Exploring the sensitivity of next generation gravitational wave detectors
- Submitting institution
-
Cardiff University / Prifysgol Caerdydd
- Unit of assessment
- 9 - Physics
- Output identifier
- 108994546
- Type
- D - Journal article
- DOI
-
10.1088/1361-6382/aa51f4
- Title of journal
- Classical and Quantum Gravity
- Article number
- 044001
- First page
- -
- Volume
- 34
- Issue
- 4
- ISSN
- 0264-9381
- Open access status
- Compliant
- Month of publication
- January
- Year of publication
- 2017
- URL
-
http://dx.doi.org/10.1088/1361-6382/aa51f4
- Supplementary information
-
-
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- No
- Number of additional authors
-
721
- Research group(s)
-
G - Gravitational Physics
- Citation count
- 329
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
-
- Author contribution statement
- I led the development of the science case for Cosmic Explorer, the US concept for the next generation of gravitational-wave detectors, described in this paper. In particular, Section III, which describes observing compact binary merger signals from high redshift and the corresponding scientific targets, grew out of my investigations and refers to my work. I was chair of the Astrophysics Working Group of the Einstein Telescope Design Study that also helped develop the science case for the Cosmic Explorer project and contributed many of the results quoted here.
- Non-English
- No
- English abstract
- -
