IMPRINT OF OMEGA ON THE COSMIC MICROWAVE BACKGROUND

被引：35

作者：

SUGIYAMA, N

SILK, J

机构：

[1] UNIV CALIF BERKELEY, BERKELEY, CA 94720 USA

[2] UNIV CALIF BERKELEY, CTR PARTICLE ASTROPHYS, BERKELEY, CA 94720 USA

[3] UNIV TOKYO, FAC SCI, DEPT PHYS, TOKYO 113, JAPAN

[4] UNIV CALIF BERKELEY, DEPT PHYS, BERKELEY, CA 94720 USA

来源：

PHYSICAL REVIEW LETTERS | 1994年 / 73卷 / 04期

关键词：

D O I：

10.1103/PhysRevLett.73.509

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We investigate the dependence of large-angular-scale cosmic microwave background anisotropies on various initial conditions, including both adiabatic and isocurvature perturbations and the initial power-law index n, in a variety of low-OMEGA cosmological models. LAMBDA-dominated flat models, inflationary open adiabatic models, with n(eff) < 1, and open isocurvature models, with n(eff) congruent-to 2, are significantly constrained.

引用

页码：509 / 513

页数：5

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