Noise from scattered light in Virgo's second science run data
T Accadia
(1, 2)
,
F Acernese
(1, 3)
,
F Antonucci
(1, 3)
,
P Astone
(1, 3)
,
G Ballardin
(1, 4)
,
F Barone
(1, 3)
,
M. Barsuglia
(1, 5)
,
Th S Bauer
(1, 6)
,
M G Beker
(1, 6)
,
A Belletoile
(1, 2)
,
S Birindelli
(1, 7)
,
M Bitossi
(1, 8)
,
M A Bizouard
(1, 9)
,
M Blom
(1, 6)
,
François Bondu
(10)
,
L Bonelli
(1, 8)
,
R Bonnand
(1)
,
V Boschi
(1, 8)
,
L Bosi
(1, 3)
,
B Bouhou
(1, 5)
,
S Braccini
(1, 8)
,
C Bradaschia
(1, 8)
,
A Brillet
(1, 7)
,
V Brisson
(1, 9)
,
R Budzyski
(1)
,
T Bulik
(1)
,
H J Bulten
(1, 6)
,
D Buskulic
(1, 2)
,
Christelle Lesvigne-Buy
(1, 5)
,
G Cagnoli
(1, 3)
,
E Calloni
(1, 3)
,
E Campagna
(1, 3)
,
B Canuel
(1, 4)
,
F Carbognani
(1, 4)
,
F Cavalier
(1, 9)
,
R Cavalieri
(1, 4)
,
G Cella
(1, 8)
,
E Cesarini
(1, 3)
,
E Chassande-Mottin
(1, 5)
,
A Chincarini
(1, 3)
,
F Cleva
(1, 7)
,
E Coccia
(1, 11)
,
C N Colacino
(1, 8)
,
J Colas
(1, 4)
,
A Colla
(1, 3)
,
M Colombini
(1, 3)
,
A Corsi
(1, 3)
,
J.-P Coulon
(1, 7)
,
E Cuoco
(1, 4)
,
Antonio 9a
(1, 11)
,
V Dattilo
(1, 4)
,
M Davier
(1, 9)
,
R Day
(1, 4)
,
Rosa 5ab
(1, 3)
,
G Debreczeni
(1)
,
M Del
(1)
,
Prete 7ac
(1, 8)
,
L Di
(1)
,
Fiore 5a
(1, 3)
,
A Di
(1)
,
Lieto 7ab
(8)
,
M Di
(1)
,
Paolo Emilio
(1, 11)
,
Virgilio 7a
(8)
,
A Dietz
(1, 2)
,
M Drago
(1, 12, 13)
,
V Fafone
(1, 11)
,
I Ferrante
(1, 8)
,
F Fidecaro
(1, 8)
,
I Fiori
(1, 4)
,
R Flaminio
(1)
,
J.-D Fournier
(1, 7)
,
J Franc
(1)
,
S Frasca
(1, 3)
,
F Frasconi
(1, 8)
,
A Freise
(1, 14)
,
M Galimberti
(1)
,
L Gammaitoni
(1, 3)
,
F Garufi
(1, 3)
,
M E Gáspár
(1)
,
G Gemme
(1, 3)
,
E Genin
(1, 4)
,
A Gennai
(1, 8)
,
A Giazotto
(1, 8)
,
R Gouaty
(1, 2)
,
M Granata
(1, 5)
,
C Greverie
(1, 7)
,
G M Guidi
(1, 3)
,
J.-F Hayau
(10)
,
H Heitmann
(1, 7)
,
P Hello
(1, 9)
,
S Hild
(1, 14)
,
D Huet
(1, 4, 14)
,
P Jaranowski
(1)
,
I Kowalska
(1)
,
A Królak
(1)
,
N Leroy
(1, 9)
,
N Letendre
(1, 2)
,
T G F Li
(6)
,
M Lorenzini
(1, 3)
,
V Loriette
(1, 9)
,
G Losurdo
(1, 3)
,
E Majorana
(1, 3)
,
I Maksimovic
(1, 9)
,
N Man
(1, 7)
,
M Mantovani
(1, 8)
,
F Marchesoni
(1, 3)
,
F Marion
(1, 2)
,
J Marque
(1, 4)
,
F Martelli
(1, 3)
,
A Masserot
(1, 2)
,
C Michel
(1)
,
L Milano
(1, 3)
,
Y Minenkov
(1, 11)
,
M Mohan
(1, 4)
,
N Morgado
(1)
,
A Morgia
(1, 11)
,
S Mosca
(1, 3)
,
V Moscatelli
(1, 3)
,
B Mours
(1, 2)
,
I Neri
(1, 3)
,
F Nocera
(1, 4)
,
G Pagliaroli
(1, 11)
,
L Palladino
(1, 11)
,
C Palomba
(1, 3)
,
F Paoletti
(1, 4, 8)
,
S Pardi
(1, 3)
,
M Parisi
(1, 3)
,
A Pasqualetti
(1, 4)
,
R Passaquieti
(1, 8)
,
D Passuello
(1, 8)
,
G Persichetti
(1, 3)
,
M Pichot
(1, 7)
,
F Piergiovanni
(1, 3)
,
M Pietka
(1)
,
L Pinard
(1)
,
R Poggiani
(1, 8)
,
M Prato
(1, 3)
,
G A Prodi
(1, 12, 13)
,
M Punturo
(1, 3)
,
P Puppo
(1, 3)
,
D S Rabeling
(1, 6)
,
I Rácz
(1)
,
P Rapagnani
(1, 3)
,
V Re
(12, 13)
,
T Regimbau
(1, 7)
,
F Ricci
(1, 3)
,
F Robinet
(1, 9)
,
A Rocchi
(1, 11)
,
L Rolland
(1, 2)
,
R Romano
(1, 3)
,
D Rosiska
(1)
,
P Ruggi
(1, 4)
,
B Sassolas
(1)
,
D Sentenac
(1, 4)
,
L Sperandio
(1, 11)
,
R Sturani
(1, 3)
,
B L Swinkels
(1, 4)
,
A Toncelli
(1, 8)
,
M Tonelli
(1, 8)
,
O Torre
(1, 8)
,
E Tournefier
(1, 2)
,
F Travasso
(1, 3)
,
G Vajente
(1, 8)
,
J F J van den Brand
(1, 6)
,
S van Der Putten
(1, 6)
,
M Vasuth
(1)
,
M Vavoulidis
(1, 9)
,
G Vedovato
(1, 12, 13)
,
D Verkindt
(1, 2)
,
F Vetrano
(1, 3)
,
A Viceré
(1, 3)
,
J.-y Vinet
(1, 7)
,
H Vocca
(1, 3)
,
M Was
(1, 9)
,
M Yvert
(1, 2)
1
ESPCI Paris -
Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris
2 USMB [Université de Savoie] [Université de Chambéry] - Université Savoie Mont Blanc
3 INFN
4 EGO - European gravitational Observatory
5 IMRB - Institut Mondor de Recherche Biomédicale
6 NIKHEF - National Institute for Subatomic Physics [Amsterdam]
7 UR - Université de Rennes
8 Sezione di Pisa a
9 UP11 - Université Paris-Sud - Paris 11
10 IPR - Institut de Physique de Rennes
11 UNIVAQ - Università degli Studi dell'Aquila = University of L'Aquila
12 UNITN - Università degli Studi di Trento = University of Trento
13 Sezione di Padova c
14 University of Glasgow
2 USMB [Université de Savoie] [Université de Chambéry] - Université Savoie Mont Blanc
3 INFN
4 EGO - European gravitational Observatory
5 IMRB - Institut Mondor de Recherche Biomédicale
6 NIKHEF - National Institute for Subatomic Physics [Amsterdam]
7 UR - Université de Rennes
8 Sezione di Pisa a
9 UP11 - Université Paris-Sud - Paris 11
10 IPR - Institut de Physique de Rennes
11 UNIVAQ - Università degli Studi dell'Aquila = University of L'Aquila
12 UNITN - Università degli Studi di Trento = University of Trento
13 Sezione di Padova c
14 University of Glasgow
M. Barsuglia
- Fonction : Auteur
- PersonId : 1190326
- ORCID : 0000-0002-1180-4050
- IdRef : 161683487
François Bondu
- Fonction : Auteur
- PersonId : 772
- IdHAL : francois-bondu
- ORCID : 0000-0001-6487-5197
- IdRef : 187902461
B Bouhou
- Fonction : Auteur
- PersonId : 941023
Christelle Lesvigne-Buy
- Fonction : Auteur
- PersonId : 924454
B Canuel
- Fonction : Auteur
- PersonId : 179999
- IdHAL : benjamin-canuel
- IdRef : 11603534X
F Cavalier
- Fonction : Auteur
- PersonId : 748863
- IdHAL : fabien-cavalier
- ORCID : 0000-0002-3658-7240
E Chassande-Mottin
- Fonction : Auteur
- PersonId : 180733
- IdHAL : eric-chassande-mottin
- ORCID : 0000-0003-3768-9908
- IdRef : 156517531
N Leroy
- Fonction : Auteur
- PersonId : 738354
- IdHAL : nicolas-leroy-cnrs
- ORCID : 0000-0002-2321-1017
- IdRef : 113609736
V Loriette
- Fonction : Auteur
- PersonId : 181377
- IdHAL : vincent-loriette
- ORCID : 0000-0002-4551-2902
- IdRef : 166006521
T Regimbau
- Fonction : Auteur
- PersonId : 1198
- IdHAL : tania-regimbau
- ORCID : 0000-0002-0631-1198
- IdRef : 074147722
L Rolland
- Fonction : Auteur
- PersonId : 4321
- IdHAL : loic-rolland
- ORCID : 0000-0003-0589-9687
- IdRef : 090243080
D Verkindt
- Fonction : Auteur
- PersonId : 739957
- IdHAL : didier-verkindt
- ORCID : 0000-0003-4344-7227
- IdRef : 188902783
A Viceré
- Fonction : Auteur
- PersonId : 764147
- ORCID : 0000-0003-0624-6231
M Was
- Fonction : Auteur
- PersonId : 739657
- IdHAL : michalwas
- ORCID : 0000-0002-1890-1128
- IdRef : 153023481
Résumé
Virgo is one of the large, ground-based interferometers aimed at detecting gravitational waves. One of the technical problems limiting its sensitivity is caused by light in the output beams which is back-scattered by seismically excited surfaces and couples back into the main beam of the interferometer. The resulting noise was thoroughly studied, measured and mitigated before Virgo's second science run (VSR2). The residual noise during VSR2, which increases in periods with large microseism activity, is accurately predicted by the theoretical model. The scattered light has been associated with transient events in the gravitational-wave signal of the interferometer.
Fichier principal
PEER_stage2_10.1088%2F0264-9381%2F27%2F19%2F194011.pdf (868.45 Ko)
Télécharger le fichier
Origine | Fichiers produits par l'(les) auteur(s) |
---|
Loading...