Towards the Limits of Cosmology

被引：4
作者：
Silk, Joseph [1 ,2 ,3 ,4 ]
机构：
[1] Inst Astrophys, 98 Bis Blvd Arago, F-75014 Paris, France
[2] Johns Hopkins Univ, Dept Phys & Astron, 3701 San Martin Dr, Baltimore, MD 21218 USA
[3] Univ Oxford, Dept Phys, Denys Wilkinson Bldg,1 Keble Rd, Oxford OX1 3RH, England
[4] Univ Oxford, Beecroft Inst Particle Astrophys & Cosmol, Denys Wilkinson Bldg,1 Keble Rd, Oxford OX1 3RH, England
来源：
FOUNDATIONS OF PHYSICS | 2018年 / 48卷 / 10期
关键词：
Cosmology; Dark matter; Dark energy; Cosmic microwave background; Radio astronomy; Inflation; MICROWAVE BACKGROUND SPECTRUM; DARK-MATTER; NEWTONIAN DYNAMICS; ROTATION; COLD; HALO;
D O I：
10.1007/s10701-018-0183-y
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
One of our greatest challenges in cosmology is understanding the origin of the structure of the universe. I will describe how the cosmic microwave background has provided a window for probing the initial conditions from which structure evolved and seeded the formation of the galaxies, and the outstanding issues that remain to be resolved. I will address our optimal choice of future strategy in order to make further progress on understanding our cosmic origins.
引用
收藏
页码：1305 / 1332
页数：28
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