SENSITIVITY OF A RIGID SMALL INTERFEROMETER IN THE 10-HZ FREQUENCY REGION

被引：19

作者：

BRADASCHIA, C

DELFABBRO, R

DIVIRGILIO, A

FLAMINIO, R

GIAZOTTO, A

MICHELOZZI, B

MONTELATICI, V

PASSUELLO, D

BRILLET, A

MAN, NC

CALLONI, E

HOLLOWAY, LE

VELLOSO, W

机构：

[1] UNIV PISA,DIPARTIMENTO FIS,I-56100 PISA,ITALY

[2] CNRS,GRAVITAT & COSMOL RELAT LAB,F-91405 ORSAY,FRANCE

[3] IST NAZL FIS NUCL,NAPLES,ITALY

[4] NAPLES UNIV,DIPARTIMENTO FIS,I-80138 NAPLES,ITALY

[5] UNIV ILLINOIS,DEPT PHYS,URBANA,IL 61801

[6] UNIV SAO PAULO,FAPESP,SAO PAULO,BRAZIL

来源：

PHYSICS LETTERS A | 1992年 / 163卷 / 1-2期

关键词：

D O I：

10.1016/0375-9601(92)90152-C

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

In the framework of the development of the super attenuators for VIRGO, the French-Italian long arm interferometric antenna for gravitational wave detection, a small interferometer has been built in the Pisa laboratory, to investigate the sensitivity in the low frequency region. The noise measured at 10 Hz is below 10(-13)m/square-root Hz, about a factor of 10 less than previous measurements in Munich. Calculation shows that the noise between 10 and 100 Hz is compatible with seismic noise.

引用

页码：15 / 20

页数：6

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