Can local inhomogeneity of the Universe explain the accelerating expansion?

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Open Astronomy Pub Date : 2022-01-01 DOI:10.1515/astro-2022-0003
Sobir Turaev, S. Nuritdinov
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Abstract

Abstract This paper discusses the disordering of the principle of cosmology on a small scale, i.e. the possibility of interpreting the observational data of type Ia Supernovae (SNe Ia) through the inhomogeneity and anisotropy of the Universe. The expansion of the Universe may appear to be accelerating due to “dark flows”, changes in the wavelength of light passing through “voids” and clusters, or anisotropy. Different sets of cosmological data are also considered without the need for a dark energy component.
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宇宙的局部不均匀性能解释加速膨胀吗?
摘要在小尺度上讨论了宇宙学原理的无序性,即通过宇宙的非均匀性和各向异性来解释Ia型超新星观测数据的可能性。由于“暗流”、穿过“空洞”和星系团的光的波长变化或各向异性,宇宙的膨胀可能看起来正在加速。不同的宇宙学数据集也被考虑在不需要暗能量成分的情况下。
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来源期刊
Open Astronomy
Open Astronomy Physics and Astronomy-Astronomy and Astrophysics
CiteScore
1.30
自引率
14.30%
发文量
37
审稿时长
16 weeks
期刊介绍: The journal disseminates research in both observational and theoretical astronomy, astrophysics, solar physics, cosmology, galactic and extragalactic astronomy, high energy particles physics, planetary science, space science and astronomy-related astrobiology, presenting as well the surveys dedicated to astronomical history and education.
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