Scientific objectives of Einstein Telescope

Sathyaprakash, B.; Abernathy, M.; Acernese, F.; Ajith, P.; Allen, B.; Amaro-Seoane, P.; Andersson, N.; Aoudia, S.; Arun, K.; Astone, P.; Krishnan, B.; Barack, L.; Barone, F.; Barr, B.; Barsuglia, M.; Bassan, M.; Bassiri, R.; Beker, M.; Beveridge, N.; Bizouard, M.; Bond, C.; Bose, S.; Bosi, L.; Braccini, S.; Bradaschia, C.; Britzger, M.; Brueckner, F.; Bulik, T.; Bulten, H.J.; Burmeister, O.; Calloni, E.; Campsie, P.; Carbone, L.; Cella, G.; Chalkley, E.; Chassande-Mottin, E.; Chelkowski, S.; Chincarini, A.; Di Cintio, A.; Clark, J.; Coccia, E.; Colacino, C.N.; Colas, J.; Colla, A.; Corsi, A.; Cumming, A.; Cunningham, L.; Cuoco, E.; Danilishin, S.; Danzmann, K.; Hild, S.; van den Brand, J.F.J.

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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 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

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Last time updated on 09/04/2021

This paper was published in Maastricht University Research Portal.

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