1998-2003年革命

P. Peebles
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引用次数: 0

摘要

这一章着眼于从1998年到2003年的五年间经验宇宙学状态的变化,这足以被称为一场革命。它是由两项伟大的实验进展推动的。首先是测量一个物体的光谱红移和它在天空中的亮度之间的关系,给定它的亮度:宇宙学红移-星等关系。二是详细绘制宇宙微波背景辐射的角分布。这两个程序基本上同时达到了对宇宙学模型进行重要约束所需的精度。他们的解释很快就被接受了,这是因为这两种截然不同的看待宇宙的方式的含义令人印象深刻的一致性,同样重要的是,这与革命前多年研究中收集的其他证据的一致性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The 1998–2003 Revolution
This chapter looks at the change in the state of empirical cosmology in the five years from 1998 to 2003, which was great enough to be termed a revolution. It was driven by the two great experimental advances. The first is the measurement of the relation between the redshift of the spectrum of an object and its brightness in the sky, given its luminosity: the cosmological redshift–magnitude relation. The second is the detailed mapping of the angular distribution of the cosmic microwave background (CMB) radiation. The two programs reached the precision needed for significant constraints on cosmological models at essentially the same time. Quick acceptance of their interpretation was driven by the impressive consistency of implications of these two quite different ways to look at the universe and, equally important, by the consistency with other lines of evidence gathered in the years of research before the revolution.
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