ΛCDMLambda Cold Dark Matter Concordance ModelLambda冷暗物质共识模型
In recent years there has been an intensive study of the expanding universe and Hubble's Law. Many experiments and lines of modeling have contributed to the evaluation of the universe's expansion. After the earlier COBE and WMAP satellite data, the Planck satellite collected data for 4.5 years and as of 2020 provides the most accurate evaluation of the CMB radiation. The graphical history of Hubble's Law evaluation shown below is from the NASA publication on the Hubble Constant, H0. 近年来,人们对膨胀的宇宙和哈勃定律进行了大量研究。许多实验和模型都为评估宇宙的膨胀做出了贡献。在早期的COBE和WMAP卫星数据之后,普朗克卫星进行了4.5年的数据收集,并截至2020年提供了对宇宙微波背景辐射最准确的评估。下面展示的哈勃定律评估的图形历史来自NASA关于哈勃常数H₀的出版物。
After the extensive data from the Planck satellite was received, the 2015 reports from the Planck Collaboration presented descriptive parameters for the universe in the ΛCDM concordance model:
在接收到来自普朗克卫星的大量数据后,普朗克合作组于2015年发布的报告给出了ΛCDM一致性模型中宇宙的描述性参数: |
Index NASA, Hubble Constant 索引 NASA,哈勃常数 | ||||||||||||||||||||||||
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Index Distance measurement Reference: 索引 距离测量 参考: | ||
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