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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5086
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dc.contributor.authorSathyaprakash, B.S.-
dc.contributor.authorAbernathy, M.-
dc.contributor.authorAcernese, F-
dc.contributor.authorAjith, P.-
dc.contributor.authorMishra, Chandrakanth-
dc.contributor.author+150 Co-authors-
dc.contributor.authorIyer, B.R.-
dc.date.accessioned2012-07-23T09:07:35Z-
dc.date.available2012-07-23T09:07:35Z-
dc.date.issued2012-06-21-
dc.identifier.citationClassical and Quantum Gravity, 2012, Vol.29, p124013en
dc.identifier.issn0264-9381-
dc.identifier.issn1361-6382 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/5086-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractThe 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.language.isoenen
dc.publisherIOP Publishing Ltd.en
dc.relation.urihttp://arxiv.org/abs/1206.0331en
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/29/12/124013en
dc.relation.urihttp://adsabs.harvard.edu/abs/2012CQGra..29l4013Sen
dc.rights2012 IOP Publishing Ltd.en
dc.subjectInstrumentation and measurementen
dc.subjectGravitation and cosmologyen
dc.titleScientific objectives of Einstein telescopeen
dc.typeArticleen
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