Big Bang Time Line大爆炸时间线
Cosmological models of the "Big Bang" expansion of the universe have converged on a general framework in time, energy, and temperature. Below is an attempt to show some of the features of the models on a time line. 宇宙大爆炸扩张的宇宙学模型在时间、能量和温度方面已达成共识。以下尝试在时间线上展示一些模型的特征。
The later parts of this time line follow the chronology suggested by Steven Weinberg in "The First Three Minutes". The models are extended to earlier times back to the Planck time when the unification of all the fundamental forces is presumed. In order to deal with some problems with the standard big bang model, Guth introduced the idea of an extraordinarily rapid inflationary epoch. Along the time line there are three spontaneous symmetry breaks which separate the unified force into the four fundamental forces operating in today's universe. 本时间线的后半部分遵循史蒂文·温伯格在《前三分钟》中所建议的编年顺序。模型被延伸至更早的时间,追溯到普朗克时间,当时假设所有基本力的统一。为了处理标准大爆炸模型中的一些问题,古特引入了极其迅速的暴胀时期的想法。在时间线中,有三个自发对称破缺事件,将统一的力分离为今天宇宙中运作的四种基本力。
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改编自Kaufmann的数据来自Guth等人 |
Index References Guth Kaufmann Ch. 29 索引参考 Guth 和 Kaufmann 的第29章 | |||
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