Cosmological Distance Scale. Part 5. Metrological Expert Opinion on Type SN Ia Supernovae

Аннотация

The detection of the accelerated expansion of the universe by the High-Z SN Search Team and the Supernova Cosmology Project is analyzed from the standpoint of solving the structural-parametric identification problem for the red-shift cosmological distance scale in the Friedman–Robertson–Walker model based on combined data for type SN Ia supernovae. A similar solution is given for the interpolation model.