wcosmo.wcosmo.comoving_volume#

wcosmo.wcosmo.comoving_volume(z, H0, Om0, w0=-1, method='pade')[source]#

Compute the comoving volume out to redshift z.

\[V_C = \frac{4\pi}{3} d^3_C(z; H_0, \Omega_{m,0}, w_0)\]
Parameters:
z: array_like

Redshift

H0: array_like

The Hubble constant in km/s/Mpc

Om0: array_like

The matter density fraction

w0: array_like

The (constant) equation of state parameter for dark energy

Returns:
Vc: array_like

The comoving volume in \(\rm{Gpc}^3\)