The third generation of gravitational wave observatories and their science reach
M Punturo
(1, 2)
,
M Abernathy
(3)
,
F Acernese
(4)
,
B Allen
(5)
,
N Andersson
(6)
,
K Arun
(7)
,
F Barone
(8)
,
B Barr
(9)
,
M. Barsuglia
(10)
,
M Beker
(11, 12)
,
N Beveridge
,
S Birindelli
,
S Bose
,
L Bosi
(13)
,
S Braccini
(14)
,
C Bradaschia
(14)
,
T Bulik
,
E Calloni
(8)
,
G Cella
(14)
,
E Chassande-Mottin
(10)
,
S Chelkowski
,
A Chincarini
(15)
,
J Clark
(16)
,
E Coccia
(17)
,
C Colacino
(14)
,
J Colas
(1)
,
A Cumming
(9)
,
L Cunningham
(9)
,
E Cuoco
(1)
,
S Danilishin
(18)
,
K Danzmann
(5)
,
G de Luca
(19)
,
R de Salvo
,
T Dent
(16)
,
R Derosa
(8)
,
L Di Fiore
,
A Di Virgilio
,
M Doets
(11, 12)
,
V Fafone
(17)
,
P Falferi
(20)
,
R Flaminio
(21)
,
J Franc
(21)
,
F Frasconi
(14)
,
A Freise
,
P Fulda
,
J Gair
(22)
,
G Gemme
(15)
,
A Gennai
,
A Giazotto
(14, 1)
,
K Glampedakis
(23)
,
M Granata
(10)
,
H Grote
(5)
,
G Guidi
(17)
,
G Hammond
(9)
,
M Hannam
(24)
,
J Harms
(25)
,
D Heinert
,
M Hendry
(9)
,
I Heng
(9)
,
E Hennes
(11, 12)
,
S Hild
(9)
,
J Hough
(9)
,
S Husa
(5)
,
S Huttner
(9)
,
G Jones
(16)
,
F Khalili
(18)
,
K Kokeyama
,
K Kokkotas
(23)
,
B Krishnan
(5)
,
M Lorenzini
(17)
,
H Uck
(5)
,
E Majorana
(26)
,
I Mandel
(27)
,
V Mandic
(25)
,
I Martin
(9)
,
C Michel
(21)
,
Y Minenkov
(17)
,
N Morgado
(21)
,
S Mosca
(8)
,
B Mours
(28)
,
H Müller-Ebhardt
(5)
,
P Murray
(9)
,
R Nawrodt
(9)
,
J Nelson
(9)
,
R Oshaughnessy
(29)
,
C D Ott
(30)
,
C Palomba
(26)
,
A Paoli
(1)
,
G Parguez
(1)
,
A Pasqualetti
(1)
,
R Passaquieti
(14)
,
D Passuello
(14)
,
L Pinard
(21)
,
R Poggiani
(14)
,
P Popolizio
(1)
,
M Prato
(15)
,
P Puppo
(26)
,
D Rabeling
(11, 31, 12)
,
P Rapagnani
(26)
,
J Read
(5)
,
T Regimbau
,
H Rehbein
(5)
,
S Reid
(9)
,
L Rezzolla
(5)
,
F Ricci
(26)
,
F Richard
(1)
,
A Rocchi
(17)
,
S Rowan
(9)
,
A Rüdiger
(5)
,
B Sassolas
(21)
,
B Sathyaprakash
(16)
,
R Schnabel
(5)
,
C Schwarz
,
P Seidel
,
A Sintes
(5)
,
K Somiya
(30)
,
F Speirits
(9)
,
K Strain
(9)
,
S Strigin
(18)
,
P Sutton
(16)
,
S Tarabrin
(18)
,
J van den Brand
(11, 12)
,
C van Leewen
(11, 12)
,
M van Veggel
(9)
,
C van den Broeck
(16)
,
A Vecchio
,
J Veitch
,
F Vetrano
(17)
,
A Vicere
(17)
,
S Vyatchanin
(18)
,
B Willke
(5)
,
G Woan
(9)
,
P Wolfango
(26)
,
K Yamamoto
(5)
1
EGO -
European gravitational Observatory
2 INFN, Sezione di Perugia - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
3 University of Glasgow
4 INFN, Sezione di Napoli - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
5 AEI - Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut )
6 University of Southampton
7 LAL - Laboratoire de l'Accélérateur Linéaire
8 Sezione di Napoli a
9 Department of Physics and Astronomy
10 APC (UMR_7164) - AstroParticule et Cosmologie
11 VU - Vrije Universiteit Amsterdam [Amsterdam]
12 University of Washington [Seattle]
13 INFN
14 University of Birmingham [Birmingham]
15 INFN
16 Cardiff University
17 INFN
18 Moscow State University
19 CALTECH - California Institute of Technology
20 IFN - CNR Istituto di Fotonica e Nanotecnologie [Trento]
21 LMA - Laboratoire des matériaux avancés
22 CAM - University of Cambridge [UK]
23 Theoretical Astrophysics ( TAT )
24 Department of Physics
25 UMN - University of Minnesota System
26 INFN - Istituto Nazionale di Fisica Nucleare [Sezione di Roma 1]
27 Department of Physics and Astronomy [Evanston]
28 LAPP - Laboratoire d'Annecy de Physique des Particules
29 Penn State - Pennsylvania State University
30 Caltech-CaRT
31 CNRS - Centre National de la Recherche Scientifique
2 INFN, Sezione di Perugia - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
3 University of Glasgow
4 INFN, Sezione di Napoli - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
5 AEI - Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut )
6 University of Southampton
7 LAL - Laboratoire de l'Accélérateur Linéaire
8 Sezione di Napoli a
9 Department of Physics and Astronomy
10 APC (UMR_7164) - AstroParticule et Cosmologie
11 VU - Vrije Universiteit Amsterdam [Amsterdam]
12 University of Washington [Seattle]
13 INFN
14 University of Birmingham [Birmingham]
15 INFN
16 Cardiff University
17 INFN
18 Moscow State University
19 CALTECH - California Institute of Technology
20 IFN - CNR Istituto di Fotonica e Nanotecnologie [Trento]
21 LMA - Laboratoire des matériaux avancés
22 CAM - University of Cambridge [UK]
23 Theoretical Astrophysics ( TAT )
24 Department of Physics
25 UMN - University of Minnesota System
26 INFN - Istituto Nazionale di Fisica Nucleare [Sezione di Roma 1]
27 Department of Physics and Astronomy [Evanston]
28 LAPP - Laboratoire d'Annecy de Physique des Particules
29 Penn State - Pennsylvania State University
30 Caltech-CaRT
31 CNRS - Centre National de la Recherche Scientifique
M. Barsuglia
- Fonction : Auteur
- PersonId : 1190326
- ORCID : 0000-0002-1180-4050
- IdRef : 161683487
N Beveridge
- Fonction : Auteur
S Birindelli
- Fonction : Auteur
S Bose
- Fonction : Auteur
T Bulik
- Fonction : Auteur
E Chassande-Mottin
- Fonction : Auteur
- PersonId : 180733
- IdHAL : eric-chassande-mottin
- ORCID : 0000-0003-3768-9908
- IdRef : 156517531
S Chelkowski
- Fonction : Auteur
R de Salvo
- Fonction : Auteur
L Di Fiore
- Fonction : Auteur
A Di Virgilio
- Fonction : Auteur
A Freise
- Fonction : Auteur
P Fulda
- Fonction : Auteur
A Gennai
- Fonction : Auteur
J Harms
- Fonction : Auteur
- PersonId : 764148
- ORCID : 0000-0002-7332-9806
D Heinert
- Fonction : Auteur
K Kokeyama
- Fonction : Auteur
T Regimbau
- Fonction : Auteur
- PersonId : 1198
- IdHAL : tania-regimbau
- ORCID : 0000-0002-0631-1198
- IdRef : 074147722
C Schwarz
- Fonction : Auteur
P Seidel
- Fonction : Auteur
A Vecchio
- Fonction : Auteur
J Veitch
- Fonction : Auteur
Résumé
Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third generation observatories in more than one decade will open the possibility to perform gravitational wave astronomical observations from the Earth. An overview of the possible science reaches and the technological progress needed to realise a third generation observatory are discussed in this paper. The status of the project Einstein Telescope (ET), a design study of a third generation gravitational wave observatory, will be reported.
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