Cosmological Distance Scale. Part 6. Statistical Anisotropy of Red Shift
- 作者: Levin S.1
-
隶属关系:
- Moscow Institute of Appraisal and Testing
- 期: 卷 60, 编号 5 (2017)
- 页面: 411-417
- 栏目: Fundamental Problems in Metrology
- URL: https://journals.rcsi.science/0543-1972/article/view/246153
- DOI: https://doi.org/10.1007/s11018-017-1211-6
- ID: 246153
如何引用文章
详细
The data on the type SN Ia supernovae used to confirm the accelerated “expansion of the universe” in 1998–1999 are analyzed statistically. A substantial statistical anisotropy with respect to declination is found in these data. It is shown that an examination of the relationship between the red shift of SN Ia supernovae and the photometric distance based on these data is not the most plausible hypothesis. An example of the construction of an anisotropic cosmological distance scale is given.
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