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哈勃常数为 30km/s/Mpc 的案例。

The Case for a Hubble Constant of 30 km s-1 Mpc-1.

出版信息

Science. 1995 Feb 17;267(5200):980-3. doi: 10.1126/science.267.5200.980.

Abstract

Although recent determinations of the distance to the Virgo cluster based on Cepheid variable stars represent an important step in pinning down the Hubble constant, after 65 years a definitive determination of the Hubble constant still eludes cosmologists. At present, most of the observational determinations place the Hubble constant between 40 and 90 kilometers per second per megaparsec (km s(-1) Mpc(-1)). The case is made here for a Hubble constant that is even smaller than the lower bound of the accepted range on the basis of the great advantages, all theoretical in nature, of a Hubble constant of around 30 kilometers per second per megaparsec. Such a value for the Hubble cures all of the ills of the current theoretical orthodoxy, that is, a spatially flat universe composed predominantly of cold dark matter.

摘要

虽然最近基于造父变星确定的室女座星系团距离是确定哈勃常数的重要一步,但 65 年来,天文学家仍未能确定哈勃常数。目前,大多数观测结果都将哈勃常数置于每秒每百万秒差距 40 到 90 公里(km/s/Mpc)之间。本文基于哈勃常数为 30km/s/Mpc 左右时具有的巨大优势,这些优势均具有理论上的必然性,提出了哈勃常数甚至比已被接受的范围下限还要小的观点。这样的值可以治愈当前理论正统观念的所有弊病,即一个主要由冷暗物质组成的、空间平坦的宇宙。

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