Primordial Gravitational Waves and Cosmology

被引:41
|
作者
Krauss, Lawrence M. [1 ,2 ]
Dodelson, Scott [3 ,4 ,5 ]
Meyer, Stephan [4 ,5 ,6 ,7 ]
机构
[1] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA
[2] Arizona State Univ, Dept Phys, Tempe, AZ 85287 USA
[3] Ctr Particle Astrophys, Fermi Natl Lab, Batavia, IL 60510 USA
[4] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[5] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[6] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[7] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
基金
美国国家科学基金会;
关键词
INFLATIONARY UNIVERSE; GRAND UNIFICATION; POLARIZATION; FLATNESS; HORIZON; CMB;
D O I
10.1126/science.1179541
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 observation of primordial gravitational waves could provide a new and unique window on the earliest moments in the history of the universe and on possible new physics at energies many orders of magnitude beyond those accessible at particle accelerators. Such waves might be detectable soon, in current or planned satellite experiments that will probe for characteristic imprints in the polarization of the cosmic microwave background, or later with direct space-based interferometers. A positive detection could provide definitive evidence for inflation in the early universe and would constrain new physics from the grand unification scale to the Planck scale.
引用
收藏
页码:989 / 992
页数:4
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