The status of the Brazilian spherical detector

被引：27

作者：

Aguiar, OD ^{[1
]}

Andrade, LA

Camargo, L

Costa, CA

de Araújo, JCN

Neto, ECD

de Souza, ST

Fauth, AC

Frajuca, C

Frossati, G

Furtado, SR

Furtado, VGS

Magalhaes, NS

Marinho, RM

Matos, ES

Meliani, MT

Melo, JL

Miranda, OD

Oliveira, NF

Ribeiro, KL

Salles, KBM

Stellati, C

Velloso, WF

机构：

[1] Inst Nacl Pesquisas Espaciais, Div Astrofis, BR-12201 Sao Jose Dos Campos, Brazil

[2] Univ Sao Paulo, Inst Fis, BR-01498 Sao Paulo, Brazil

[3] Inst Tecnol Aeronaut, Sao Jose Dos Campos, Brazil

[4] Univ Estadual Campinas, Inst Fis, Campinas, SP, Brazil

[5] Ctr Fed Ensino Tecnol Sao Paulo, Sao Paulo, Brazil

[6] Univ Bandeirante Sao Paulo, Sao Paulo, Brazil

[7] Leiden Univ, Kamerlingh Onnes Lab, NL-2300 RA Leiden, Netherlands

来源：

CLASSICAL AND QUANTUM GRAVITY | 2002年 / 19卷 / 07期

关键词：

D O I：

10.1088/0264-9381/19/7/397

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The first phase of the Brazilian Graviton Project is the construction and operation of the gravitational wave detector Mario Schenberg at the Physics Institute of the University of Sao Paulo. This gravitational wave spherical antenna is planned to feature a sensitivity better than h = 10(-21) Hz(-1/2) at the 3.0-3.4 kHz bandwidth, and to work not only as a detector, but also as a testbed for the development of new technologies. Here we present the status of this detector.

引用

页码：1949 / 1953

页数：5

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