COSMIC BACKGROUND-RADIATION ANISOTROPY IN AN OPEN INFLATION, COLD DARK-MATTER COSMOGONY

被引：51

作者：

KAMIONKOWSKI, M

RATRA, B

SPERGEL, DN

SUGIYAMA, N

机构：

[1] PRINCETON UNIV,JOSEPH HENRY LABS,PRINCETON,NJ 08544

[2] PRINCETON UNIV OBSERV,PRINCETON,NJ 08544

[3] UNIV CALIF BERKELEY,DEPT ASTRON,BERKELEY,CA 94720

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

来源：

ASTROPHYSICAL JOURNAL | 1994年 / 434卷 / 01期

关键词：

COSMIC MICROWAVE BACKGROUND; GALAXIES; FORMATION; LARGE-SCALE STRUCTURE OF THE UNIVERSE;

D O I：

10.1086/187558

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We compute the cosmic background radiation anisotropy, produced by energy-density fluctuations generated during an early epoch of inflation, in an open cosmological model based on the cold dark matter scenario. At Omega(0) similar to 0.3-0.4, the COBE normalized open model appears to be consistent with most observations.

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页码：L1 / L4

页数：4

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