astropy_background ================================================ Calculate background cosmology using astropy +-------------+---------------------------------------------------------+ | File | background/astropy_background/astropy_background.py | +-------------+---------------------------------------------------------+ | Attribution | CosmoSIS Team (interface) | +-------------+---------------------------------------------------------+ | | Astropy Team (library) | +-------------+---------------------------------------------------------+ | URL | https://docs.astropy.org/en/stable/cosmology/index.html | +-------------+---------------------------------------------------------+ | Citations | The Astropy Collaboration et al 2022 ApJ 935 167 | +-------------+---------------------------------------------------------+ The astropy cosmology library can compute background evolution distances as a function of redshift for a range of different cosmologies: - FlatLambdaCDM - FlatwCDM - Flatw0waCDM - LambdaCDM - wCDM - w0waCDM - w0wzCDM - w0wzCDM - wpwaCDM This module requires the user to choose one of these models and then will read the appropriate parameters for that model and compute a range of distance measures. Assumptions ----------- - Various depending on model choice Setup Parameters ---------------- .. list-table:: :header-rows: 1 * - Name - Type - Default - Description * - zmax - real - - Maximum redshift to compute distances to * - nz - real - - Number of redshift sample points to compute distances to * - model - str - - Name of the astropy model to use Input values ---------------- .. list-table:: :header-rows: 1 * - Section - Name - Type - Default - Description * - cosmological_parameters - hubble - real - - Hubble parameter today in km/s/Mpc * - - omega_m - real - - Dark matter density fraction today * - - omega_lambda - real - - Dark energy density fraction today. Only for some models. * - - w - real - - Dark energy equation of state today. Only for some models. * - - wa - real - - Dark energy equation of state scale factor derivative. Only for some models. * - - wz - real - - Dark energy equation of state redshift derivative today. Only for some models. * - - zp - real - - Redshift pivot for wpwaCDM model * - - wp - real - - Dark energy equation of state at zp for wpwaCDM model Output values ---------------- .. list-table:: Output values :header-rows: 1 * - Section - Name - Type - Description * - distances - z - real 1d - Redshifts of distance samples * - - a - real 1d - Scale factor of distance samples * - - d_a - real 1d - Angular diameter distance in Mpc * - - d_m - real 1d - Co-moving transverse distance in Mpc * - - d_l - real 1d - Luminosity distance in Mpc * - - mu - real 1d - Distance modulus * - - h - real 1d - Hubble parameter with in units of Mpc * - - d_v - real 1d - Comoving volume in Mpc^3 * - - d_c - real 1d - Comoving line-of-sight distance in Mpc