Brief description
A numerical study of the homogeneous, isotropic (i.e., Friedmann)
model universes which are free of any pressure (i.e., are matter
dominated) is to be made for different values of the defining cosmological
parameters. The characteristics that might be investigated are the
behaviour of the scale factor and Hubble parameter with epoch and
the variation of angular diameter and luminosity distance with redshift.
These model predictions can be compared with recent observations
of distant supernovae to determine cosmological parameters.

Resources

