Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/5086| Title: | Scientific objectives of Einstein telescope |
| Authors: | Sathyaprakash, B.S. Abernathy, M. Acernese, F Ajith, P. Mishra, Chandrakanth +150 Co-authors Iyer, B.R. |
| Keywords: | Instrumentation and measurement Gravitation and cosmology |
| Issue Date: | 21-Jun-2012 |
| Publisher: | IOP Publishing Ltd. |
| Citation: | Classical and Quantum Gravity, 2012, Vol.29, p124013 |
| Abstract: | The advanced interferometer network will herald a new era in observational astronomy. There is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz to 10 kHz, with sensitivity a factor 10 better in amplitude. Such detectors will be able to probe a range of topics in nuclear physics, astronomy, cosmology and fundamental physics, providing insights into many unsolved problems in these areas. |
| Description: | Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations) |
| URI: | http://hdl.handle.net/2289/5086 |
| ISSN: | 0264-9381 1361-6382 (Online) |
| Alternative Location: | http://arxiv.org/abs/1206.0331 http://dx.doi.org/10.1088/0264-9381/29/12/124013 http://adsabs.harvard.edu/abs/2012CQGra..29l4013S |
| Copyright: | 2012 IOP Publishing Ltd. |
| Appears in Collections: | Research Papers (TP) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 2012_CQG_V29_p124013.pdf Restricted Access | Restricted Access | 2.62 MB | Adobe PDF | View/Open Request a copy |
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