在早期宇宙和今天的声学振荡
C J Miller1, R C Nichol, D J Batuski
1Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213, USA.
概括
科学家检测到宇宙微波背景 (CMB) 和物质分布中的声学振荡. 这些不同宇宙时间的发现支持热大爆炸模型.
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:
- 早期的宇宙是一个热的,有离子的等离子体与相结合的光子和物质.
- 引力崩和光子压力在这个原始流体中产生了声学振荡.
研究的目的:
- 将在宇宙微波背景 (CMB) 中检测到的声振荡与当今物质密度分布中的声振荡进行比较.
- 为标准热大爆炸模型提供进一步证据.
主要方法:
- 对 BOOMERANG 和 MAXIMA CMB 数据 (红移 ~ 1000) 的分析.
- 与物质密度功率光谱数据 (红移~0.1) 的比较.
主要成果:
- 在CMB中检测声学振荡.
- 在物质密度功率光谱中一致检测相应的振荡.
- 在CMB和物质分布观测之间达成协议.
结论:
- 来自两个不同的宇宙学时代的一致结果强烈支持标准热大爆炸模型.
- 声学振荡是早期宇宙物理学的可预测的印记.
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