Gravitational-wave physics and astronomy in the 2020s and 2030s
M. Bailes, B. K. Berger, P. R. Brady, M. Branchesi, K. Danzmann, M. Evans, Kelly Holley‐Bockelmann, B. R. Iyer, T. Kajita, S. Katsanevas, M. Krämer, A. Lazzarini, Luis Lehner, G. Losurdo, Harald Lück, D. E. McClelland, M. A. McLaughlin, M. Punturo, S. M. Ransom, Somak Raychaudhury, D. H. Reitze, F. Ricci, S. Rowan, Y. Saito, G. H. Sanders, B. S. Sathyaprakash, B. F. Schutz, Alberto Sesana, H. Shinkai, X. Siemens, D. H. Shoemaker, James Ira Thorpe, J. F. J. van den Brand, S. Vitale
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. In the past few years, gravitational-wave observations provided stunning insights into some of the most cataclysmic events in the Universe, heralding a bright future for gravitational-wave physics and astronomy. This is a Roadmap for the field in the coming two decades.