The gravitational wave burst observatory: Present state and future perspectives

被引：1

作者：

Baggio, L

Bonaldi, M

Cerdonio, M

Conti, L

Visconti, VC

Falferi, P

Fortini, P

Mezzena, R

Martinucci, V

Ortolan, A

Prodi, GA

Taffarello, L

Vedovato, G

Vitale, S

Zendri, JP

机构：

[1] Univ Padua, Dept Phys, I-35131 Padua, Italy

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

[3] CNR, ITC, Ctr CeFSA, I-38050 Trento, Italy

[4] Ist Nazl Fis Nucl, Grp Coll Trento, Sez Padova, I-38050 Trento, Italy

[5] Univ Trent, Dept Phys, I-38050 Trento, Italy

[6] Univ Ferrara, Dept Phys, I-44100 Ferrara, Italy

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

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

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 1999年 / 70卷

关键词：

D O I：

10.1016/S0920-5632(98)00490-3

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The expected performances of the gravitational wave observatory composed by the five resonant detectors currently in operation are discussed. The potential near future improvements are also examined assuming that the noise properties of the up-graded resonant detectors will be in agreement with predictions. With the initial operation of long baselines interferometers a substantial improvement in the burst search is expected.

引用

页码：537 / 544

页数：8

共 18 条

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