arXiv · 1905.02842
Astrophysical science metrics for next-generation gravitational-wave detectors
Abstract
The second generation of gravitational-wave detectors are being built and tuned all over the world. The detection of signals from binary black holes is beginning to fulfill the promise of gravitational-wave astronomy. In this work, we examine several possible configurations for third-generation laser interferometers in existing km-scale facilities. We propose a set of astrophysically motivated metrics to evaluate detector performance. We measure the impact of detector design choices against these metrics, providing a quantitative cost-benefit analyses of the resulting scientific payoffs.
Explore related subjects
Keep this discovery
Rana X Adhikari, P Ajith, Yanbei Chen, James A Clark, Vladimir Dergachev, Nicolas V Fotopoulos, Sarah E. Gossan, Ilya Mandel, Maria Okounkova, Vivien Raymond, Jocelyn S Read. 2019-05-07. Astrophysical science metrics for next-generation gravitational-wave detectors. https://doi.org/10.1088/1361-6382%2Fab3cff
Cite the original work for its findings. Save a collection to share your selection of sources.