Performance of the Glasgow 10 m prototype gravitational wave detector operating at λ=1064 nm

被引：5

作者：

Skeldon, KD ^{[1
]}

Clubley, DA ^{[1
]}

Barr, BW ^{[1
]}

Casey, MM ^{[1
]}

Hough, J ^{[1
]}

Killbourn, SD ^{[1
]}

McNamara, PW ^{[1
]}

Newton, GP ^{[1
]}

Plissi, MV ^{[1
]}

Robertson, DI ^{[1
]}

Robertson, NA ^{[1
]}

Strain, KA ^{[1
]}

Ward, H ^{[1
]}

机构：

[1] Univ Glasgow, Dept Phys & Astron, Glasgow G12 8QQ, Lanark, Scotland

来源：

PHYSICS LETTERS A | 2000年 / 273卷 / 5-6期

关键词：

D O I：

10.1016/S0375-9601(00)00511-9

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We report on measurements performed with the Glasgow prototype gravitational wave detector which has recently been converted to operate with a Nd:YAG laser at 1064 nm. The differential displacement amplitude spectral density above a few hundred Hz is similar to 5 x 10(-19) m/root Hz which is consistent with the limitations imposed by shot noise in this frequency range. We also present sensitivity spectra over a lower frequency regime to highlight the impact of improved suspension designs. (C) 2000 Elsevier Science B.V. All rights reserved.

引用

页码：277 / 284

页数：8

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