QND measurements for future gravitational-wave detectors

被引：30

作者：

Chen, Yanbei ^{[2
]}

Danilishin, Stefan L. ^{[1
]}

Khalili, Farid Ya. ^{[1
]}

Mueller-Ebhardt, Helge ^{[3
,4
]}

机构：

[1] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119991, Russia

[2] CALTECH, Pasadena, CA 91125 USA

[3] Leibniz Univ Hannover, D-30167 Hannover, Germany

[4] Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-30167 Hannover, Germany

来源：

GENERAL RELATIVITY AND GRAVITATION | 2011年 / 43卷 / 02期

关键词：

Gravitational-wave detectors; Quantum Non-Demolition (QND) measurement; Standard Quantum Limit (SQL) beating; Optical rigidity; Quantum speed meter; Intracavity schemes; POLARIZATION SAGNAC INTERFEROMETER; QUANTUM LIMITS; SPEED METER; ANTENNAE; RIGIDITY; NOISE;

D O I：

10.1007/s10714-010-1060-y

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Second-generation interferometric gravitational-wave detectors will be operating at the Standard Quantum Limit (SQL), a sensitivity limitation set by the trade off between measurement accuracy and quantum back action, which is governed by the Heisenberg Uncertainty Principle. We review several schemes that allows the quantum noise of interferometers to surpass the SQL significantly over a broad frequency band. Such schemes may be an important component of the design of third-generation detectors.

引用

页码：671 / 694

页数：24

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