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; S. Hild; J.F.J. van den Brand

doi:10.1088/0264-9381/29/12/124013

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, S. Hild, J.F.J. van den Brand

^*Corresponding author for this work

Research output: Contribution to journal › Article › Academic › peer-review

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.

Original language	English
Article number	124013
Number of pages	16
Journal	Classical and Quantum Gravity
Volume	29
Issue number	12
DOIs	https://doi.org/10.1088/0264-9381/29/12/124013
Publication status	Published - 21 Jun 2012
Externally published	Yes

Keywords

BLACK-HOLE
PHYSICS
INTERMEDIATE
BINARY

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10.1088/0264-9381/29/12/124013

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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., ... van den Brand, J. F. J. (2012). Scientific objectives of Einstein Telescope. Classical and Quantum Gravity, 29(12), Article 124013. https://doi.org/10.1088/0264-9381/29/12/124013

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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.",

keywords = "BLACK-HOLE, PHYSICS, INTERMEDIATE, BINARY",

author = "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 S. Bose and L. Bosi and S. Braccini and C. Bradaschia and M. Britzger and F. Brueckner and T. Bulik and H.J. Bulten 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 \{Di Cintio\}, A. and J. Clark and E. Coccia and C.N. Colacino and J. Colas and A. Colla and A. Corsi and A. Cumming and L. Cunningham and E. Cuoco and S. Danilishin and K. Danzmann and S. Hild and \{van den Brand\}, J.F.J.",

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doi = "10.1088/0264-9381/29/12/124013",

language = "English",

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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, HJ, 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, CN, Colas, J, Colla, A, Corsi, A, Cumming, A, Cunningham, L, Cuoco, E, Danilishin, S, Danzmann, K, Hild, S & van den Brand, JFJ 2012, 'Scientific objectives of Einstein Telescope', Classical and Quantum Gravity, vol. 29, no. 12, 124013. https://doi.org/10.1088/0264-9381/29/12/124013

TY - JOUR

T1 - Scientific objectives of Einstein Telescope

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 - Bose, S.

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 - Di Cintio, A.

AU - Clark, J.

AU - Coccia, E.

AU - Colacino, C.N.

AU - Colas, J.

AU - Colla, A.

AU - Corsi, A.

AU - Cumming, A.

AU - Cunningham, L.

AU - Cuoco, E.

AU - Danilishin, S.

AU - Danzmann, K.

AU - Hild, S.

AU - van den Brand, J.F.J.

PY - 2012/6/21

Y1 - 2012/6/21

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 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.

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 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.

KW - BLACK-HOLE

KW - PHYSICS

KW - INTERMEDIATE

KW - BINARY

U2 - 10.1088/0264-9381/29/12/124013

DO - 10.1088/0264-9381/29/12/124013

M3 - Article

SN - 0264-9381

VL - 29

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 12

M1 - 124013

ER -

Scientific objectives of Einstein Telescope

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Keywords

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