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单词 Dark flow
释义

Dark flow

中文百科

宇宙暗流

Full-sky image derived from nine years' WMAP data
Panoramic view of galaxies beyond Milky Way, with Norma cluster & Great Attractor shown by a long blue arrow at the bottom-right in image near the disk of the Milky Way.
The dark flow. The colored dots are clusters within one of four distance ranges, with redder colors indicating greater distance. Colored ellipses show the direction of bulk motion for the clusters of the corresponding color. Images of representative galaxy clusters in each distance slice are also shown. Image credit: A. Kashlinsky (NASA).

宇宙暗流英语:Dark Flow),天体物理学用语,2008年最新发表的研究表明多数星系团以本动速度共通的大规模的速度场(纯粹的偏置值)天文现象而给予的学术名称。这是一种科学假说。本动速度与宇宙微波背景辐射(CMB)为基准的情况下,以哈伯定律预测星系团的运动与实际观测运动的偏差。(但是,银河团是太远方角度方向的运动是无法观测。可观测的运动多普勒转移从可观测的视线方向的运动而已。另外,通常这些偏差的原因是无法说明,因此“黑暗”被表现。)

根据标准的宇宙学模型,相对于宇宙微波背景星系团的运动应该是随机分布在所有方向。然而,分析三年的威尔金森微波各向异性探测器(WMAP)使用的运动SZ效应数据,天文学家亚力山大.卡什林斯基等科学家发现了一个“令人惊讶的是一致的“600–1000公里/秒流集群,向20度天区的半人马座和船帆星座之间的证据。

英语百科

Dark flow 宇宙暗流

Full-sky image derived from nine years' WMAP data
Panoramic view of galaxies beyond Milky Way, with Norma cluster & Great Attractor shown by a long blue arrow at the bottom-right in image near the disk of the Milky Way.
The dark flow. The colored dots are clusters within one of four distance ranges, with redder colors indicating greater distance. Colored ellipses show the direction of bulk motion for the clusters of the corresponding color. Images of representative galaxy clusters in each distance slice are also shown. Image credit: A. Kashlinsky (NASA).

Dark flow is an astrophysical term describing a possible non-random component of the peculiar velocity of galaxy clusters. The actual measured velocity is the sum of the velocity predicted by Hubble's Law plus a possible small and unexplained (or dark) velocity flowing in a common direction.

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更新时间:2025/6/26 2:24:24