Title
Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
Document Type
Article
Publication Date
1-24-2017
Abstract
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.
DOI
10.1088/1361-6382/aa51f4
MSU Digital Commons Citation
Abbott, B. P.; Abbott, R.; Abbott, T. D.; Abernathy, M. R.; Ackley, K.; Adams, C.; Addesso, P.; Adhikari, R. X.; Adya, V. B.; Affeldt, C.; Aggarwal, N.; Aguiar, O. D.; Ain, A.; Ajith, P.; Allen, B.; Altin, P. A.; Anderson, S. B.; Anderson, W. G.; Arai, K.; Araya, M. C.; Arceneaux, C. C.; Areeda, J. S.; Arun, K. G.; Ashton, G.; Ast, M.; Aston, S. M.; Aufmuth, P.; Aulbert, C.; Babak, S.; and Baker, P. T., "Exploring the Sensitivity of Next Generation Gravitational Wave Detectors" (2017). Department of Physics and Astronomy Faculty Scholarship and Creative Works. 50.
https://digitalcommons.montclair.edu/physics-astron-facpubs/50