LARGE-SCALE STRUCTURE IN THE UNIVERSE

被引：41

作者：

KASHLINSKY, A ^{[1
]}

JONES, BJT ^{[1
]}

机构：

[1] UNIV SUSSEX, DEPT ASTRON, BRIGHTON BN1 9QH, E SUSSEX, ENGLAND

来源：

NATURE | 1991年 / 349卷 / 6312期

关键词：

D O I：

10.1038/349753a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

A variety of observations constrain models of the origin of large-scale cosmic structures. Enough observational data have accumulated to constrain (and perhaps determine) the power spectrum of primordial density fluctuations over a very large range of scales, independently of the particular cosmogonical theory assumed. Observations in the near future should be able to weed out many such theories.

引用

页码：753 / 760

页数：8

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