Details
Original language | Undefined/Unknown |
---|---|
Title of host publication | - |
Place of Publication | Cardiff University |
Publisher | American Institute of Physics |
Volume | 29 |
Publication status | Published - 2012 |
Abstract
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-. Vol. 29 Cardiff University: American Institute of Physics, 2012.
Research output: Chapter in book/report/conference proceeding › Conference contribution › Research › peer review
}
TY - GEN
T1 - Scientific Objectives of Einstein Telescope
AU - Einstein Telescope Collaboration
AU - Sathyaprakash, B.
AU - Abernathy, M.
AU - Acernese, F.
AU - Ajith, P.
AU - Allen, B.
AU - Amaro-Seoane, P.
AU - Andersson, N.
AU - Aoudia, S.
AU - Arun, K.
AU - Astone, P.
AU - Krishnan, B.
AU - Barack, L.
AU - Barone, F.
AU - Barr, B.
AU - Barsuglia, M.
AU - Bassan, M.
AU - Bassiri, R.
AU - Beker, M.
AU - Beveridge, N.
AU - Bizouard, M.
AU - Bond, C.
AU - Bosi, L.
AU - Braccini, S.
AU - Bradaschia, C.
AU - Britzger, M.
AU - Brueckner, F.
AU - Bulik, T.
AU - Bulten, H. J.
AU - Burmeister, O.
AU - Calloni, E.
AU - Campsie, P.
AU - Carbone, L.
AU - Cella, G.
AU - Chalkley, E.
AU - Chassande-Mottin, E.
AU - Chelkowski, S.
AU - Chincarini, A.
AU - Cintio, A. Di.
AU - Clark, J.
AU - Coccia, E.
AU - Danilishin, S.
AU - Danzmann, K.
AU - Kawazoe, F.
AU - Lück, H.
AU - Schmidt, P.
AU - Vahlbruch, H.
AU - Willke, B.
AU - Yamamoto, K.
PY - 2012
Y1 - 2012
N2 - 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.
AB - 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.
U2 - 10.1088/0264-9381/29/12/124013
DO - 10.1088/0264-9381/29/12/124013
M3 - Aufsatz in Konferenzband
VL - 29
BT - -
PB - American Institute of Physics
CY - Cardiff University
ER -