Steady-State theory and the cosmological controversy

H. Kragh
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引用次数: 0

Abstract

The presently accepted big-bang model of the universe emerged during the period 1930-1970, following a road that was anything but smooth. By 1950 the essential features of the big-bang theory were established by George Gamow and his collaborators, and yet the theory failed to win recognition. A major reason was that the big-bang picture of the evolving universe was challenged by the radically different picture of a steady-state universe favoured by Fred Hoyle and others. By the late 1950s there was no convincing reason to adopt one theory over the other. Out of the epic controversy between the two incompatible world models arose our modern view of the universe. Although the classical steady-state model was abandoned in the mid-1960s, attempts to modify it can be followed up to the present.
稳态理论与宇宙学之争
目前被接受的宇宙大爆炸模型是在1930-1970年期间出现的,它走过了一条不平坦的道路。到1950年,乔治·伽莫夫和他的合作者建立了大爆炸理论的基本特征,但该理论未能赢得认可。一个主要的原因是,弗雷德·霍伊尔等人所支持的宇宙稳定状态的完全不同的观点,对宇宙演化的大爆炸理论提出了挑战。到20世纪50年代末,没有令人信服的理由来采用一种理论而不是另一种理论。在两种不相容的世界模型之间的史诗般的争论中,产生了我们现代的宇宙观。尽管经典的稳态模型在20世纪60年代中期被抛弃,但对其进行修正的尝试可以延续到现在。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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