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논문

Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

https://doi.org/10.1088/1361-6382/aa51f4

  • 저자B.P. Abbott, R. Abbott, ....J.J.Oh, S.H.Oh, E.J.Son,..
  • 학술지Classical and Quantum Gravity 34
  • 등재유형
  • 게재일자(2017)

The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.

The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.

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