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Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
使用宇宙背景成像仪进行极化观测
A C S Readhead1, S T Myers, T J Pearson
1Owens Valley Radio Observatory, California Institute of Technology, Pasadena, CA 91125, USA. acr@astro.caltech.edu
概括
宇宙微波背景 (CMB) 偏振观测检测到E模式偏振. 观察到的光谱是指所观察到的光谱.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 宇宙微波背景辐射宇宙微波背景辐射
背景情况:
- 宇宙微波背景 (CMB) 是早期宇宙的遗留辐射.
- 了解CMB极化为我们提供了关于宇宙学参数和早期宇宙物理学的见解.
研究的目的:
- 检测和描述CMB的E模式偏振.
- 为了比较CMB偏振的角度功率光谱与总强度的角度功率光谱.
主要方法:
- 利用了从2002年9月至2004年5月期间收集的宇宙背景成像仪 (CBI) 的数据.
- 分析了CMB的极化观测结果.
主要成果:
- 在CMB中实现了对E模式偏振的显著检测.
- 观察到极化辐射的角度功率光谱,其中有峰值和谷值.
- 发现极化光谱的相位与总强度光谱相对转移了半个周期.
结论:
- 在光谱相的协议支持宇宙学的标准模型.
- 这些发现与由暗物质和暗能量主导的宇宙是一致的.
- 结果支持一个几乎平坦的几何形状和adiabatic原始密度波动,与通货膨胀模型保持一致.
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