First search for gravitational wave bursts with a network of detectors

被引：82

作者：

Allen, ZA

Astone, P

Baggio, L

Busby, D

Bassan, M

Blair, DG

Bonaldi, M

Bonifazi, P

Carelli, P

Cerdonio, M

Coccia, E

Conti, L

Cosmelli, C

Visconti, VC

D'Antonio, S

Fafone, V

Falferi, P

Fortini, P

Frasca, S

Hamilton, WO

Heng, IS

Ivanov, EN

Johnson, WW

Kingham, M

Locke, CR

Marini, A

Martinucci, V

Mauceli, E

McHugh, MP

Mezzena, R

Minenkov, Y

Modena, I

Modestino, G

Moleti, A

Ortolan, A

Pallottino, GV

Pizzella, G

Prodi, GA ^{[1
]}

Rocco, E

Ronga, F

Salemi, F

Santostasi, G

Taffarello, L

Terenzi, R

Tobar, ME

Vedovato, G

Vinante, A

Visco, M

Vitale, S

Votano, L

机构：

[1] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA

[2] Ist Nazl Fis Nucl, I-00185 Rome, Italy

[3] Univ Padua, Dipartimento Fis, I-35131 Padua, Italy

[4] Ist Nazl Fis Nucl, I-35131 Padua, Italy

[5] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy

[6] Ist Nazl Fis Nucl, I-00133 Rome, Italy

[7] Univ Western Australia, Dept Phys, Nedlands, WA 6907, Australia

[8] CNR, ITC, Ctr Fis Stati Aggregati, I-38050 Trento, Italy

[9] Ist Nazl Fis Nucl, I-38050 Trento, Italy

[10] CNR, Ist Fis Spazio Interplanetario, I-00133 Rome, Italy

[11] Univ Aquila, Dipartimento Fis, I-67100 Laquila, Italy

[12] Ist Nazl Fis Nucl, I-67100 Laquila, Italy

[13] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy

[14] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy

[15] Univ Ferrara, Dipartmento Fis, I-44100 Ferrara, Italy

[16] Ist Nazl Fis Nucl, I-44100 Ferrara, Italy

[17] Univ Trent, Dipartimento Fis, I-38050 Trento, Italy

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

[19] Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Legnaro, Padova, Italy

[20] Ist Nazl Fis Nucl, I-35131 Padua, Italy

来源：

PHYSICAL REVIEW LETTERS | 2000年 / 85卷 / 24期

关键词：

D O I：

10.1103/PhysRevLett.85.5046

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We report the initial results from a search for bursts of gravitational radiation by a network of five cryogenic resonant detectors during 1997 and 1998. This is the first significant search with mon than two detectors observing simultaneously. No gravitational wave burst was detected. The false alarm rate was lower than 1 per 10(4) yr when three or more detectors were operating simultaneously. The typical threshold was H similar or equal to 4 x 10(-21) Hz(-1) on the Fourier component at similar to 10(3) Hz of the gravitational wave strain amplitude. New upper Limits for amplitude and rate of gravitational wave bursts have been set.

引用

页码：5046 / 5050

页数：5

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