Freise, A., Hild, S., Somiya, K., Strain, K.A. , Viceré, A., Barsuglia, M. and Chelkowski, S. (2010) Optical detector topology for third-generation gravitational wave observatories. General Relativity and Gravitation, 43(2), pp. 537-567. (doi: 10.1007/s10714-010-1018-0)
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Publisher's URL: http://dx.doi.org/10.1007/s10714-010-1018-0
Abstract
The third generation of gravitational wave observatories, with the aim of providing 100 times better sensitivity than currently operating interferometers, is expected to establish the evolving field of gravitational wave astronomy. A key element, required to achieve this ambitious sensitivity goal, is the exploration of new interferometer geometries, topologies and configurations. In this article we review the current status of the ongoing design work for third-generation gravitational wave observatories. The main focus is the evaluation of the detector geometry and detector topology. In addition we discuss some promising detector configurations and potential noise reduction schemes.
| Item Type: | Articles |
|---|---|
| Status: | Published |
| Refereed: | Yes |
| Glasgow Author(s) Enlighten ID: | Hild, Professor Stefan and Strain, Professor Kenneth |
| Authors: | Freise, A., Hild, S., Somiya, K., Strain, K.A., Viceré, A., Barsuglia, M., and Chelkowski, S. |
| Subjects: | Q Science > QC Physics |
| College/School: | College of Science and Engineering > School of Physics and Astronomy |
| Research Centre: | College of Science and Engineering > School of Physics and Astronomy > Institute for Gravitational Research |
| Journal Name: | General Relativity and Gravitation |
| Publisher: | Springer New York LLC |
| ISSN: | 0001-7701 |
| ISSN (Online): | 1572-9532 |
| Published Online: | 08 June 2010 |
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