在分析非线性扩散模型中的部分Ly热化
1Institute for Theoretical Physics, Heidelberg University, Philosophenweg 16, Heidelberg, 69120, Baden Württemberg, Germany. wolschin@uni-hd.de.
Scientific reports
|February 28, 2024
概括
宇宙微波背景辐射受到中性气的干扰.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
背景情况:
- 在早期宇宙的重组时代.
- 宇宙微波背景 (CMB) 异形. 异形.
- 来自中性的莱曼-α (Lyα) 排放.
研究的目的:
- 为了建模Lyα能量的热化.
- 分析它对CMB的影响.
- 为了与观测数据进行比较.
主要方法:
- 分析的非线性扩散模型.
- 时间依赖的热化分析.
- 莱α线的红移.
主要成果:
- Lyα 能量部分热化.
- 由此产生的Lyα线幅度过低.
- 与普朗克的观测结果一致.
结论:
- 热化的Lyα线在CMB中无法检测到.
- 数字模型和普朗克数据支持这一发现.
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