宇宙等离子体对 Ia 超新星观测的影响

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Research in Astronomy and Astrophysics Pub Date : 2023-12-06 DOI:10.1088/1674-4527/ad12fb
Yi-jia Zheng
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引用次数: 0

摘要

在观测宇宙学中,超新星Ia被用作标准烛光,以便将哈勃图扩展到更高的红移范围。天体物理学家发现,观测到的高红移超新星Ia的亮度比预期的要暗。这种变暗效应被认为是宇宙中存在暗能量的观测证据。应该指出的是,这个结论是基于宇宙等离子体的质量密度非常小的假设。因此,宇宙等离子体中自由电子的康普顿散射引起的变暗效应可以忽略不计。x射线观测表明,宇宙等离子体的质量密度可能非常大。理论上,观测到的高红移超新星Ia的变暗效应可能是由宇宙等离子体中自由电子的康普顿散射引起的。本文将证明这种想法是合理的。因此,没有必要在宇宙学中引入令人困惑的暗能量概念。
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Effect of cosmic plasma on the observation of Supernovae Ia
In observational cosmology, Supernova Ia is used as a standard candle in order to extend the Hubble diagram to a higher redshift range. Astrophysicists found that the observed brightness of high redshift supernovae Ia is dimmer than expected. This dimming effect is considered observational evidence for the existence of dark energy in the universe. It should be noted that this conclusion is based on an assumption that the mass density of the cosmic plasma is very small. Therefore, the dimming effect caused by the Compton scattering of free electrons in cosmic plasma can be neglected. X-Ray observations suggest that the mass density of the cosmic plasma may be very large. In theory, the observed dimming effect of high redshift supernovae Ia may be caused by the Compton scattering of free electrons in the cosmic plasma. In this paper it will be shown that this idea is reasonable. Therefore, there is no need to introduce the confusing concept of dark energy into cosmology.
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来源期刊
Research in Astronomy and Astrophysics
Research in Astronomy and Astrophysics 地学天文-天文与天体物理
CiteScore
3.20
自引率
16.70%
发文量
2599
审稿时长
6.0 months
期刊介绍: Research in Astronomy and Astrophysics (RAA) is an international journal publishing original research papers and reviews across all branches of astronomy and astrophysics, with a particular interest in the following topics: -large-scale structure of universe formation and evolution of galaxies- high-energy and cataclysmic processes in astrophysics- formation and evolution of stars- astrogeodynamics- solar magnetic activity and heliogeospace environments- dynamics of celestial bodies in the solar system and artificial bodies- space observation and exploration- new astronomical techniques and methods
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