DIRECT OBSERVATION OF STRUCTURE IN THE COSMIC MICROWAVE BACKGROUND

被引：135
|
作者：
HANCOCK, S
DAVIES, RD
LASENBY, AN
DELACRUZ, CMG
WATSON, RA
REBOLO, R
BECKMAN, JE
机构：
[1] INST ASTROFIS CANARIAS,E-38071 LA LAGUNA,SPAIN
[2] UNIV CAMBRIDGE,CAVENDISH LAB,MULLARD RADIO ASTRON OBSERV,CAMBRIDGE CB3 0HE,ENGLAND
来源：
NATURE | 1994年 / 367卷 / 6461期
关键词：
D O I：
10.1038/367333a0
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：
Temperature fluctuations in the cosmic microwave background are a key prediction of cosmological models of structure formation in the early Universe. Ground-based multi-frequency radio observations of the microwave background reveal well defined features that are not of atmospheric or Galactic origin; instead, they delineate the primordial density perturbations from which the structure in the present Universe originated. The amplitude of these perturbations confirms the earlier statistical detection by the COBE satellite.
引用
收藏
页码：333 / 338
页数：6
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