

FLRW
======================

.. currentmodule:: astropy.cosmology

.. autoclass:: FLRW
   :show-inheritance:

   
     
   

   
   

   .. rubric:: Attributes Summary

   .. autosummary::
   
      ~FLRW.H0
      ~FLRW.Neff
      ~FLRW.Ob0
      ~FLRW.Ode0
      ~FLRW.Odm0
      ~FLRW.Ogamma0
      ~FLRW.Ok0
      ~FLRW.Om0
      ~FLRW.Onu0
      ~FLRW.Tcmb0
      ~FLRW.Tnu0
      ~FLRW.critical_density0
      ~FLRW.h
      ~FLRW.has_massive_nu
      ~FLRW.hubble_distance
      ~FLRW.hubble_time
      ~FLRW.m_nu

   
   

   
   

   .. rubric:: Methods Summary

   .. autosummary::
   
      ~FLRW.H
      ~FLRW.Ob
      ~FLRW.Ode
      ~FLRW.Odm
      ~FLRW.Ogamma
      ~FLRW.Ok
      ~FLRW.Om
      ~FLRW.Onu
      ~FLRW.Tcmb
      ~FLRW.Tnu
      ~FLRW.abs_distance_integrand
      ~FLRW.absorption_distance
      ~FLRW.age
      ~FLRW.angular_diameter_distance
      ~FLRW.angular_diameter_distance_z1z2
      ~FLRW.arcsec_per_kpc_comoving
      ~FLRW.arcsec_per_kpc_proper
      ~FLRW.clone
      ~FLRW.comoving_distance
      ~FLRW.comoving_transverse_distance
      ~FLRW.comoving_volume
      ~FLRW.critical_density
      ~FLRW.de_density_scale
      ~FLRW.differential_comoving_volume
      ~FLRW.distmod
      ~FLRW.efunc
      ~FLRW.inv_efunc
      ~FLRW.kpc_comoving_per_arcmin
      ~FLRW.kpc_proper_per_arcmin
      ~FLRW.lookback_distance
      ~FLRW.lookback_time
      ~FLRW.lookback_time_integrand
      ~FLRW.luminosity_distance
      ~FLRW.nu_relative_density
      ~FLRW.scale_factor
      ~FLRW.w

   
   

   
   

   .. rubric:: Attributes Documentation

   
   .. autoattribute:: H0
   .. autoattribute:: Neff
   .. autoattribute:: Ob0
   .. autoattribute:: Ode0
   .. autoattribute:: Odm0
   .. autoattribute:: Ogamma0
   .. autoattribute:: Ok0
   .. autoattribute:: Om0
   .. autoattribute:: Onu0
   .. autoattribute:: Tcmb0
   .. autoattribute:: Tnu0
   .. autoattribute:: critical_density0
   .. autoattribute:: h
   .. autoattribute:: has_massive_nu
   .. autoattribute:: hubble_distance
   .. autoattribute:: hubble_time
   .. autoattribute:: m_nu

   
   

   
   

   .. rubric:: Methods Documentation

   
   .. automethod:: H
   .. automethod:: Ob
   .. automethod:: Ode
   .. automethod:: Odm
   .. automethod:: Ogamma
   .. automethod:: Ok
   .. automethod:: Om
   .. automethod:: Onu
   .. automethod:: Tcmb
   .. automethod:: Tnu
   .. automethod:: abs_distance_integrand
   .. automethod:: absorption_distance
   .. automethod:: age
   .. automethod:: angular_diameter_distance
   .. automethod:: angular_diameter_distance_z1z2
   .. automethod:: arcsec_per_kpc_comoving
   .. automethod:: arcsec_per_kpc_proper
   .. automethod:: clone
   .. automethod:: comoving_distance
   .. automethod:: comoving_transverse_distance
   .. automethod:: comoving_volume
   .. automethod:: critical_density
   .. automethod:: de_density_scale
   .. automethod:: differential_comoving_volume
   .. automethod:: distmod
   .. automethod:: efunc
   .. automethod:: inv_efunc
   .. automethod:: kpc_comoving_per_arcmin
   .. automethod:: kpc_proper_per_arcmin
   .. automethod:: lookback_distance
   .. automethod:: lookback_time
   .. automethod:: lookback_time_integrand
   .. automethod:: luminosity_distance
   .. automethod:: nu_relative_density
   .. automethod:: scale_factor
   .. automethod:: w

   
   