ANISOTROPIC ASYMPTOTIC-BEHAVIOR IN CHAOTIC INFLATION

被引：41

作者：

HEUSLER, M

机构：

[1] Institute for Theoretical Physics, University of Zürich, CH-8001 Zurich

来源：

PHYSICS LETTERS B | 1991年 / 253卷 / 1-2期

关键词：

D O I：

10.1016/0370-2693(91)91359-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We show that homogeneous cosmological models which are coupled to a scalar field can only approach isotropy at infinite times if the underlying Lie group is admitted by a Friedmann-Robertson-Walker model. This result generalizes a theorem of Collins and Hawking for matter satisfying the positive pressure condition to scalar fields with an arbitrary positive, convex potential having a local minimum at phi-0 with V[phi-0] = 0.

引用

页码：33 / 37

页数：5

共 16 条

[11]

LINDE AD, 1983, PHYS LETT B, V129, P177, DOI 10.1016/0370-2693(83)90837-7

[12] ANISOTROPY IN THE CHAOTIC INFLATIONARY UNIVERSE [J].