THE END OF COLD DARK MATTER

被引：102

作者：

DAVIS, M

EFSTATHIOU, G

FRENK, CS

WHITE, SDM

机构：

[1] UNIV DURHAM, DEPT PHYS, DURHAM DH1 3LE, ENGLAND

[2] UNIV OXFORD, MULLARD & ASTROPHYS LAB, DEPT PHYS, OXFORD OX1 3RH, ENGLAND

[3] UNIV CAMBRIDGE, INST ASTRON, CAMBRIDGE CB3 0HA, ENGLAND

[4] UNIV CAMBRIDGE, INST ASTRON, DEPT PHYS, CAMBRIDGE CB3 0HA, ENGLAND

来源：

NATURE | 1992年 / 356卷 / 6369期

关键词：

D O I：

10.1038/356489a0

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：

The successful cold dark matter (CDM) theory for the formation of structure in the Universe has suffered recent setbacks from observational evidence suggesting that there is more large-scale structure than it can explain. This may force a fundamental revision or even abandonment of the theory, or may simply reflect a modulation of the galaxy distribution by processes associated with galaxy formation. Better understanding of galaxy formation is needed before the demise of CDM is declared.

引用

页码：489 / 494

页数：6

共 88 条

[1] COSMOLOGY FOR GRAND UNIFIED THEORIES WITH RADIATIVELY INDUCED SYMMETRY-BREAKING [J].