Gravitational-wave physics and astronomy in the 2020s and 2030s

M. Bailes, B. K. Berger, P. R. Brady, M. Branchesi, K. Danzmann, M. Evans, K. Holley-Bockelmann, B. R. Iyer, T. Kajita, S. Katsanevas, M. Kramer, A. Lazzarini, L. Lehner, G. Losurdo, H. Lück, D. E. McClelland, M. A. McLaughlin, M. Punturo, S. Ransom, S. RaychaudhuryD. H. Reitze, F. Ricci, S. Rowan, Y. Saito, G. H. Sanders, B. S. Sathyaprakash, B. F. Schutz, A. Sesana, H. Shinkai, X. Siemens, D. H. Shoemaker, J. Thorpe, J. F.J. van den Brand, S. Vitale

Research output: Contribution to journalReview articlepeer-review

7 Scopus citations

Abstract

The 100 years since the publication of Albert Einstein’s theory of general relativity saw significant development of the understanding of the theory, the identification of potential astrophysical sources of sufficiently strong gravitational waves and development of key technologies for gravitational-wave detectors. In 2015, the first gravitational-wave signals were detected by the two US Advanced LIGO instruments. In 2017, Advanced LIGO and the European Advanced Virgo detectors pinpointed a binary neutron star coalescence that was also seen across the electromagnetic spectrum. The field of gravitational-wave astronomy is just starting, and this Roadmap of future developments surveys the potential for growth in bandwidth and sensitivity of future gravitational-wave detectors, and discusses the science results anticipated to come from upcoming instruments.

Original languageEnglish (US)
Pages (from-to)344-366
Number of pages23
JournalNature Reviews Physics
Volume3
Issue number5
DOIs
StatePublished - May 2021

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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