cpod.templates.pycosmo_template_for_cpod_test.F = 1.14¶??? [under development]
cpod.templates.pycosmo_template_for_cpod_test.Nnu = 3.04¶Number of effective massless neutrino species [under development] [1]
cpod.templates.pycosmo_template_for_cpod_test.Tcmb = 2.725¶CMB temperature [K]
cpod.templates.pycosmo_template_for_cpod_test.Yp = 0.24¶Helium fraction [under development] [1]
cpod.templates.pycosmo_template_for_cpod_test.aini = 1e-07¶a used as initial starting point for Boltzman calculation - Warning: aini may now be a function k for some settings [under development]
cpod.templates.pycosmo_template_for_cpod_test.cosmics_dir = '../Tests/comparison_files/cosmics/zend_0/'¶COSMICS directory for recombination [under development]
cpod.templates.pycosmo_template_for_cpod_test.cosmo_nudge = [1.0, 1.0, 1.0]¶nudge factors for H0, omega_gam, and omega_neu to compare with other codes - set to [1.,1.,1.] or leave out to suppress nudge
cpod.templates.pycosmo_template_for_cpod_test.deltah = 1843785.9626¶Powerspectrum Normalisation (early time)
cpod.templates.pycosmo_template_for_cpod_test.fDM = 0.0¶??? [under development]
cpod.templates.pycosmo_template_for_cpod_test.h = 0.7¶dimensionless Hubble constant H0 = h*100km/s/Mpc [1]
cpod.templates.pycosmo_template_for_cpod_test.n = 1.0¶Spectral index for scalar modes [1]
cpod.templates.pycosmo_template_for_cpod_test.omega_b = 0.045¶Baryon density parameter (z=0) [1]
cpod.templates.pycosmo_template_for_cpod_test.omega_l_in = 'flat'¶Dark energy density. If ‘flat’ then omega_l is 1.- omega_m - omega_r [1]
cpod.templates.pycosmo_template_for_cpod_test.omega_m = 0.3¶Matter density paramater (dark matter + baryons) (z=0) [1]
cpod.templates.pycosmo_template_for_cpod_test.omega_r_0 = 0.0¶Radiation density (z=0)
cpod.templates.pycosmo_template_for_cpod_test.omega_suppress = False¶suppress radiation contribution in omega total as is often done
cpod.templates.pycosmo_template_for_cpod_test.pk_nonlin_type = 'halofit'¶sets if the nonlinear matter power spectrum should be calculated using the halofit fitting function (‘halofit’) or the revised halofit fitting function (‘rev_halofit’)
cpod.templates.pycosmo_template_for_cpod_test.pk_norm = 0.8¶Power spectrum normalisation value: either deltah or sigma8 depending on pk_norm_type setting
cpod.templates.pycosmo_template_for_cpod_test.pk_norm_type = 'sigma8'¶Power spectrum normalisation scheme: ‘deltah’ for CMB normalisation or ‘sigma8’ for sigma8 normalisation
cpod.templates.pycosmo_template_for_cpod_test.pk_type = 'EH'¶sets is the linear perturbations should be calculated using boltzman solver (‘boltz’) or approximations (‘EH’ for Einstein and Hu or ‘BBKS’)
cpod.templates.pycosmo_template_for_cpod_test.recomb = 'recfast++'¶code to compute recombination: ‘recfast++’ or ‘cosmics’ [under development]
cpod.templates.pycosmo_template_for_cpod_test.sigma8_0 = 0.8¶Powerspectrum Normalisation (z=0)
cpod.templates.pycosmo_template_for_cpod_test.tau = 0.09¶Optical depth [under development]
cpod.templates.pycosmo_template_for_cpod_test.w0 = -1.0¶DE equation of state at z=0 [1]
cpod.templates.pycosmo_template_for_cpod_test.wa = 0.0¶DE equation of state evolution such that w(a)=w0+wa(1-a) [1]