The Einstein Telescope: a third-generation gravitational wave observatory
M Punturo
(1, 2)
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M Abernathy
(3)
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F Acernese
(4, 5)
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B Allen
(6)
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N Andersson
(7)
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K Arun
(8)
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F Barone
(4, 5)
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B Barr
(3)
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M. Barsuglia
(9)
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M Beker
(10)
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N Beveridge
(3)
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S Birindelli
(11)
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S Bose
(12)
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L Bosi
(1)
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S Braccini
(13)
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C Bradaschia
(13)
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T Bulik
(14)
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E Calloni
(4, 15)
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G Cella
(13)
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E Chassande Mottin
(9)
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S Chelkowski
(16)
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A Chincarini
(17)
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J Clark
(18)
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E Coccia
(4, 19)
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C Colacino
(13)
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J Colas
(2)
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A Cumming
(3)
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L Cunningham
(3)
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E Cuoco
(2)
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S Danilishin
(20)
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K Danzmann
(6)
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G de Luca
(21)
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R de Salvo
(22)
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T Dent
(18)
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R de Rosa
(4, 15)
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L Di Fiore
(4, 15)
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a Di Virgilio
(13)
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M Doets
(10)
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V Fafone
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P Falferi
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R Flaminio
(24)
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J Franc
(24)
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F Frasconi
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A Freise
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P Fulda
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J Gair
(25)
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G Gemme
(17)
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A Gennai
(16)
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A Giazotto
(2, 13)
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K Glampedakis
(26)
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M Granata
(9)
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H Grote
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G Guidi
(4, 27)
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G Hammond
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M Hannam
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J Harms
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D Heinert
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M Hendry
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I Heng
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E Hennes
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S Hild
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J Hough
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S Husa
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S Huttner
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G Jones
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F Khalili
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K Kokeyama
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K Kokkotas
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B Krishnan
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M Lorenzini
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H Uck
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E Majorana
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I Mandel
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V Mandic
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I Martin
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C Michel
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Y Minenkov
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N Morgado
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S Mosca
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B Mours
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H Uller-Ebhardt
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P Murray
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R Nawrodt
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J Nelson
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R Oshaughnessy
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C D Ott
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C Palomba
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A Paoli
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G Parguez
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A Pasqualetti
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R Passaquieti
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D Passuello
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L Pinard
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R Poggiani
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P Popolizio
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M Prato
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P Puppo
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D Rabeling
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P Rapagnani
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J Read
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T Regimbau
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H Rehbein
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S Reid
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L Rezzolla
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F Ricci
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F Richard
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A Rocchi
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S Rowan
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A Udiger
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B Sassolas
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B Sathyaprakash
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R Schnabel
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C Schwarz
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P Seidel
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A Sintes
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K Somiya
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F Speirits
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K Strain
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S Strigin
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P Sutton
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S Tarabrin
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a T Uring
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J van den Brand
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C van Leewen
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M van Veggel
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C van den Broeck
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A Vecchio
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J Veitch
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F Vetrano
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A Vicere
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S Vyatchanin
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B Willke
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G Woan
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P Wolfango
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K Yamamoto
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1
INFN
2 European Gravitational Observatory ( EGO )
3 Department of Physics and Astronomy
4 INFN
5 UNISA - Università degli Studi di Salerno = University of Salerno
6 AEI - Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut )
7 University of Southampton
8 LAL - Laboratoire de l'Accélérateur Linéaire
9 APC (UMR_7164) - AstroParticule et Cosmologie
10 VU - Vrije Universiteit Amsterdam [Amsterdam]
11 OCA - Observatoire de la Côte d'Azur
12 University of Washington [Seattle]
13 INFN - Istituto Nazionale di Fisica Nucleare [Pisa]
14 Astronomical Observatory [Warsaw]
15 Complesso Universitario di Monte S. Angelo
16 University of Birmingham [Birmingham]
17 INFN
18 Cardiff University
19 Università di Roma Tor
20 Moscow State University
21 LNGS - Laboratori Nazionali del Gran Sasso
22 LIGO
23 IFN - CNR Istituto di Fotonica e Nanotecnologie [Trento]
24 LMA - Laboratoire des matériaux avancés
25 CAM - University of Cambridge [UK]
26 Theoretical Astrophysics ( TAT )
27 Università degli Studi di Urbino 'Carlo Bo'
28 Department of Physics
29 UMN - University of Minnesota [Twin Cities]
30 Friedrich-Schiller-Universität = Friedrich Schiller University Jena [Jena, Germany]
31 Department of Physics and Astronomy [Evanston]
32 NSF Astronomy and Astrophysics Postdoctoral Fellow
33 LAPP - Laboratoire d'Annecy de Physique des Particules
34 Penn State - Pennsylvania State University
35 CALTECH - California Institute of Technology
36 University of Pisa - Università di Pisa
37 UNIROMA - Università degli Studi di Roma "La Sapienza" = Sapienza University [Rome]
38 ROMA TRE - Università degli Studi Roma Tre = Roma Tre University
39 UniFI - Università degli Studi di Firenze = University of Florence = Université de Florence
2 European Gravitational Observatory ( EGO )
3 Department of Physics and Astronomy
4 INFN
5 UNISA - Università degli Studi di Salerno = University of Salerno
6 AEI - Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut )
7 University of Southampton
8 LAL - Laboratoire de l'Accélérateur Linéaire
9 APC (UMR_7164) - AstroParticule et Cosmologie
10 VU - Vrije Universiteit Amsterdam [Amsterdam]
11 OCA - Observatoire de la Côte d'Azur
12 University of Washington [Seattle]
13 INFN - Istituto Nazionale di Fisica Nucleare [Pisa]
14 Astronomical Observatory [Warsaw]
15 Complesso Universitario di Monte S. Angelo
16 University of Birmingham [Birmingham]
17 INFN
18 Cardiff University
19 Università di Roma Tor
20 Moscow State University
21 LNGS - Laboratori Nazionali del Gran Sasso
22 LIGO
23 IFN - CNR Istituto di Fotonica e Nanotecnologie [Trento]
24 LMA - Laboratoire des matériaux avancés
25 CAM - University of Cambridge [UK]
26 Theoretical Astrophysics ( TAT )
27 Università degli Studi di Urbino 'Carlo Bo'
28 Department of Physics
29 UMN - University of Minnesota [Twin Cities]
30 Friedrich-Schiller-Universität = Friedrich Schiller University Jena [Jena, Germany]
31 Department of Physics and Astronomy [Evanston]
32 NSF Astronomy and Astrophysics Postdoctoral Fellow
33 LAPP - Laboratoire d'Annecy de Physique des Particules
34 Penn State - Pennsylvania State University
35 CALTECH - California Institute of Technology
36 University of Pisa - Università di Pisa
37 UNIROMA - Università degli Studi di Roma "La Sapienza" = Sapienza University [Rome]
38 ROMA TRE - Università degli Studi Roma Tre = Roma Tre University
39 UniFI - Università degli Studi di Firenze = University of Florence = Université de Florence
M. Barsuglia
- Fonction : Auteur
- PersonId : 1190326
- ORCID : 0000-0002-1180-4050
- IdRef : 161683487
E Chassande Mottin
- Fonction : Auteur
- PersonId : 180733
- IdHAL : eric-chassande-mottin
- ORCID : 0000-0003-3768-9908
- IdRef : 156517531
J Harms
- Fonction : Auteur
- PersonId : 764148
- ORCID : 0000-0002-7332-9806
T Regimbau
- Fonction : Auteur
- PersonId : 1198
- IdHAL : tania-regimbau
- ORCID : 0000-0002-0631-1198
- IdRef : 074147722
Résumé
Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational wave astronomy, a further substantial improvement in sensitivity is required. The future space-based Laser Interferometer Space Antenna and the third-generation ground-based observatory Einstein Telescope (ET) promise to achieve the required sensitivity improvements in frequency ranges. The vastly improv ed sensitivity of the third generation of gravitational wave observatories could permit detailed measurements of the sources' physical parameters and could complement, in a multi-messenger approach, the observation of signals emitted by cosmological sourc es obtained through other kinds of telescopes. This paper describes the progress of the ET project which is currently in its design study phase
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