Stochastic gravitational wave backgrounds

被引：237

作者：

Christensen, Nelson ^{[1
,2
]}

机构：

[1] Univ Cote Azur, ARTEMIS, CNRS, Observ Cote Azur, F-06304 Nice, France

[2] Carleton Coll, Phys & Astron, Northfield, MN 55057 USA

来源：

REPORTS ON PROGRESS IN PHYSICS | 2019年 / 82卷 / 01期

基金：

俄罗斯科学基金会; 美国国家科学基金会; 澳大利亚研究理事会; 中国国家自然科学基金; 俄罗斯基础研究基金会; 英国科学技术设施理事会; 匈牙利科学研究基金会; 新加坡国家研究基金会; 瑞士国家科学基金会;

关键词：

gravitational waves; cosmology; astrophysics; BARYON ACOUSTIC-OSCILLATIONS; ROTATING NEUTRON-STARS; PRE-BIG-BANG; GENERAL-RELATIVITY; UPPER LIMITS; INFLATIONARY UNIVERSE; CBR ANISOTROPY; POPULATION-III; ADVANCED LIGO; BLACK-HOLES;

D O I：

10.1088/1361-6633/aae6b5

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A stochastic background of gravitational waves could be created by the superposition of a large number of independent sources. The physical processes occurring at the earliest moments of the universe certainly created a stochastic background that exists, at some level, today. This is analogous to the cosmic microwave background, which is an electromagnetic record of the early universe. The recent observations of gravitational waves by the Advanced LIGO and Advanced Virgo detectors imply that there is also a stochastic background that has been created by binary black hole and binary neutron star mergers over the history of the universe. Whether the stochastic background is observed directly, or upper limits placed on it in specific frequency bands, important astrophysical and cosmological statements about it can be made. This review will summarize the current state of research of the stochastic background, from the sources of these gravitational waves to the current methods used to observe them.

引用

页数：30

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