max_lensed_ix, maxl_phi
real(dl) , dimension (:,:,:), allocatable :: bare_cls
real(dl) pp(CP%InitPower%nn,CP%Max_l)
real(dl) asum(CP%InitPower%nn), RR(CP%InitPower%nn), roots(CP%Max_l)
real(dl) asum_TE(CP%InitPower%nn), asum_EE(CP%InitPower%nn), asum_BB(CP%InitPower%nn)
integer l1,l2,al,j, j1, k, hk, llp_1, llp_al, g1
real(dl) F, fct
real(dl) g2l,g2l1, norm
real(dl) a3j(CP%Max_l*2+1), tF, expF
logical DoPol
real(dl) iContribs(lSamp%l0,CP%InitPower%nn, 1:4), intcontrib(lmin:lSamp%l(lSamp%l0))
real(dl) , dimension (:,:,:), allocatable :: iCl_lensed
integer max_j_contribs
real(sp) timeprev
!Otherwise use second order perturbative harmonic method
if (DebugMsgs) timeprev=GetTestTime()
DoPol = CP%AccuratePolarization
maxl = CP%Max_l
if (allocated(Cl_lensed)) deallocate(Cl_lensed)
allocate(bare_cls(CP%InitPower%nn,maxl,1:4))
RR = 0
do j=lmin,maxl
norm = OutputDenominator/(j*(j+1))
if (lensing_includes_tensors .and. CP%WantTensors .and. j<= CP%Max_l_tensor) then !Use total Cls
bare_cls(:,j,CT_Temp:CT_E) = (Cl_scalar(j,:,C_Temp:C_E) + &
Cl_tensor(j,:,CT_Temp:CT_E))*norm
bare_cls(:,j,CT_B) = Cl_tensor(j,:,CT_B)*norm
bare_cls(:,j,CT_Cross) = (Cl_scalar(j,:,C_Cross) + &
Cl_tensor(j,:,CT_Cross))*norm
else
bare_cls(:,j,CT_Temp:CT_E) = Cl_scalar(j,:,C_Temp:C_E)*norm
bare_cls(:,j,CT_B) = 0
bare_cls(:,j,CT_Cross) = Cl_scalar(j,:,C_Cross)*norm
end if
pp(:,j) = Cl_scalar(j,:,C_Phi)/real(j**2,dl)**2
RR = RR + j*(j+1)*real(2*j+1,dl)*pp(:,j)
roots(j) = sqrt(real(2*j+1,dl))
end do
RR = RR/2/fourpi
if (RR(1) > 1e-5) then
write (*,*) 'You need to normalize realistically to use lensing.'
write (*,*) 'see http://cosmocoffee.info/viewtopic.php?t=94'
stop
end if
if (maxl > lmax_donelnfa) then
!Get ln factorials
if (allocated(lnfa)) deallocate(lnfa)
allocate(lnfa(0:maxl*3+1))
lmax_donelnfa = maxl
lnfa(0) = 0
do i=1,CP%Max_l*3+1
lnfa(i)=lnfa(i-1) + log(real(i,dl))
end do
end if
max_lensed_ix = lSamp%l0-1
do while(lSamp%l(max_lensed_ix) > maxl -250)
max_lensed_ix = max_lensed_ix -1
end do
lmax_lensed = lSamp%l(max_lensed_ix)
allocate(iCl_lensed(max_lensed_ix, CP%InitPower%nn, 1:4))
max_j_contribs = lSamp%l0-1
if (.not. DoPol) then
maxl_phi = min(maxl,nint(max(600,(maxl*2)/5)*scale*AccuracyBoost))
do while (lSamp%l(max_j_contribs) > maxl_phi)
max_j_contribs=max_j_contribs-1
end do
end if
!$OMP PARALLEL DO DEFAULT(SHARED), SCHEDULE(DYNAMIC), SHARED(max_j_contribs) &
!$OMP PRIVATE(al,g1,llp_al,llp_1,g2l,asum,l1,g2l1,l2,k,hk,F,fct,almin), &
!$OMP PRIVATE(asum_EE,asum_BB,asum_TE,expF,tF, a3j, iContribs,in,intcontrib)
do j=max_lensed_ix,1,-1
!Only compute lensed spectra at lSamp%l(j). Start with slow ones.
al=lSamp%l(j)
llp_al = al*(al+1)
g2l=sqrt((2*al+1)/fourpi)
asum = 0
asum_EE = 0
asum_BB = 0
asum_TE = 0
do j1 = 1, max_j_contribs
! Contributions to C_al are a smooth function of l_1 - so interpolate
l1=lSamp%l(j1)
llp_1 = l1*(l1+1)
g2l1=roots(l1)
almin = max(abs(al-l1),2)
if (DoPol) then
call GetThreeJs(a3j(almin),l1,al,0,2)
do l2= almin, min(maxl,al+l1)
g1 = llp_1+l2*(l2+1)-llp_al
if (g1 == 0 ) cycle
k=al+l1+l2
fct=g1*g2l*g2l1*roots(l2)/2
tF = fct*a3j(l2)
if (mod(k,2)==0) then
hk = k/2
F = lnfa(hk)-lnfa(hk-al)-lnfa(hk-l1)-lnfa(hk-l2)+(lnfa(k-2*al)+lnfa(k-2*l1)&
& +lnfa(k-2*l2)-lnfa(k+1))/2
expF = exp(F)
asum=asum + bare_cls(:,l2,C_Temp)*(expF*fct)**2
asum_EE = asum_EE + bare_cls(:,l2,CT_E)*tF**2
asum_BB = asum_BB + bare_cls(:,l2,CT_B)*tF**2
if (mod(hk,2)/=0) tF=-tF
asum_TE = asum_TE + bare_cls(:,l2,CT_Cross)*expF*fct*tF
else
asum_BB = asum_BB + bare_cls(:,l2,CT_E)*tF**2
asum_EE = asum_EE +bare_cls(:,l2,CT_B)*tF**2
end if
end do
else !No polarization
do l2= almin +mod(al+l1+almin,2),min(maxl,al+l1), 2
!Only do lSamp%l's where al + l1 + l2 is even
g1 = llp_1+l2*(l2+1)-llp_al
if (g1 == 0 ) cycle !Contribution is zero
k=al+l1+l2
hk=k/2
fct=g1*g2l*g2l1*roots(l2)/2
expF = exp(2*(lnfa(hk)-lnfa(hk-al)-lnfa(hk-l1)-lnfa(hk-l2))+lnfa(k-2*al)+lnfa(k-2*l1)&
& +lnfa(k-2*l2)-lnfa(k+1))
asum=asum + bare_cls(:,l2,CT_Temp)*expF *fct**2
end do
end if !No polarization
iContribs(j1,:,CT_Temp) = asum*pp(:,l1)
if (DoPol) then
iContribs(j1,:,CT_E) = asum_EE*pp(:,l1)
iContribs(j1,:,CT_B) = asum_BB*pp(:,l1)
iContribs(j1,:,CT_Cross) = asum_TE*pp(:,l1)
end if
asum = 0
asum_EE = 0
asum_BB = 0
asum_TE = 0
end do
!Interpolate contributions to sum and add up
do in=1, CP%InitPower%nn
call InterpolateClArr(lSamp,iContribs(1,in,CT_Temp),intcontrib,max_j_contribs)
asum(in) = sum(intcontrib(lmin:lSamp%l(max_j_contribs)))
if (DoPol) then
call InterpolateClArr(lSamp,iContribs(1,in,CT_E),intcontrib,max_j_contribs)
asum_EE(in) = sum(intcontrib(lmin:lSamp%l(max_j_contribs)))
call InterpolateClArr(lSamp,iContribs(1,in,CT_B),intcontrib,max_j_contribs)
asum_BB(in) = sum(intcontrib(lmin:lSamp%l(max_j_contribs)))
call InterpolateClArr(lSamp,iContribs(1,in,CT_Cross),intcontrib,max_j_contribs)
asum_TE(in) = sum(intcontrib(lmin:lSamp%l(max_j_contribs)))
end if
end do
iCl_lensed(j,:,CT_Temp) = ((1-al*(al+1)*RR)*bare_cls(:,al,CT_Temp) & !Linear part
+ asum/(2*al+1))*llp_al/OutputDenominator !add quadratic part and *l(l+1)/2pi
if (DoPol) then
iCl_lensed(j,:,CT_E) = ((1-(al**2+al-4)*RR)*bare_cls(:,al,CT_E) &
+ asum_EE/(2*al+1))*llp_al/OutputDenominator
iCl_lensed(j,:,CT_B) = ((1-(al**2+al-4)*RR)*bare_cls(:,al,CT_B) &
+ asum_BB/(2*al+1))*llp_al/OutputDenominator
iCl_lensed(j,:,CT_Cross) = ((1-(al**2+al-2)*RR)*bare_cls(:,al,CT_Cross) &
+ asum_TE/(2*al+1))*llp_al/OutputDenominator
else
iCl_lensed(j,:,CT_E:CT_Cross) = bare_cls(:,al,CT_E:CT_Cross)
end if
end do
!$OMP END PARALLEL DO
deallocate(bare_cls)
allocate(Cl_lensed(lmin:lmax_lensed,CP%InitPower%nn,1:4))
!Interpolate to get final spectrum
do in=1, CP%InitPower%nn
do j = CT_Temp, CT_Cross
call InterpolateClArr(lSamp,iCl_lensed(1,in,j),Cl_lensed(lmin, in, j),max_lensed_ix)
end do
end do
deallocate(iCl_lensed)
if (DebugMsgs) then
if (FeedbackLevel>0) write(*,*) GetTestTime()-timeprev,' Timing for lensing'
end if
end subroutine BadHarmonic
subroutine GetBessels(MaxArg)
real(dl), intent(in):: MaxArg
integer i
real(dl), allocatable, dimension(:) :: x
integer max_bes_ix
integer, save :: last_max = 0
max_bes_ix = nint(MaxArg / dbessel) + 3
if (max_bes_ix > last_max) then
last_max = max_bes_ix
if (allocated(Bess0)) then
deallocate(Bess0,ddBess0)
deallocate(Bess2,ddBess2)
deallocate(Bess4,ddBess4)
deallocate(Bess6,ddBess6)
end if
allocate(Bess0(max_bes_ix),ddBess0(max_bes_ix))
allocate(Bess2(max_bes_ix),ddBess2(max_bes_ix))
allocate(Bess4(max_bes_ix),ddBess4(max_bes_ix))
allocate(Bess6(max_bes_ix),ddBess6(max_bes_ix))
allocate(x(max_bes_ix))
Bess0(1)=1
Bess2(1)=0; Bess4(1)=0; Bess6(1)=0
x(1)=0
do i=2, max_bes_ix
x(i) = (i-1)*dbessel
Bess0(i) = Bessj0(x(i))
Bess2(i) = Bessj(2,x(i))
Bess4(i) = Bessj(4,x(i))
Bess6(i) = Bessj(6,x(i))
end do
call spline(x,Bess0,max_bes_ix,spl_large,spl_large,ddBess0)
call spline(x,Bess2,max_bes_ix,spl_large,spl_large,ddBess2)
call spline(x,Bess4,max_bes_ix,spl_large,spl_large,ddBess4)
call spline(x,Bess6,max_bes_ix,spl_large,spl_large,ddBess6)
deallocate(x)
end if
end subroutine GetBessels
FUNCTION bessj0(x)
real(dl) bessj0,x
real(dl) ax,xx,z
real(dl) p1,p2,p3,p4,p5,q1,q2,q3,q4,q5,r1,r2,r3,r4,r5,r6, &
s1,s2,s3,s4,s5,s6,y
SAVE p1,p2,p3,p4,p5,q1,q2,q3,q4,q5,r1,r2,r3,r4,r5,r6,s1,s2,s3,s4, &
s5,s6
DATA p1,p2,p3,p4,p5/1.d0,-.1098628627d-2,.2734510407d-4, &
-.2073370639d-5,.2093887211d-6/, q1,q2,q3,q4,q5/-.1562499995d-1, &
.1430488765d-3,-.6911147651d-5,.7621095161d-6,-.934945152d-7/
DATA r1,r2,r3,r4,r5,r6/57568490574.d0,-13362590354.d0, &
651619640.7d0,-11214424.18d0,77392.33017d0,-184.9052456d0/,s1,s2, &
s3,s4,s5,s6/57568490411.d0,1029532985.d0,9494680.718d0, &
59272.64853d0,267.8532712d0,1.d0/
if(abs(x).lt.8.d0)then
y=x**2
bessj0=(r1+y*(r2+y*(r3+y*(r4+y*(r5+y*r6)))))/(s1+y*(s2+y*(s3+y* &
(s4+y*(s5+y*s6)))))
else
ax=abs(x)
z=8.d0/ax
y=z**2
xx=ax-.785398164d0
bessj0=sqrt(.636619772d0/ax)*(cos(xx)*(p1+y*(p2+y*(p3+y*(p4+y* &
p5))))-z*sin(xx)*(q1+y*(q2+y*(q3+y*(q4+y*q5)))))
endif
! (C) Copr. 1986-92 Numerical Recipes Software
END FUNCTION bessj0
FUNCTION BESSJ1(X)
real(dl), intent(in) :: x