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


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Resumo

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.

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S. Levin

Moscow Institute of Appraisal and Testing

Autor responsável pela correspondência
Rússia, Moscow

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