A python package to calculate cosmological distances in a FRW metric.
A package to calculate cosmological distances. The workhorse is a class Cosmo that wraps and the underlying C code. The geometry can be non-flat.
In order to take advantage of the speed of the underlying C code, you should, if at all possible, send numpy arrays to the methods rather than repeatedly call the python methods.
python setup.py install --prefix=/some/path
import cosmology
c=cosmology.Cosmo()
# comoving distance to z=0.5
c.Dc(0.0, 0.5)
# angular diameter distance between z=0.5 and z=0.9
c.Da(0.5, 0.9)
# luminosity distance between z=0.2 and a sequence of redshifts
c.Dl(0.2, [0.3, 0.4, 0.5])
# new cosmology
c=cosmology.Cosmo(H0=70.0, omega_m=0.25)
# inverse critical density for lensing, lens at 0.2 and
# source at 0.3
c.sigmacritinv(0.2, 0.3)
import cosmology
cosmology.test()
- Add equation of state
- Add evolving equation of state.