Scientific objectives of Einstein telescope
| dc.contributor.author | Sathyaprakash, B S | |
| dc.contributor.author | Abernathy, M R | |
| dc.contributor.author | Acernese, F | |
| dc.contributor.author | Ajith, P | |
| dc.contributor.author | Mishra, Chandrakanth | |
| dc.contributor.author | +150 Co-authors | |
| dc.contributor.author | Iyer, B.R. | |
| dc.date.accessioned | 2012-07-23T09:07:35Z | |
| dc.date.available | 2012-07-23T09:07:35Z | |
| dc.date.issued | 2012-06-21 | |
| dc.description | Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations) | en |
| dc.description.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. | en |
| dc.identifier.citation | Classical and Quantum Gravity, 2012, Vol.29, p124013 | en |
| dc.identifier.issn | 0264-9381 | |
| dc.identifier.issn | 1361-6382 (Online) | |
| dc.identifier.uri | http://hdl.handle.net/2289/5086 | |
| dc.language.iso | en | en |
| dc.publisher | IOP Publishing Ltd. | en |
| dc.relation.uri | http://arxiv.org/abs/1206.0331 | en |
| dc.relation.uri | http://dx.doi.org/10.1088/0264-9381/29/12/124013 | en |
| dc.relation.uri | http://adsabs.harvard.edu/abs/2012CQGra..29l4013S | en |
| dc.rights | 2012 IOP Publishing Ltd. | en |
| dc.subject | Instrumentation and measurement | en |
| dc.subject | Gravitation and cosmology | en |
| dc.title | Scientific objectives of Einstein telescope | en |
| dc.type | Article | en |

