def A(x, pars, lmax=2000):
# Gets the spectrum for a set of parameters
if len(pars) == 5:
H0, ombh2, omch2, As, ns = pars
tau = 0.05
elif len(pars) == 1:
H0, ombh2, omch2, As, ns = [
68.4756197, .0224459632, .116026743, 2.05024029e-09, .969172419
]
tau = pars[0]
else:
H0, ombh2, omch2, As, ns, tau = pars
pars = camb.CAMBparams()
pars.set_cosmology(H0=H0,
ombh2=ombh2,
omch2=omch2,
mnu=0.06,
omk=0,
tau=tau)
pars.InitPower.set_params(As=As, ns=ns, r=0)
pars.set_for_lmax(lmax, lens_potential_accuracy=0)
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(pars, CMB_unit='muK')
cmb = powers['total']
tt = cmb[:,
0] #you could return the full power spectrum here if you wanted to do say EE
return tt[x.astype(int)]
def __initialize_nonlin_CAMB(self):
print 'Initializing nonlinear CAMB.'
parsnl = camb.CAMBparams()
parsnl.set_cosmology(H0=self.H0,
ombh2=self.Ob * self.h**2.,
omch2=self.Oc * self.h**2.,
omk=0.,
mnu=self.Mnu,
standard_neutrino_neff=self.Neff,
nnu=self.Neff,
TCMB=self.TCMB)
parsnl.InitPower.set_params(ns=self.ns,
As=self.As,
pivot_scalar=self.pivot_scalar)
# parsnl.NonLinear = model.NonLinear_both
parsnl.set_matter_power(redshifts=[0.], kmax=101.)
self.my_PK_psi = get_matter_power_interpolator(
parsnl,
zmin=0.,
zmax=1100.,
nz_step=150,
kmax=101.,
nonlinear=True,
hubble_units=True,
k_hunit=True,
var1=model.Transfer_Weyl,
var2=model.Transfer_Weyl).P
def get_spectrum(p, lmax_acc=2000, lmax_ret=1200):
"""Get power spectrum with CAMB
Args:
p: parameters H0, ombh2, omch2, tau, As, ns
lmax_acc: maximum l index for the accuracy of calculations
lmax_ret: maximum l index for the returned power spectrum
Returns:
tt: TT power spectrum for multipole indices 2 (quadrupole) to lmax_ret
"""
H0 = p[0]
ombh2 = p[1]
omch2 = p[2]
tau = p[3]
As = p[4]
ns = p[5]
pars = camb.CAMBparams()
pars.set_cosmology(H0=H0, ombh2=ombh2, omch2=omch2, omk=0.0, mnu=0.06,
tau=tau)
pars.InitPower.set_params(As=As, ns=ns, r=0)
pars.set_for_lmax(lmax_acc, lens_potential_accuracy=0)
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(pars, CMB_unit='muK', lmax=lmax_ret)
cmb = powers['total']
tt = cmb[:, 0][2:] # don't need first to indices
return tt
def test_cosmo_io_read_write_c_ell(self):
pars = camb.CAMBparams(**self.cosmo_opts)
cosmo_new = Cosmology(pars)
with tempfile.TemporaryDirectory(dir=self.path) as tmpdirname:
filename = os.path.join(tmpdirname, 'c_ell')
self.cosmo.write_c_ell(filename)
cosmo_new.read_c_ell(filename)
np.testing.assert_almost_equal(
cosmo_new.c_ell['lensed_scalar']['c_ell'],
self.cosmo.c_ell['lensed_scalar']['c_ell'])
np.testing.assert_equal(cosmo_new.c_ell['lensed_scalar']['ells'],
self.cosmo.c_ell['lensed_scalar']['ells'])
np.testing.assert_almost_equal(
cosmo_new.c_ell['unlensed_scalar']['c_ell'],
self.cosmo.c_ell['unlensed_scalar']['c_ell'])
np.testing.assert_equal(
cosmo_new.c_ell['unlensed_scalar']['ells'],
self.cosmo.c_ell['unlensed_scalar']['ells'])
def matterps2corr2esd(redshift,cosmology):
z = redshift
H_null,Ombh2,Omch2=cosmology
pars = camb.CAMBparams()
pars.set_cosmology(H0=H_null,ombh2=Ombh2,omch2=Omch2)
pars.set_dark_energy()
pars.InitPower.set_params(ns=nps)
pars.set_matter_power(redshifts=[0.0,z],kmax=2.0)
#Linear spectra--------
pars.NonLinear=model.NonLinear_none
results =camb.get_results(pars)
kh,znon,pk =results.get_matter_power_spectrum(minkh=1e-4,maxkh=1000.0,npoints=1024)
xi =mcfit.P2xi(kh,l=0)
#Calculate corr from PS------
nxx = 50
Rmin = -2.0
Rmax = 2.0
rr = np.logspace(Rmin,Rmax,nxx)
rx,corrfunc =xi(pk,extrap=True)
corr = np.interp(rr,rx,corrfunc[0,:])
#Calculate ESD from corr------
nxx = 10
Rp = np.linspace(0.03,20.,nxx)
ESD = np.zeros(nxx)
for i in range(nxx):
tmp1 = integrate.quad(simR,Rp[i]+0.001,90.0,args=(rr,corr,Rp[i]),epsabs=1e-4)
tmp2 = integrate.quad(simLR,0.001,Rp[i],args=(rr,corr,Rp[i]),epsabs=1e-4)
ESD[i] = (4.0*tmp2[0]/Rp[i]/Rp[i]-2.0*tmp1[0])*omega_m*h #Luo et al 2017ApJ 836 38L EQ. 39-40
return {'Rp':Rp,'ESD':ESD}
def getPars():
"""
Purpose:
quickly get camb parameters object
follows example code from http://camb.readthedocs.io/en/latest/CAMBdemo.html
but with slightly different parameters
Inputs:
Returns:
the pars object
"""
#Set up a new set of parameters for CAMB
pars = camb.CAMBparams()
#This function sets up CosmoMC-like settings, with one massive neutrino and helium set using BBN consistency
#pars.set_cosmology(H0=67.5, ombh2=0.022, omch2=0.122, mnu=0.06, omk=0, tau=0.06) #why 0.122?
pars.set_cosmology(H0=67.51,
ombh2=0.022,
omch2=0.119,
mnu=0.06,
omk=0,
tau=0.06)
pars.set_dark_energy() #re-set defaults
pars.InitPower.set_params(ns=0.965, r=0)
return pars
def change_neutrino(mnu):
'''
mnu : neutrino mass (eV)
other params set to Planck 2018 results
'''
# setup six init params from the paper
params = camb.CAMBparams() # the obj stores params
params.set_cosmology(H0=67.4,
ombh2=0.022383,
omch2=0.122011,
omk=0,
tau=0.0543,
mnu=mnu,
neutrino_hierarchy='degenerate')
params.InitPower.set_params(As=np.exp(3.0448) * 1e-10, ns=0.96605)
params.set_for_lmax(2500, lens_potential_accuracy=0)
# calculate the results of params
results = camb.get_results(params)
# get power spec
power_spec = results.get_cmb_power_spectra(params,
CMB_unit="muK",
lmax=2500)
return power_spec
def change_curvature(omk):
'''
omk : curvature density
other params set to Planck 2018 results
'''
# setup six init params from the paper
params = camb.CAMBparams() # the obj stores params
params.set_cosmology(H0=67.4,
ombh2=0.022383,
omch2=0.122011,
omk=omk,
tau=0.0543)
params.InitPower.set_params(As=np.exp(3.0448) * 1e-10, ns=0.96605)
params.set_for_lmax(2500, lens_potential_accuracy=0)
# calculate the results of params
results = camb.get_results(params)
# get power spec
power_spec = results.get_cmb_power_spectra(params,
CMB_unit="muK",
lmax=2500)
return power_spec
def rspectrum(nu, r, sig, scaling=1.0):
"""
Calculates the CMB amplituded given a value of r and requested modes
"""
import camb
from camb import model, initialpower
import healpy as hp
#Set up a new set of parameters for CAMB
pars = camb.CAMBparams()
#This function sets up CosmoMC-like settings, with one massive neutrino and helium set using BBN consistency
pars.set_cosmology(H0=67.5, ombh2=0.022, omch2=0.122, mnu=0.06, omk=0, tau=0.06)
pars.InitPower.set_params(As=2e-9, ns=0.965, r=r)
lmax=6000
pars.set_for_lmax(lmax, lens_potential_accuracy=0)
pars.WantTensors = True
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(params=pars, lmax=lmax, CMB_unit='muK', raw_cl=True,)
l = np.arange(2,lmax+1)
if sig == "TT":
cl = powers['unlensed_scalar']
signal = 0
elif sig == "EE":
cl = powers['unlensed_scalar']
signal = 1
elif sig == "BB":
cl = powers['tensor']
signal = 2
bl = hp.gauss_beam(40/(180/np.pi*60), lmax,pol=True)
A = np.sqrt(sum( 4*np.pi * cl[2:,signal]*bl[2:,signal]**2/(2*l+1) ))
return cmb(nu, A*scaling)
def compute_ffp8(ombh2, omch2, omnuh2, H0, tau, As, ns):
r'''
Computes a lensed TT `D_\ell` power spectrum given a set of cosmological
parameters.
'''
Neff = 3.046
params = camb.CAMBparams(
omnuh2=omnuh2,
H0=H0,
ombh2=ombh2,
omch2=omch2,
num_nu_massive=1,
num_nu_massless=Neff - 1,
nu_mass_degeneracies=[Neff / 3],
nu_mass_fractions=[1.0],
nu_mass_numbers=[1],
tau=tau,
WantTransfer=True,
# By default uses PArthENoPE
bbn_predictor=camb.bbn.BBN_table_interpolator())
params.InitPower.set_params(As=As, ns=ns) #, r=0)
params.Transfer.accurate_massive_neutrinos = True
params.Transfer.high_precision = True
params.set_for_lmax(2500, lens_potential_accuracy=1)
params.Reion.use_optical_depth = True
params.Reion.optical_depth = tau
result = camb.get_results(params)
return result.get_cmb_power_spectra(params, CMB_unit='muK')
def __init__(self,omega_m,sigma_8,h,z):
self.omega_m = omega_m
self.sigma_8 = sigma_8
self.h = h
self.z = z
self.k_max = 10.0
self.c = 2.99792e+5
#=========================
cosmo = camb.CAMBparams()
cosmo.set_cosmology(H0=100.0*self.h, ombh2=0.048*(self.h**2.0), omch2=(self.omega_m - 0.048)*(self.h**2.0), mnu=0.06, omk=0, tau=0.06)
cosmo.InitPower.set_params(As=2.0e-9, ns=0.973)
results = camb.get_results(cosmo)
cosmo.set_matter_power(redshifts=[0.0], kmax=10.0)
cambres= camb.get_transfer_functions(cosmo)
cosmo.NonLinear = model.NonLinear_both
kh, z, pk = cambres.get_matter_power_spectrum(minkh=1e-3, maxkh=1.0, npoints = 10)
sigma_8_temp = cambres.get_sigma8()
As_new = ((self.sigma_8/sigma_8_temp)**2.0)*(2.0e-9)
cosmo.InitPower.set_params(As=As_new, ns=0.973)
cambres = camb.get_results(cosmo)
backres = camb.get_background(cosmo)
self.chi = backres.comoving_radial_distance(self.z)
self.PK = camb.get_matter_power_interpolator(cosmo, nonlinear=True,
hubble_units=False, k_hunit=False, kmax=self.k_max, zmin = 0.0, zmax=self.z[-1])
self.H_z = (backres.hubble_parameter(self.z))/self.c #Hubble parameter in 1/Mpc
def parametrosCAMB():
#Se preparan los parámetros de CAMB
pars = camb.CAMBparams()
#Set cosmology || Se preparan los datos cosmológicos a como se desean.
pars.set_cosmology(H0=H00,
ombh2=omegab * pow(hubble, 2),
omch2=omegac * pow(hubble, 2),
omk=0,
mnu=0)
pars.set_dark_energy() #LCDM (default)
pars.InitPower.set_params(ns=nss, r=0, As=Ass)
pars.set_for_lmax(2500, lens_potential_accuracy=0)
#Se calculan resultados para esos parámetros
results = camb.get_results(pars)
#Get matter power spectrum at z=0: P(k,z=0)
pars.set_matter_power(redshifts=[0.], kmax=2.0)
#Linear spectra
pars.NonLinear = model.NonLinear_none
results.calc_power_spectra(pars)
kh, z, pk = results.get_matter_power_spectrum(minkh=1e-4,
maxkh=2.0,
npoints=200)
return kh, z, pk
def CL_mat(theta, pts, NL):
pars = camb.CAMBparams()
pars.set_cosmology(H0=theta[0],
ombh2=theta[1],
omch2=theta[2],
mnu=mnu,
omk=omk,
tau=theta[5])
pars.InitPower.set_params(As=theta[3], ns=theta[4], r=r)
pars.set_for_lmax(pts, lens_potential_accuracy=0)
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(pars, CMB_unit="muK")
totCL = powers['total']
ls = np.arange(totCL.shape[0])
TT = totCL[:, 0]
EE = totCL[:, 1]
TE = totCL[:, 3]
CL = []
for element in ls:
Cmatrix = np.zeros((2, 2))
Cmatrix[0, 0] = TT[element] + NL[element]
Cmatrix[1, 1] = EE[element] + NL[element]
Cmatrix[0, 1], Cmatrix[1, 0] = TE[element], TE[element]
CL.append(Cmatrix)
return (np.array(CL)[2:])
def camb_sigma8(cosmology, camb_params=None):
"""get camb sigma8
inputs:
cosmology: can vary H0, Omegabh2,Omegach2,Omegak,mnu,As,ns,OmegaL and w
camb_params: some parameters controling k
"""
if camb_params is None:
raise ValueError('need camb params')
pars = camb.CAMBparams()
pars.set_cosmology(H0=cosmology['H0'],
ombh2=cosmology['Omegabh2'],
omch2=cosmology['Omegach2'],
omk=cosmology['Omegak'],
mnu=cosmology['mnu'])
if 'As' in cosmology:
pars.InitPower.set_params(ns=cosmology['ns'], As=cosmology['As'])
else:
warn('cannot compute sigma8 reliably without input As')
pars.InitPower.set_params(ns=cosmology['ns'])
pars.set_dark_energy(cosmology['w']) #re-set defaults
pars.omegav = cosmology['OmegaL']
pars.set_matter_power(redshifts=[0.], kmax=camb_params['kmax'])
results = camb.get_results(pars)
sigma8 = results.get_sigma8()[0]
pars.set_dark_energy() #re-set defaults
return sigma8
def change_lambda(omlambda):
'''
omlambda : dark energy density
other params set to Planck 2018 results
'''
H0 = 67.4
h2 = (H0 * 0.01)**2
omm = 0.321
omb = 0.02212 / h2 / (omm + omlambda)
omc = 0.1206 / h2 / (omm + omlambda)
# calc ombh2 and omch2
ombh2 = omb * h2
omch2 = omc * h2
# setup six init params from the paper
params = camb.CAMBparams() # the obj stores params
params.set_cosmology(H0=H0, ombh2=ombh2, omch2=omch2, omk=0, tau=0.0543)
params.InitPower.set_params(As=np.exp(3.0448) * 1e-10, ns=0.96605)
params.set_for_lmax(2500, lens_potential_accuracy=0)
# calculate the results of params
results = camb.get_results(params)
# get power spec
power_spec = results.get_cmb_power_spectra(params,
CMB_unit="muK",
lmax=2500)
return power_spec
def Gencl(r=0.05, raw_cl=True, tensorBB_only=False):
'''
Generate the theoretical power spectra using camb
'''
pars = camb.CAMBparams()
pars.set_cosmology(H0=67.26,
ombh2=0.022,
omch2=0.1199,
mnu=0.06,
omk=0,
tau=0.078)
pars.InitPower.set_params(As=2.19856 * 1e-9, ns=0.9652, r=r)
pars.set_for_lmax(3000, lens_potential_accuracy=1)
pars.WantTensors = True
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(pars, CMB_unit='muK', raw_cl=raw_cl)
if tensorBB_only:
totCL = powers['tensor'] ## TT EE BB TE
return totCL.T[2]
else:
totCL = powers['total'] ## TT EE BB TE
return totCL.T
def get_spectrum_fix(pars, lmax=1500):
"""Give the power spectrum of the CMB using the camb package with tau fixed.
-Arguments: -pars (array): The parmaters for the model that will be updated
-lmax (array): Number of point at which we evaluate the function
-Returns: -tt (array): The power spectrum evaluated up to around lmax"""
H0 = pars[0]
ombh2 = pars[1]
omch2 = pars[2]
tau = 0.05
As = pars[3]
ns = pars[4]
pars = camb.CAMBparams()
pars.set_cosmology(H0=H0,
ombh2=ombh2,
omch2=omch2,
mnu=0.06,
omk=0,
tau=tau)
pars.InitPower.set_params(As=As, ns=ns, r=0)
pars.set_for_lmax(lmax, lens_potential_accuracy=0)
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(pars, CMB_unit='muK')
cmb = powers['total']
tt = cmb[:,
0] #you could return the full power spectrum here if you wanted to do say EE
return tt
def convert_mead_cosmology(cosm, verbose=False):
# Set up a new default set of parameters for CAMB
pars = camb.CAMBparams()
# Get CAMB cosmology from my structure
wb = cosm.w_b
wc = cosm.w_c
h = cosm.h
As = cosm.As
ns = cosm.ns
w = cosm.w
wa = cosm.wa
Om_k = cosm.Om_k
m_nu = cosm.m_nu
# This function sets standard and helium set using BBN consistency
pars.set_cosmology(ombh2=wb, omch2=wc, H0=100. * h, mnu=m_nu, omk=Om_k)
pars.set_dark_energy(w=w, wa=wa, dark_energy_model='ppf')
pars.InitPower.set_params(As=As, ns=ns, r=0)
# Print out the full list of cosmological parameters
if (verbose):
print(pars)
return pars
def __init__(self, params=None, smica_path=None): # Setting cosmo params if params is None: params = def_cosmo.copy() else: for key, val in def_cosmo.iteritems(): params.setdefault(key,val) self.params = params.copy() #Let's initialize CAMB for distances, growth factor ders, and CMB TT spectrum self.pars = camb.CAMBparams() self.pars.set_cosmology(H0=self.params['H0'], ombh2=self.params['ombh2'], omch2=self.params['omch2'], mnu=self.params['mnu'], omk=self.params['omk'], tau=self.params['tau']) self.pars.InitPower.set_params(As=params['As'], ns=params['ns'], r=0) self.pars.set_for_lmax(2500, lens_potential_accuracy=0); results = camb.get_results(self.pars) self.bkd = camb.get_background(self.pars) self.eta_star = self.bkd.conformal_time(1089) # conformal time at recombination cmb = results.get_cmb_power_spectra(self.pars,lmax=1000, raw_cl=True) self.TCMBmuK = 2.726e6 self.cltt = np.copy(cmb['lensed_scalar'][:,0])*self.TCMBmuK**2 # muK^2 self.zmin = 0 self.zmax = 8 self.nz = 300 self.z = np.linspace(self.zmin,self.zmax,self.nz) ev = results.get_redshift_evolution(1e-2, self.z, ['growth']) self.growth_eta = UnivariateSpline(self.bkd.conformal_time(self.z[::-1]), ev[:, 0][::-1], ext=3) self.der_growtg_eta = self.growth_eta.derivative() if smica_path is None: self.smica_path = '/Users/fbianchini/Research/pSZ/data/smica_nside512.fits' self.smica_init = False
def make_cl(r=0,
return_cl=True,
Alens=1.,
lmax=2500,
tau=0.054,
As=2.1e-9,
ombh2=0.02227716,
omch2=0.1184293):
pars = camb.CAMBparams()
pars.WantTensors = True
pars.set_cosmology(H0=67.86682,
ombh2=ombh2,
omch2=omch2,
mnu=0.06,
omk=0,
tau=tau)
pars.InitPower.set_params(ns=0.9682903, r=r, As=As)
pars.set_for_lmax(lmax - 50, lens_potential_accuracy=0)
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(pars, CMB_unit='muK')
if Alens == 0:
totCL = powers['unlensed_total'].T
else:
tot_tensor = powers['tensor'].T
tot_lens = powers['lensed_scalar'].T * Alens
totCL = tot_tensor + tot_lens
if return_cl:
l = np.arange(len(totCL[0]))
totCL = 2 * np.pi * totCL / l / (l + 1)
totCL[:, 0] = 0
return totCL
def test_cosmology_init(self):
pars = camb.CAMBparams(**self.cosmo_opts)
cosmo = Cosmology(pars)
self.assertIs(cosmo.camb_params.WantTensors, False)
self.assertIs(cosmo.camb_params.DoLateRadTruncation, False)
self.assertIs(cosmo.camb_params.WantCls, True)
self.assertIs(cosmo.camb_params.WantTransfer, False)
self.assertIs(cosmo.camb_params.DoLensing, True)
self.assertEqual(cosmo.camb_params.Accuracy.AccuracyBoost, 2)
self.assertEqual(cosmo.camb_params.Accuracy.lSampleBoost, 2)
self.assertEqual(cosmo.camb_params.Accuracy.lAccuracyBoost, 2)
self.assertIs(cosmo.camb_params.Accuracy.AccurateBB, True)
self.assertIs(cosmo.camb_params.Accuracy.AccurateReionization, True)
self.assertEqual(cosmo.camb_params.Accuracy.BessIntBoost, 30)
self.assertEqual(cosmo.camb_params.Accuracy.KmaxBoost, 3)
self.assertEqual(cosmo.camb_params.Accuracy.IntTolBoost, 4)
self.assertEqual(cosmo.camb_params.Accuracy.TimeStepBoost, 4)
self.assertEqual(cosmo.camb_params.Accuracy.SourcekAccuracyBoost, 5)
self.assertEqual(cosmo.camb_params.Accuracy.BesselBoost, 5)
self.assertEqual(cosmo.camb_params.Accuracy.IntkAccuracyBoost, 5)
self.assertEqual(cosmo.camb_params.Accuracy.lSampleBoost, 2)
self.assertEqual(cosmo.camb_params.Accuracy.IntkAccuracyBoost, 5)
self.assertEqual(cosmo.transfer, {})
self.assertEqual(cosmo.c_ell, {})
self.assertEqual(cosmo.red_bispectra, [])
def __init__(self, pk_zref=None):
"""
Setup cosmological model.
If pk_zref is set, it will compute linear power at z=pk_zref.
"""
self.pars = camb.CAMBparams()
ob = 0.02214
om = 0.1414
oc = om - ob
h = 0.719
self.pars.set_cosmology(H0=100.0 * h, ombh2=ob, omch2=oc)
self.pars.InitPower.set_params(As=2.2e-9, ns=0.961, r=0)
self.pk_zref = pk_zref
if self.pk_zref:
self.pars.set_matter_power(redshifts=[self.pk_zref], kmax=10.0)
# compute and store linear power spectrum (at zref)
self.pars.NonLinear = model.NonLinear_none
self.results = camb.get_results(self.pars)
else:
# compute only background expansion
self.results = camb.get_results(self.pars)
# not sure where to put this
self.c_kms = 2.998e5
self.lya_A = 1215.67 #Angstrom
def sigma2_fit(z=0, cosmo='Planck15'):
if type(cosmo)==str:
if cosmo.lower() in ['planck15']: cosmo = cosmology.Planck15
elif cosmo.lower() in ['planck13']: cosmo = cosmology.Planck13
elif cosmo.lower() in ['wmap9']: cosmo = cosmology.WMAP9
elif cosmo.lower() in ['wmap7']: cosmo = cosmology.WMAP7
elif cosmo.lower() in ['wmap5']: cosmo = cosmology.WMAP5
else:
print('Setting to Planck15 cosmology.')
cosmo = cosmology.Planck15
#Now get matter power spectra and sigma8 at redshift 0 and z
pars = camb.CAMBparams()
pars.set_cosmology(H0=cosmo.H0.value, ombh2=cosmo.Ob0*cosmo.h**2, omch2=cosmo.Om0*cosmo.h**2)
pars.InitPower.set_params(ns=0.96)
pars.set_matter_power(redshifts=[z], kmax=2.0)
#Linear spectra
#pars.NonLinear = model.NonLinear_none
results = camb.get_results(pars)
kh, zs, pk = results.get_matter_power_spectrum(minkh=1e-4, maxkh=1, npoints = 200)
s8 = np.array(results.get_sigma8())
rho_mean = cosmo.Om(z)*cosmo.critical_density(z)
Ms = 10**np.linspace(5,17,100)*units.solMass/cosmo.h
fM2R = lambda M: np.cbrt(3*M/(4*np.pi*rho_mean)).to('Mpc')
sigR = np.array([results.get_sigmaR(r.to('Mpc').value, z_indices=None, hubble_units=False, return_R_z=False) for r in tqdm(fM2R(Ms))]).squeeze()
sigM_tck = splrep(Ms.value, sigR)
return lambda x: splev(x.to('solMass').value if type(x)==units.quantity.Quantity else x, sigM_tck)
def get_camb_params(p,
num_massive_neutrinos=1,
neutrino_hierarchy='degenerate',
inpars=None):
pars = inpars or camb.CAMBparams()
if p.get('wa', 0) or p.get(
'alpha1', 0) or p.get('Alens', 1) != 1 or p.get('Aphiphi', 1) != 1:
raise Exception(
'Parameter not currrently supported by Cosmomc-> camb converter')
pars.set_cosmology(H0=p['H0'],
ombh2=p['omegabh2'],
omch2=p['omegach2'],
mnu=p.get('mnu', 0.06),
omk=p.get('omegak', 0),
tau=p['tau'],
deltazrei=p.get('deltazrei', None),
nnu=p.get('nnu', 3.046),
YHe=p.get('yheused', None),
meffsterile=p.get('meffsterile', 0),
num_massive_neutrinos=num_massive_neutrinos,
neutrino_hierarchy=neutrino_hierarchy)
pars.InitPower.set_params(ns=p['ns'],
r=p.get('r', 0),
As=p['A'] * 1e-9,
nrun=p.get('nrun', 0),
nrunrun=p.get('nrunrun', 0))
pars.set_dark_energy(w=p.get('w', -1))
pars.set_for_lmax(2500, lens_potential_accuracy=1)
return pars
def __initialize_CAMB(self): #{{{
# adds linear matter power interpolator
print 'Initializing CAMB.'
pars = camb.CAMBparams()
pars.set_cosmology(H0=self.H0,
ombh2=self.Ob * self.h**2.,
omch2=self.Oc * self.h**2.,
omk=0.,
mnu=self.Mnu,
standard_neutrino_neff=self.Neff,
nnu=self.Neff,
TCMB=self.TCMB)
pars.InitPower.set_params(ns=self.ns,
As=self.As,
pivot_scalar=self.pivot_scalar)
pars.NonLinear = model.NonLinear_none
# print(pars)
self.my_PK = get_matter_power_interpolator(pars,
zmin=0.,
zmax=6.,
nz_step=150,
kmax=101.,
nonlinear=False,
hubble_units=True,
k_hunit=True).P
pars.set_matter_power(redshifts=[0.], kmax=20.)
results = camb.get_results(pars)
self.sigma8 = results.get_sigma8()[0]
print 'sigma8 = ' + str(self.sigma8)
def getBAOCamb(zrange, params, AccuracyBoost=False):
'''
Get BAO's fk=rs/D_V from CAMB. Return 1D array of fk for all redshifts z
'''
pars = camb.CAMBparams()
if AccuracyBoost:
pars.set_accuracy(AccuracyBoost=2.0,
lSampleBoost=2.0,
lAccuracyBoost=2.0)
#pars.set_accuracy(AccuracyBoost=3.0, lSampleBoost=3.0, lAccuracyBoost=3.0)
pars.set_cosmology(H0=params['H0'],
ombh2=params['ombh2'],
omch2=params['omch2'],
tau=params['tau'],
mnu=params['mnu'],
nnu=params['nnu'],
omk=params['omk'])
pars.set_dark_energy(w=params['w'])
pars.InitPower.set_params(As=params['As'], ns=params['ns'], r=params['r'])
#pars.set_for_lmax(lmax=int(params['lmax']), lens_potential_accuracy=1, max_eta_k=2*params['lmax'])
camb.set_z_outputs(zrange)
results = camb.get_results(pars)
fk = results.get_background_outputs() #results.get_BAO(zrange,pars)[:,0]
#print fk
fk = np.nan_to_num(fk[:, 0])
return fk
def matter_power(*,
hub=0.7,
omega_b=0.049,
omega_c=0.25,
ns=0.965,
As=2.41e-9,
zz=3.):
"""Get a matter power spectrum using CAMB's python interface."""
#Set up a new set of parameters for CAMB
pars = camb.CAMBparams()
#This function sets up CosmoMC-like settings, with one massive neutrino and helium set using BBN consistency
pars.set_cosmology(H0=hub * 100,
ombh2=omega_b * hub**2,
omch2=omega_c * hub**2,
mnu=0.,
omk=0,
tau=0.06)
pars.InitPower.set_params(As=As, ns=ns, r=0)
if len(zz) == 1:
zz = [
zz,
]
pars.set_matter_power(redshifts=zz, kmax=10)
assert pars.validate()
pars.NonLinear = camb.model.NonLinear_none
results = camb.get_results(pars)
kh, _, pk = results.get_matter_power_spectrum(minkh=1e-2,
maxkh=10,
npoints=200)
return kh, pk
def testTimeTransfers(self):
from camb import initialpower
pars = camb.set_params(H0=69, YHe=0.22, lmax=2000, lens_potential_accuracy=1, ns=0.96, As=2.5e-9)
results1 = camb.get_results(pars)
cl1 = results1.get_total_cls()
pars = camb.set_params(H0=69, YHe=0.22, lmax=2000, lens_potential_accuracy=1)
results = camb.get_transfer_functions(pars, only_time_sources=True)
inflation_params = initialpower.InitialPowerLaw()
inflation_params.set_params(ns=0.96, As=2.5e-9)
results.power_spectra_from_transfer(inflation_params)
cl2 = results.get_total_cls()
np.testing.assert_allclose(cl1, cl2, rtol=1e-4)
inflation_params.set_params(ns=0.96, As=1.9e-9)
results.power_spectra_from_transfer(inflation_params)
inflation_params.set_params(ns=0.96, As=2.5e-9)
results.power_spectra_from_transfer(inflation_params)
cl2 = results.get_total_cls()
np.testing.assert_allclose(cl1, cl2, rtol=1e-4)
pars = camb.CAMBparams()
pars.set_cosmology(H0=78, YHe=0.22)
pars.set_for_lmax(2000, lens_potential_accuracy=1)
pars.WantTensors = True
results = camb.get_transfer_functions(pars, only_time_sources=True)
cls = []
for r in [0, 0.2, 0.4]:
inflation_params = initialpower.InitialPowerLaw()
inflation_params.set_params(ns=0.96, r=r, nt=0)
results.power_spectra_from_transfer(inflation_params)
cls += [results.get_total_cls(CMB_unit='muK')]
self.assertTrue(np.allclose((cls[1] - cls[0])[2:300, 2] * 2, (cls[2] - cls[0])[2:300, 2], rtol=1e-3))
def get_spectrum(par, lmax):
#print('pars are ',pars)
H0 = par[0]
ombh2 = par[1]
omch2 = par[2]
tau = par[3]
As = par[4]
ns = par[5]
pars = camb.CAMBparams()
pars.set_cosmology(H0=H0,
ombh2=ombh2,
omch2=omch2,
mnu=0.06,
omk=0,
tau=tau)
pars.InitPower.set_params(As=As, ns=ns, r=0)
pars.set_for_lmax(lmax, lens_potential_accuracy=0)
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(pars, CMB_unit='muK')
cmb = powers['total']
tt = cmb[:,
0] #you could return the full power spectrum here if you wanted to do say EE
return tt
def get_spectrum2(par, lmax):
#print('pars are ',pars)
#THIS FUNCTION IS ONLY USED TO GET THE COVARIANCE MATRIX FOR ALL 6 PARAMETERS AS MENTIONNNED IN QUESTION 3
H0 = par[0]
ombh2 = par[1]
omch2 = par[2]
tau = par[3]
As = par[4]
ns = par[5]
pars = camb.CAMBparams()
pars.set_cosmology(H0=H0,
ombh2=ombh2,
omch2=omch2,
mnu=0.06,
omk=0,
tau=tau)
pars.InitPower.set_params(As=As, ns=ns, r=0)
pars.set_for_lmax(lmax, lens_potential_accuracy=0)
results = camb.get_results(pars)
powers = results.get_cmb_power_spectra(pars, CMB_unit='muK')
cmb = powers['total']
tt = cmb[:,
0] #you could return the full power spectrum here if you wanted to do say EE
return tt