Year: 2018
Type: article
Abstract: 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.
Source: Reports on Progress in Physics
Author: Nelson Christensen
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Funders: National Science Foundation, Institut des Origines de Lyon, Leverhulme Trust, Scottish Universities Physics Alliance, European Commission, Council of Scientific and Industrial Research, India, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, National Natural Science Foundation of China, Russian Foundation for Basic Research, Industry Canada, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Hungarian Scientific Research Fund, National Research Foundation of Korea, Ministry of Education, India, Centre National de la Recherche Scientifique, Russian Science Foundation, Ministero dello Sviluppo Economico, Nemzeti Kutatási Fejlesztési és Innovációs Hivatal, Istituto Nazionale di Fisica Nucleare, ICTP South American Institute for Fundamental Research, Science and Engineering Research Board, European Regional Development Fund, Agencia Estatal de Investigación, Division of Physics, National Research, Development and Innovation Office
Award: G2093914612
OpenAlex ID: W2897076601
