Email this article Cosmological Distance Scale. Part 5. Metrological Expert Opinion on Type SN Ia Supernovae
- Authors: Levin S.F.1
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Affiliations:
- Moscow Institute of Appraisal and Testing
- Issue: Vol 59, No 8 (2016)
- Pages: 791-802
- Section: Fundamental Problems in Metrology
- URL: https://journals.rcsi.science/0543-1972/article/view/245443
- DOI: https://doi.org/10.1007/s11018-016-1047-5
- ID: 245443
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Abstract
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.
About the authors
S. F. Levin
Moscow Institute of Appraisal and Testing
Author for correspondence.
Email: AntoninaEL@rostest.ru
Russian Federation, Moscow
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