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Research and Development for Third-Generation Gravitational Wave Detectors

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Handbook of Gravitational Wave Astronomy

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Abstract

Gravitational wave astronomy is a new and exciting field but has a long history as well as a bright future. The first detections of gravitational waves were from instruments of the second generation of detectors – the first generation of kilometer-scale ground based detectors operated as planned, but did not conclusively observe gravitational waves. The second-generation detectors (Advanced LIGO and Advanced Virgo) opened the field, and the third-generation detectors will expand our view of the gravitational wave universe to cosmic distances. This chapter will discuss the technological research and development required to build these third-generation detectors.

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Authors and Affiliations

  1. Centre for Gravitational Astrophysics, Research Schools of Physics, and of Astronomy and Astrophysics, The Australian National University, Acton, Australia

    Robert L. Ward & Bram J. J. Slagmolen

  2. Gravitational Wave Science Project, National Astronomical Observatory of Japan, Mitaka, Japan

    Yoichi Aso

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  1. Department of Physics, Fudan University, Shanghai, China

    Cosimo Bambi

  2. Université de Paris and European Gravitational Observatory, Paris, France

    Stavros Katsanevas

  3. Institute for Astronomy and Astrophysics Eberhard Karls, University of Tübingen, Tübingen, Germany

    Konstantinos D. Kokkotas

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Ward, R.L., Slagmolen, B.J.J., Aso, Y. (2022). Research and Development for Third-Generation Gravitational Wave Detectors. In: Bambi, C., Katsanevas, S., Kokkotas, K.D. (eds) Handbook of Gravitational Wave Astronomy. Springer, Singapore. https://doi.org/10.1007/978-981-16-4306-4_8

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