Sathyaprakash, B. and Ajith, P. and Corsi, A. and Favata, M. and Harms, J. and Ott, C. D. and Santamaría, L. (2012) Scientific objectives of Einstein Telescope. Classical and Quantum Gravity, 29 (12). Art. No. 124013. ISSN 0264-9381. http://resolver.caltech.edu/CaltechAUTHORS:20120803-105338433
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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.
|Additional Information:||© 2012 Institute of Physics. Received 3 March 2012, in final form 8 May 2012. Published 1 June 2012. This work was supported by the European Commission under the Framework Programme 7 (FP7) ‘Capacities’, project Einstein Telescope (ET) design study (Grant Agreement 211743), http://www.et-gw.eu/. We thank Drs Asad Ali and Evan Ochsner for comments.|
|Subject Keywords:||Instrumentation and measurement; Gravitation and cosmology; Astrophysics and astroparticles|
|Classification Code:||PACS: 95.36.+x, 97.60.Lf, 98.62.Py, 04.80.Nn, 95.55.Ym, 97.60.Bw, 97.60.Jd, 07.60.Ly, 95.45.+i. MSC: 83C35|
|Official Citation:||Scientific objectives of Einstein Telescope B Sathyaprakash et al 2012 Class. Quantum Grav. 29 124013|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||03 Aug 2012 18:24|
|Last Modified:||23 Aug 2016 10:15|
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