Cosmological Distance Scale. Part 5. Metrological Expert Opinion on Type SN Ia Supernovae
- 作者: Levin S.F.1
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隶属关系:
- Moscow Institute of Appraisal and Testing
- 期: 卷 59, 编号 8 (2016)
- 页面: 791-802
- 栏目: 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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详细
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.
作者简介
S. Levin
Moscow Institute of Appraisal and Testing
编辑信件的主要联系方式.
Email: AntoninaEL@rostest.ru
俄罗斯联邦, Moscow
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