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Scientific Objectives of Einstein Telescope

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  • Einstein Telescope Collaboration

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Original languageUndefined/Unknown
Title of host publication-
Place of PublicationCardiff University
PublisherAmerican Institute of Physics
Volume29
Publication statusPublished - 2012

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.

Cite this

Scientific Objectives of Einstein Telescope. / Einstein Telescope Collaboration.
-. Vol. 29 Cardiff University: American Institute of Physics, 2012.

Research output: Chapter in book/report/conference proceeding › Conference contribution › Research › peer review

Einstein Telescope Collaboration 2012, Scientific Objectives of Einstein Telescope. in -. vol. 29, American Institute of Physics, Cardiff University. https://doi.org/10.1088/0264-9381/29/12/124013
Einstein Telescope Collaboration (2012). Scientific Objectives of Einstein Telescope. In - (Vol. 29). American Institute of Physics. https://doi.org/10.1088/0264-9381/29/12/124013
Einstein Telescope Collaboration. Scientific Objectives of Einstein Telescope. In -. Vol. 29. Cardiff University: American Institute of Physics. 2012 doi: 10.1088/0264-9381/29/12/124013
Einstein Telescope Collaboration. / Scientific Objectives of Einstein Telescope. -. Vol. 29 Cardiff University : American Institute of Physics, 2012.
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title = "Scientific Objectives of Einstein Telescope",
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.",
author = "{Einstein Telescope Collaboration} and B. Sathyaprakash and M. Abernathy and F. Acernese and P. Ajith and B. Allen and P. Amaro-Seoane and N. Andersson and S. Aoudia and K. Arun and P. Astone and B. Krishnan and L. Barack and F. Barone and B. Barr and M. Barsuglia and M. Bassan and R. Bassiri and M. Beker and N. Beveridge and M. Bizouard and C. Bond and L. Bosi and S. Braccini and C. Bradaschia and M. Britzger and F. Brueckner and T. Bulik and Bulten, {H. J.} and O. Burmeister and E. Calloni and P. Campsie and L. Carbone and G. Cella and E. Chalkley and E. Chassande-Mottin and S. Chelkowski and A. Chincarini and Cintio, {A. Di.} and J. Clark and E. Coccia and S. Danilishin and K. Danzmann and F. Kawazoe and H. L{\"u}ck and P. Schmidt and H. Vahlbruch and B. Willke and K. Yamamoto",
year = "2012",
doi = "10.1088/0264-9381/29/12/124013",
language = "Undefined/Unknown",
volume = "29",
booktitle = "-",
publisher = "American Institute of Physics",
address = "United States",

}

Download

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 -