Status and perspectives of the Virgo gravitational wave detector

被引：32

作者：

Accadia, T. ^{[21
]}

Acernese, F. ^{[21
]}

Antonucci, F. ^{[15
]}

Aoudia, S. ^{[25
]}

Arun, K. G. ^{[20
]}

Astone, P. ^{[15
]}

Ballardin, G. ^{[2
]}

Barone, F. ^{[7
,9
]}

Barsuglia, M. ^{[1
]}

Bauer, Th. S. ^{[23
]}

Beker, M. G. ^{[23
]}

Belletoile, A. ^{[21
]}

Bigotta, S. ^{[12
,13
]}

Birindelli, S. ^{[25
]}

Bizouard, M. A. ^{[20
]}

Blom, M. ^{[23
]}

Boccara, C. ^{[3
]}

Bondu, F. ^{[26
]}

Bonelli, L. ^{[12
,13
]}

Bonnand, R. ^{[22
]}

Bosi, L. ^{[10
]}

Braccini, S. ^{[12
]}

Bradaschia, C. ^{[12
]}

Brillet, A. ^{[25
]}

Brisson, V. ^{[20
]}

Budzynski, R. ^{[32
]}

Bulik, T. ^{[33
,34
]}

Bulten, H. J. ^{[23
,24
]}

Buskulic, D. ^{[21
]}

Buy, C. ^{[1
]}

Cagnoli, G. ^{[4
]}

Calloni, E. ^{[7
,8
]}

Campagna, E. ^{[4
,5
]}

Canuel, B. ^{[2
]}

Carbognani, F. ^{[2
]}

Cavalier, F. ^{[20
]}

Cavalieri, R. ^{[2
]}

Cella, G. ^{[12
]}

Cesarini, E. ^{[5
]}

Chassande-Mottin, E. ^{[1
]}

Chincarini, A. ^{[6
]}

Cleva, F. ^{[25
]}

Coccia, E. ^{[17
,18
]}

Colacino, C. N. ^{[12
]}

Colas, J. ^{[2
]}

Colla, A. ^{[15
,16
]}

Colombini, M. ^{[16
]}

Corsi, A. ^{[15
]}

Coulon, J. -P. ^{[25
]}

Cuoco, E. ^{[2
]}

机构：

[1] Univ Denis Diderot Paris VII, CEA DSM IRFU, Observ Paris, APC,CNRS UMR7164,IN2P3, Paris, France

[2] EGO, I-56021 Cascina, Pi, Italy

[3] CNRS, ESPCI, F-75005 Paris, France

[4] Ist Nazl Fis Nucl, Sez Firenze, I-50019 Sesto Fiorentino, Italy

[5] Univ Urbino Carlo Bo, I-61029 Urbino, Italy

[6] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy

[7] Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy

[8] Univ Napoli Federico II, I-80126 Naples, Italy

[9] Univ Salerno, I-84084 Salerno, Italy

[10] Ist Nazl Fis Nucl, Sez Perugia, I-6123 Perugia, Italy

[11] Univ Perugia, I-6123 Perugia, Italy

[12] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[13] Univ Pisa, I-56127 Pisa, Italy

[14] Univ Siena, I-53100 Siena, Italy

[15] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

[16] Univ Roma La Sapienza, I-00185 Rome, Italy

[17] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy

[18] Univ Roma Tor Vergata, I-00133 Rome, Italy

[19] Univ Aquila, I-67100 Laquila, Italy

[20] Univ Paris 11, LAL, IN2P3, CNRS, F-91898 Orsay, France

[21] Univ Savoie, IN2P3, CNRS, LAPP, F-74941 Annecy Le Vieux, France

[22] CNRS, IN2P3, LMA, F-69622 Villeurbanne, Lyon, France

[23] Natl Inst Subatom Phys, NL-1009 DB Amsterdam, Netherlands

[24] Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands

[25] Univ Nice Sophia Antipolis, CNRS, Observ Cote Azur, F-06304 Nice, France

[26] Univ Rennes 1, CNRS, Inst Phys Rennes, F-35042 Rennes, France

[27] Ist Nazl Fis Nucl, Grp Collegato Trento, I-38050 Povo, Trento, Italy

[28] Univ Trento, I-38050 Povo, Trento, Italy

[29] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[30] Univ Padua, I-35131 Padua, Italy

[31] IM PAN, PL-00956 Warsaw, Poland

[32] Warsaw Univ, F Phys, PL-00681 Warsaw, Poland

[33] Warsaw Univ, Astro Obs, PL-00478 Warsaw, Poland

[34] CAMK PAN, PL-00716 Warsaw, Poland

[35] Bialystok Univ, PL-15424 Bialystok, Poland

[36] IPJ, PL-05400 Otwock, Poland

[37] Inst Astron, 17-65265 Zielona Gora, Poland

[38] Univ Birmingham, Birmingham B15 2TT, W Midlands, England

来源：

TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS (TAUP2009) | 2010年 / 203卷

关键词：

D O I：

10.1088/1742-6596/203/1/012074

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Virgo is designed to detect gravitational waves of both astrophysical and cosmological origin in the frequency range from a few Hz to a few kHz. After the end of the first science run, partially overlapped with the LIGO fifth science run, the detector underwent several upgrades to improve its sensitivity. The second Virgo science run started at the beginning of July 2009 in coincidence with LIGO. A further upgrade is planned at beginning of 2010 with the installation of new suspensions for the test masses and of new mirrors. This will lead to a considerable improvement in the sensitivity and represents an intermediate step toward the development of the advanced detectors.

引用

页数：5

共 2 条

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