Document Type
Article
Publication Date
6-21-2012
Journal / Book Title
Classical and Quantum Gravity
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 1Hz to 10kHz, 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.
DOI
10.1088/0264-9381/29/12/124013
MSU Digital Commons Citation
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.; and Favata, Marc, "Scientific Objectives of Einstein Telescope" (2012). Department of Physics and Astronomy Faculty Scholarship and Creative Works. 104.
https://digitalcommons.montclair.edu/physics-astron-facpubs/104
Published Citation
Sathyaprakash, B., Abernathy, M., Acernese, F., Ajith, P., Allen, B., Amaro-Seoane, P., ... & Palomba, C. (2012). Scientific objectives of Einstein telescope. Classical and Quantum Gravity, 29(12), 124013.