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一个4+1维宇宙模型
引用本文:朱炯明,朱世昌,郭汉英.一个4+1维宇宙模型[J].物理学报,1985,34(10):1342-1347.
作者姓名:朱炯明  朱世昌  郭汉英
作者单位:(1)上海师范大学物理系; (2)中国科学院理论物理研究所
摘    要:我们讨论的4+1维宇宙模型是通常的四维时空和一个紧致的一维内禀空间的直积空间。我们假定四维时空的能量密度是以辐射为主的,而内禀子空间的能动张量是一个阶跃函数。通过求解五维的Einstein场方程得到前四维时空由de-Sitter解过渡到标准模型的辐射为主解,与此同时内禀子空间的尺度由减幅振荡过渡到为按t的负幂次收缩而趋于一常量。 关键词

收稿时间:1984-11-30

A(4 + 1)-DIMENSIONAL COSMOLOGICAL MODEL
ZHU JIONG-MIN,ZHU SHI-CHANG and GUO HAN-YING.A(4 + 1)-DIMENSIONAL COSMOLOGICAL MODEL[J].Acta Physica Sinica,1985,34(10):1342-1347.
Authors:ZHU JIONG-MIN  ZHU SHI-CHANG and GUO HAN-YING
Abstract:The (4+1)-dimensional cosmological model discussed in this paper is a direct product of the usual 4-dimensional spacetime and a. 1-dimensional compaetified internal space. The energy density of the 4-dimensional spacetime is supposed to be dominated by incoherent radiation and the energy-momentum tensor of the internal subspace is a step function. By solving the 5-dimensional Einstein field equations without cosmolog-ical term we get the de-Sitter solution to describe the usual spacetime and at a certain time it changes to the radiation-dominated solution for standard model, and the size of the internal subspace changes with time in a form of oscillation with amplitude attenuating and then contracts to a constant.
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