ON THE ORIGIN OF COSMIC STRUCTURE

被引:5
作者
LAYZER, D
机构
[1] Department of Astronomy, Harvard University, Cambridge
关键词
COSMOLOGY; THEORY; GALAXIES; FORMATION; LARGE-SCALE STRUCTURE OF UNIVERSE;
D O I
10.1086/186412
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A parameter-free theory of the origin and evolution of structure in an initially cold Friedmann universe predicts that self-gravitating systems, from stars and planetary systems to galaxy clusters, are formed from the bottom up by repeated clustering, while a qualitatively different kind of structure, characterized by convex, connected, underdense regions and connected sheetlike or filamentary overdense regions, evolves from quantum fluctuations at the Planck era.
引用
收藏
页码:L5 / L8
页数:4
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