The Advanced Virgo detector

10th International LISA Symposium

Acernese, F.^11,35 ; Adams, T.^19 ; Agathos, M.^23 ; Agatsuma, K.^23 ; Allocca, A.^14,36 ; Astone, P.^15 ; Ballardin, G.^5 ; Barone, F.^11,35 ; Barsuglia, M.^1 ; Basti, A.^14,31 ; Bauer, Th.S.^23 ; Bavigadda, V.^5 ; Bejger, M.^4 ; Belczynski, C.^3 ; Bersanetti, D.^9,28 ; Bertolini, A.^23 ; Bitossi, M.^5,14 ; Bizouard, M.A.^18 ; Bloemen, S.^23,24 ; Boer, M.^2 ; Bogaert, G.^2 ; Bondu, F.^32 ; Bonelli, L.^14,31 ; Bonnand, R.^19 ; Boschi, V.^14 ; Bosi, L.^13 ; Bradaschia, C.^14 ; Branchesi, M.^8,38 ; Briant, T.^20 ; Brillet, A.^2 ; Brisson, V.^18 ; Bulik, T.^3 ; Bulten, H.J.^23,26 ; Buskulic, D.^19 ; Buy, C.^1 ; Cagnoli, G.^21 ; Calloni, E.^11,29 ; Carbognani, F.^5 ; Cavalier, F.^18 ; Cavalieri, R.^5 ; Cella, G.^14 ; Cesarini, E.^16 ; Chassande-Mottin, E.^1 ; Chincarini, A.^9 ; Chiummo, A.^5 ; Chua, S.^20 ; Cleva, F.^2 ; Coccia, E.^10,34 ; Cohadon, P.-F.^20 ; Colla, A.^15,33 ; Colombini, M.^13 ; Conte, A.^15,33 ; Coulon, J.-P.^2 ; Cuoco, E.^5 ; D'Antonio, S.^16 ; Dattilo, V.^5 ; Davier, M.^18 ; Day, R.^5 ; Debreczeni, G.^25,39 ; Degallaix, J.^21 ; De Laurentis, M.^11,29 ; Deléglise, S.^20 ; Del Pozzo, W.^23 ; Dereli, H.^2 ; De Rosa, R.^11,29 ; Fiore, L Di^11 ; Di Lieto, A.^14,31 ; Di Virgilio, A.^14 ; Dolique, V.^21 ; Drago, M.^17,37 ; Ducrot, M.^19 ; Endroczi, G.^25,39 ; Fafone, V.^16,34 ; Farinon, S.^9 ; Ferrante, I.^14,31 ; Ferrini, F.^5 ; Fidecaro, F.^14,31 ; Fiori, I.^5 ; Flaminio, R.^21 ; Fournier, J.-D.^2 ; Franco, S.^18 ; Frasca, S.^15,33 ; Frasconi, F.^14 ; Gammaitoni, L.^13,30 ; Garufi, F.^11,29 ; Gatto, A.^1 ; Gemme, G.^9 ; Gendre, B.^2 ; Genin, E.^5 ; Gennai, A.^14 ; Ghosh, S.^23,24 ; Giazotto, A.^14 ; Gouaty, R.^19 ; Granata, M.^21 ; Greco, G.^8,38 ; Groot, P.^24 ; Guidi, G.M.^8,38 ; Harms, J.^8 ; Heidmann, A.^20 ; Heitmann, H.^2 ; Hello, P.^18 ; Hemming, G.^5 ; Hofman, D.^21 ; Jonker, R.J.G.^23 ; Kasprzack, M.^5,18 ; Kéfélian, F.^2 ; Królak, A.^7,22 ; Kutynia, A.^22 ; Lazzaro, C.^12 ; Lebigot, E.^1 ; Leonardi, M.^17,37 ; Leroy, N.^18 ; Letendre, N.^19 ; Lorenzini, M.^16,34 ; Loriette, V.^6 ; Losurdo, G.^8 ; Majorana, E.^15 ; Maksimovic, I.^6 ; Malvezzi, V.^16,34 ; Man, N.^2 ; Mangano, V.^15,33 ; Mantovani, M.^5,14 ; Marchesoni, F.^13,27 ; Marion, F.^19 ; Marque, J.^5 ; Martelli, F.^8,38 ; Martinelli, L.^2 ; Masserot, A.^19 ; Meacher, D.^2 ; Meidam, J.^23 ; Mezzani, F.^15,33 ; Michel, C.^21 ; Milano, L.^11,29 ; Minenkov, Y.^16 ; Moggi, A.^14 ; Mohan, M.^5 ; Mours, B.^19 ; Nagy, M.F.^25,39 ; Nardecchia, I.^16,34 ; Naticchioni, L.^15,33 ; Nelemans, G.^23,24 ; Neri, I.^13,30 ; Neri, M.^9,28 ; Nocera, F.^5 ; Palomba, C.^15 ; Paoletti, F.^5,14 ; Pasqualetti, A.^5 ; Passaquieti, R.^14,31 ; Passuello, D.^14 ; Pichot, M.^2 ; Piergiovanni, F.^8,38 ; Pillant, G.^5 ; Pinard, L.^21 ; Poggiani, R.^14,31 ; Prijatelj, M.^5 ; Prodi, G.A.^17,37 ; Punturo, M.^13 ; Puppo, P.^15 ; Rabeling, D.S.^23,26 ; Rácz, I.^25,39 ; Rapagnani, P.^15,33 ; Razzano, M.^14,31 ; Re, V.^16,34 ; Regimbau, T.^2 ; Ricci, F.^15,33 ; Robinet, F.^18

APC, AstroParticule et Cosmologie, Université Paris Diderot, Sorbonne Paris Cité, 10, rue Alice Domon et Leonie Duquet, Paris Cedex 13

F-75205, France^1

ARTEMIS, Université Nice-Sophia-Antipolis, Observatoire de la Côte d'Azur, Nice

F-06304, France^2

Astronomical Observatory Warsaw University, Warsaw

00-478, Poland^3

CAMK-PAN, Warsaw

00-716, Poland^4

European Gravitational Observatory (EGO), Cascina, Pisa

I-56021, Italy^5

ESPCI, CNRS, Paris

F-75005, France^6

IM-PAN, Warsaw

00-956, Poland^7

INFN, Sezione di Firenze, Sesto Fiorentino, Firenze

I-50019, Italy^8

INFN, Sezione di Genova, Genova

I-16146, Italy

(10) INFN, Gran Sasso Science Institute, L'Aquila

I-67100, Italy

(11) INFN, Sezione di Napoli, Complesso Universitario di Monte S.Angelo, Napoli

I-80126, Italy

(12) INFN, Sezione di Padova, Padova

I-35131, Italy

(13) INFN, Sezione di Perugia, Perugia

I-06123, Italy

(14) INFN, Sezione di Pisa, Pisa

I-56127, Italy

(15) INFN, Sezione di Roma, Rome

I-00185, Italy

(16) INFN, Sezione di Roma Tor Vergata, Rome

I-00133, Italy

(17) INFN, Trento Institute for Fundamental Physics and Applications, Povo, Trento

I-38123, Italy

(18) LAL, Université Paris-Sud, IN2P3/CNRS, Orsay

F-91898, France

(19) Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, Annecy-le-Vieux

F-74941, France

(20) Laboratoire Kastler Brossel, ENS, Université Pierre et Marie Curie, Paris

F-75005, France

(21) Laboratoire des Materiaux Avances (LMA), IN2P3/CNRS, Université de Lyon, Villeurbanne, Lyon

F-69622, France

(22) NCBJ, wierk-Otwock

05-400, Poland

(23) Nikhef, Science Park, Amsterdam

1098 XG, Netherlands

(24) Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, Nijmegen

6500 GL, Netherlands

(25) Wigner RCP, RMKI, Budapest

H-1121, Hungary

(26) VU University Amsterdam, Amsterdam

1081 HV, Netherlands

(27) Università di Camerino, Dipartimento di Fisica, Camerino

I-62032, Italy

(28) Università Degli Studi di Genova, Genova

I-16146, Italy

(29) Università di Napoli 'Federico II', Complesso Universitario di Monte S.Angelo, Napoli

I-80126, Italy

(30) Università di Perugia, Perugia

I-06123, Italy

(31) Università di Pisa, Pisa

I-56127, Italy

(32) Institut de Physique de Rennes, CNRS, Université de Rennes 1, Rennes

F-35042, France

(33) Università di Roma 'La Sapienza', Rome

I-00185, Italy

(34) Università di Roma Tor Vergata, Rome

I-00133, Italy

(35) Università di Salerno, Fisciano, Salerno

I-84084, Italy

(36) Università di Siena, Siena

I-53100, Italy

(37) Università di Trento, Povo, Trento

I-38123, Italy

(38) Università Degli Studi di Urbino 'Carlo Bo', Urbino

I-61029, Italy

(39) Konkoly Thege, Miklós út 29-33, Hungary^9

关键词: Detection rates;    Technical features;    Three orders of magnitude;    Time schedules;    VIRGO detector;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/610/1/012014/pdf
DOI  :  10.1088/1742-6596/610/1/012014

来源: IOP

【 摘 要 】

The Advanced Virgo interferometer is the upgraded version of the Virgo detector having the goal to extend by a factor 10 the observation horizon in the universe and consequently increase the detection rate by three orders of magnitude. Its installation is in progress and is expected to be completed in late 2015. In this proceeding we will present the scheme and the main challenging technical features of the detector and we will give an outline of the installation status and the foreseen time schedule which will bring Advanced Virgo to its full operation.