Measurement of the seismic attenuation performance of the VIRGO Superattenuator

被引：75

作者：

Braccini, S

Barsotti, L

Bradaschia, C

Cella, G

Di Virgilio, A

Ferrante, I

Fidecaro, F

Fiori, I

Frasconi, F

Gennai, A

Giazotto, A

Paoletti, F

Passaquieti, R

Passuello, D

Poggiani, R

Campagna, E

Guidi, G

Losurdo, G

Martelli, F

Mazzoni, M

Perniola, B

Piergiovanni, F

Stanga, R

Vetrano, F

Viceré, A

Brocco, L

Frasca, S

Majorana, E

Pai, A

Palomba, C

Puppo, P

Rapagnani, P

Ricci, F

Ballardin, G

Barillé, R

Cavalieri, R

Cuoco, E

Dattilo, V

Enard, D

Flaminio, R

Freise, A

Hebri, S

Holloway, L

La Penna, P

Loupias, M

Marque, J

Moins, C

Pasqualetti, A

Ruggi, P

Taddei, R

机构：

[1] Univ Pisa, Sez Pisa Andlor, Ist Nazl Fis Nucl, I-56127 Pisa, Italy

[2] Sez Firenze Urbino, Ist Nazl Fis Nucl, I-50019 Florence, Italy

[3] Univ Florence, I-50125 Florence, Italy

[4] Univ Urbino, I-61029 Urbino, Italy

来源：

ASTROPARTICLE PHYSICS | 2005年 / 23卷 / 06期

关键词：

D O I：

10.1016/j.astropartphys.2005.04.002

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The gravitational wave detector VIRGO aims at extending the detection band down to a few Hertz by isolating the mirrors of the interferometer from seismic noise. This result is achieved by hanging each mirror through an elastic suspension (Superattenuator), designed to filter mechanical vibrations in all the degrees of freedom. An experimental upper limit of the mirror residual seismic noise at a few Hertz is provided in this paper. This is lower than the thermal noise floor, expected to limit the antenna sensitivity in the low frequency range. (c) 2005 Elsevier B.V. All rights reserved.

引用

页码：557 / 565

页数：9

共 23 条

[1] Seismic isolation for Advanced LIGO
Abbott, R
Adhikari, R
Allen, G
Cowley, S
Daw, E
DeBra, D
Giaime, J
Hammond, G
Hammond, M
Hardham, C
How, J
Hua, W
Johnson, W
Lantz, B
Mason, K
Mittleman, R
Nichol, J
Richman, S
Rollins, J
Shoemaker, D
Stapfer, G
Stebbins, R
[J]. CLASSICAL AND QUANTUM GRAVITY, 2002, 19 (07) : 1591 - 1597
[2] The present status of the VIRGO Central Interferometer
Acernese, F
Amico, P
Arnaud, N
Arnault, C
Babusci, D
Ballardin, G
Barone, F
Barsuglia, M
Bellachia, F
Beney, JL
Bilhaut, R
Bizouard, MA
Boccara, C
Boget, D
Bondu, F
Bourgoin, C
Bozzi, A
Bracci, L
Braccini, S
Bradaschia, C
Brillet, A
Brisson, V
Buskulic, D
Cachenaut, J
Calamai, G
Calloni, E
Canitrot, P
Caron, B
Casciano, C
Cattuto, C
Cavalier, F
Cavaliere, S
Cavalieri, R
Cecchi, R
Cella, G
Chiche, R
Chollet, F
Cleva, F
Cokelaer, T
Cortese, S
Coulon, JP
Cuoco, E
Cuzon, S
Dattilo, V
David, PY
Davier, M
De Rosa, M
De Rosa, R
Dehamme, M
Di Fiore, L
[J]. CLASSICAL AND QUANTUM GRAVITY, 2002, 19 (07) : 1421 - 1428
[3] Properties of seismic noise at the Virgo site
Acernese, F
Amico, P
Arnaud, N
Babusci, D
Barillé, R
Barone, F
Barsotti, L
Barsuglia, M
Beauville, F
Bizouard, MA
Boccara, C
Bondu, F
Bosi, L
Bradaschia, C
Bracci, L
Braccini, S
Brillet, A
Brisson, V
Brocco, L
Buskulic, D
Calamai, G
Calloni, E
Campagna, E
Cavalier, F
Cella, G
Chassande-Mottin, E
Cleva, F
Cokelaer, T
Corda, C
Coulon, JP
Cuoco, E
Dattilo, V
Davier, M
De Rosa, R
Di Fiore, L
Di Virgilio, A
Dujardin, B
Eleuteri, A
Enard, D
Ferrante, I
Fidecaro, F
Fiori, I
Flaminio, R
Fournier, JD
Frasca, S
Frasconi, F
Gammaitoni, L
Gennai, A
Giazotto, A
Giordano, G
[J]. CLASSICAL AND QUANTUM GRAVITY, 2004, 21 (05) : S433 - S440
[4] First locking of the Virgo central area interferometer with suspension hierarchical control
Acernese, F
Amico, P
Arnaud, N
Babusci, D
Barillé, R
Barone, F
Barsotti, L
Barsuglia, M
Beauville, F
Bizouard, MA
Boccara, C
Bondu, F
Bosi, L
Bradaschia, C
Bracci, L
Braccini, S
Brillet, A
Brisson, V
Brocco, L
Buskulic, D
Calamai, G
Calloni, E
Campagna, E
Cavalier, F
Cella, G
Chassande-Mottin, E
Cleva, F
Cokelaer, T
Confort, G
Corda, C
Coulon, JP
Cuoco, E
Dattilo, V
Davier, M
De Rosa, R
Di Fiore, L
Di Virgilio, A
Dujardin, B
Eleuteri, A
Enard, D
Ferrante, I
Fidecaro, F
Fiori, I
Flamino, R
Fournier, JD
Frasca, S
Frasconi, F
Gammaitoni, L
Gennai, A
Giazotto, A
[J]. ASTROPARTICLE PHYSICS, 2004, 20 (06) : 629 - 640
[5] Acernese F, 2003, CLASSICAL QUANT GRAV, V20, pS609, DOI 10.1088/0264-9381/20/17/304
[6] ACERNESE F, 2002, CLASSICAL QUANT GRAV, V19, P1631
[7] ACERNESE F, 2002, CLASSICAL QUANT GRAV, V19, P1623
[8] The thermal noise limit to the Virgo sensitivity
Amico, P
Carbone, L
Cattuto, C
Gammaitoni, L
Marchesoni, F
Mischianti, R
Punturo, M
Travasso, F
Vocca, H
[J]. CLASSICAL AND QUANTUM GRAVITY, 2001, 18 (19) : 4127 - 4131
[9] Measurement of the VIRGO superattenuator performance for seismic noise suppression
Ballardin, G
Bracci, L
Braccini, S
Bradaschia, C
Casciano, C
Calamai, G
Cavalieri, R
Cecchi, R
Cella, G
Cuoco, E
D'Ambrosio, E
Dattilo, V
Di Virgilio, A
Fabbroni, L
Fidecaro, F
Frasconi, F
Gaddi, A
Gennai, A
Gennaro, G
Giazotto, A
Losurdo, G
Holloway, L
La Penna, P
Lelli, F
Majorana, E
Mazzoni, M
Paoletti, F
Pasotti, M
Pasqualetti, A
Passaquieti, R
Passuello, D
Poggiani, R
Puppo, P
Raffaelli, F
Rapagnani, P
Ricci, F
Ruggi, P
Stanga, R
Taddei, R
Vetrano, F
Vicerè, A
Zhang, Z
[J]. REVIEW OF SCIENTIFIC INSTRUMENTS, 2001, 72 (09) : 3643 - 3652
[10] Extending the VIRGO gravitational wave detection band down to a few Hz: metal blade springs and magnetic antisprings
Beccaria, M
Bernardini, M
Bougleux, E
Braccini, S
Bradaschia, C
Casciano, C
Cella, G
Cucco, E
DAmbrosio, E
DeCarolis, G
DelFabbro, R
DeSalvo, R
DiVirgilio, A
Ferrante, I
Fidecaro, F
Flaminio, R
Gaddi, A
Gennai, A
Gennaro, G
Giazotto, A
Holoway, L
LaPenna, P
Losurdo, G
Malik, S
Mancini, S
Nicolas, J
Palla, F
Pan, HB
Paoletti, F
Pasqualetti, A
Passuello, D
Poggiani, R
Popolizio, P
Raffaelli, F
Vicere, A
Waharte, F
Zhang, Z
[J]. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1997, 394 (03) : 397 - 408

← 1 2 3 →