Scalar field cosmologies with barotropic matter:: models of Bianchi class B

被引：28

作者：

Billyard, AP ^{[1
]}

Coley, AA

van den Hoogen, RJ

Ibáñez, J

Olasagasti, I

机构：

[1] Dalhousie Univ, Dept Math & Stat, Halifax, NS B3H 3J5, Canada

[2] St Francis Xavier Univ, Dept Math Stat & Comp Sci, Antigonish, NS B2G 2W5, Canada

[3] Univ Basque Country, Dept Fis Teor, E-48080 Bilbao, Spain

来源：

CLASSICAL AND QUANTUM GRAVITY | 1999年 / 16卷 / 12期

关键词：

D O I：

10.1088/0264-9381/16/12/320

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We investigate in detail the qualitative behaviour of the class of Bianchi type B spatially homogeneous cosmological models in which the matter content is composed of two noninteracting components; the first component is described by a barotropic fluid having a gamma-law equation of state, whilst the second is a non-interacting scalar field phi with an exponential potential V(phi) = Lambda e(k phi). In particular, we study the asymptotic properties of the models both at early and late times, paying particular attention to whether the models isotropize (and inflate) to the future, and we discuss the genericity of the cosmological scaling solutions.

引用

页码：4035 / 4056

页数：22

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