Ground Based Gravitational Wave Astronomy in the Asian Region

Vaishali Adya, Matthew Bailes, Carl Blair, David Blair, Johannes Eichholz, Joris van Heijningen, Eric Howell, Li Ju, Paul Lasky, Andrew Melatos, David Ottaway, Chunnong Zhao

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Abstract

The current gravitational wave detectors have identified a surprising population of heavy stellar mass black holes, and an even larger population of coalescing neutron stars. The first observations have led to many dramatic discoveries and the confirmation of general relativity in very strong gravitational fields. The future of gravitational wave astronomy looks bright, especially if additional detectors with greater sensitivity, broader bandwidth, and better global coverage can be implemented. The first discoveries add impetus to gravitational wave detectors designed to detect in the nHz, mHz and kHz frequency bands. This paper reviews the century-long struggle that led to the recent discoveries, and reports on designs and possibilities for future detectors. The benefits of future detectors in the Asian region are discussed, including analysis of the benefits of a detector located in Australia.
Original languageUndefined/Unknown
Specialist publicationarXiv preprint
Publication statusPublished - 7 Feb 2020

Cite this

Adya, V., Bailes, M., Blair, C., Blair, D., Eichholz, J., Heijningen, J. V., Howell, E., Ju, L., Lasky, P., Melatos, A., Ottaway, D., & Zhao, C. (2020). Ground Based Gravitational Wave Astronomy in the Asian Region. arXiv preprint.