INFLATIONARY MODELS WITH OMEGA NOT-EQUAL 1

被引：28

作者：

ELLIS, GFR

LYTH, DH

MIJIC, MB

机构：

[1] CALIF STATE UNIV LOS ANGELES,DEPT PHYS & ASTRON,LOS ANGELES,CA 90032

[2] UNIV CAPE TOWN,DEPT APPL MATH,RONDEBOSCH 7700,SOUTH AFRICA

[3] UNIV LANCASTER,DEPT PHYS,LANCASTER LA1 4YB,ENGLAND

来源：

PHYSICS LETTERS B | 1991年 / 271卷 / 1-2期

关键词：

D O I：

10.1016/0370-2693(91)91277-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe the general features and a few specific models of inflationary cosmology that lead to OMEGA not-equal 1 today, solve all standard problems of classical cosmology, and generate density perturbations that may be responsible for the formation of structures in the universe. Further development along these lines may require a more elaborate analysis of the initial conditions, both for the classical evolution and for the density perturbations.

引用

页码：52 / 60

页数：9

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