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arXiv · 1206.0331

Scientific Objectives of Einstein Telescope

B. Sathyaprakash·M. Abernathy·F. Acernese·P. Ajith·B. Allen·P. Amaro-Seoane·N. Andersson·S. Aoudia·K. Arun·P. Astone·B. Krishnan·L. Barack·F. Barone·B. Barr·M. Barsuglia·M. Bassan·R. Bassiri·M. Beker·N. Beveridge·M. Bizouard·C. Bond·S. Bose·L. Bosi·S. Braccini·C. Bradaschia·M. Britzger·F. Brueckner·T. Bulik·H. J. Bulten·O. Burmeister·E. Calloni·P. Campsie·L. Carbone·G. Cella·E. Chalkley·E. Chassande-Mottin·S. Chelkowski·A. Chincarini·A. Di. Cintio·J. Clark·E. Coccia·C. N. Colacino·J. Colas·A. Colla·A. Corsi·A. Cumming·L. Cunningham·E. Cuoco·S. Danilishin·K. Danzmann·E. Daw·R. De. Salvo·W. Del. Pozzo·T. Dent·R. De. Rosa·L. Di. Fiore·M. Di. Paolo. Emilio·A. Di. Virgilio·A. Dietz·M. Doets·J. Dueck·M. Edwards·V. Fafone·S. Fairhurst·P. Falferi·M. Favata·V. Ferrari·F. Ferrini·F. Fidecaro·R. Flaminio·J. Franc·F. Frasconi·A. Freise·D. Friedrich·P. Fulda·J. Gair·M. Galimberti·G. Gemme·E. Genin·A. Gennai·A. Giazotto·K. Glampedakis·S. Gossan·R. Gouaty·C. Graef·W. Graham·M. Granata·H. Grote·G. Guidi·J. Hallam·G. Hammond·M. Hannam·J. Harms·K. Haughian·I. Hawke·D. Heinert·M. Hendry·I. Heng·E. Hennes·S. Hild
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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-10 kHz, with sensitivity a factor ten 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.

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B. Sathyaprakash, M. Abernathy, F. Acernese, P. Ajith, B. Allen, P. Amaro-Seoane, N. Andersson, S. Aoudia, K. Arun, P. Astone, B. Krishnan, L. Barack, F. Barone, B. Barr, M. Barsuglia, M. Bassan, R. Bassiri, M. Beker, N. Beveridge, M. Bizouard, C. Bond, S. Bose, L. Bosi, S. Braccini, C. Bradaschia, M. Britzger, F. Brueckner, T. Bulik, H. J. Bulten, O. Burmeister, E. Calloni, P. Campsie, L. Carbone, G. Cella, E. Chalkley, E. Chassande-Mottin, S. Chelkowski, A. Chincarini, A. Di. Cintio, J. Clark, E. Coccia, C. N. Colacino, J. Colas, A. Colla, A. Corsi, A. Cumming, L. Cunningham, E. Cuoco, S. Danilishin, K. Danzmann, E. Daw, R. De. Salvo, W. Del. Pozzo, T. Dent, R. De. Rosa, L. Di. Fiore, M. Di. Paolo. Emilio, A. Di. Virgilio, A. Dietz, M. Doets, J. Dueck, M. Edwards, V. Fafone, S. Fairhurst, P. Falferi, M. Favata, V. Ferrari, F. Ferrini, F. Fidecaro, R. Flaminio, J. Franc, F. Frasconi, A. Freise, D. Friedrich, P. Fulda, J. Gair, M. Galimberti, G. Gemme, E. Genin, A. Gennai, A. Giazotto, K. Glampedakis, S. Gossan, R. Gouaty, C. Graef, W. Graham, M. Granata, H. Grote, G. Guidi, J. Hallam, G. Hammond, M. Hannam, J. Harms, K. Haughian, I. Hawke, D. Heinert, M. Hendry, I. Heng, E. Hennes, S. Hild. 2012-06-02. Scientific Objectives of Einstein Telescope. https://doi.org/10.1088/0264-9381/29/12/124013

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