Laser frequency stabilization with the use of homodyne quadrature interferometers

被引:0
|
作者
Di Fronzo, C. [1 ,2 ,3 ]
Holland, N. A. [4 ,5 ]
Mitchell, A. L. [4 ,5 ]
Cooper, S. J. [2 ,3 ]
Valentini, M. [4 ,5 ]
Martynov, D. [2 ,3 ]
Prokhorov, L. [2 ,3 ]
Mow-Lowry, C. M. [2 ,4 ,5 ]
机构
[1] Univ Liege, Precis Mechatron Lab, B-4000 Liege, Belgium
[2] Univ Birmingham, Inst Gravitat Wave Astron, Birmingham B15 2TT, England
[3] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, England
[4] Dutch Natl Inst Subatom Phys Nikhef, NL-1098 XG Amsterdam, Netherlands
[5] Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands
基金
欧洲研究理事会;
关键词
laser stabilization; compact interferometry; gravitational waves;
D O I
10.1088/1361-6382/ad13c4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Laser frequency stabilization is a crucial technique for precision metrology. We demonstrate laser frequency control using a compact, interferometric sensor, specially modified for sensitivity to laser frequency noise. This setup achieves a balance between compact size, ease of use, and affordability. We stabilize the laser frequency noise, of a low-cost solid-state laser, to 4.5 kHz Hz-1 at 1 Hz. The requirement for additional technology, and expense, is negated when identical, compact, interferometric sensors are deployed. The use of compact interferometric sensors is already a technology under investigation for integration into gravitational-wave observatories and out study enables wider applications by mitigating a fundamental noise source, inherent to their design.
引用
收藏
页数:10
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