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Chinese Journal of Lasers

Optimal Design of Single-Frequency Laser System for 795 nm Squeezed Light Source

李志秀 Li Zhixiu, 杨文海 Yang Wenhai, 王雅君 Wang Yajun, 郑耀辉 Zheng Yaohui

Published Jan 1, 2015• 1 citation
Publisher
DOI
10.3788/cjl201542.0902002

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The worldwide network of laser interferometric gravitational-wave detectors is currently in an upgrade phase and will most likely detect gravitational waves within the next few years. Their strain sensitivity will be limited by photon shot noise over a large frequency band. A measurement beyond the shot noise level has already been accomplished via injecting squeezed vacuum states of light into the interferometers. In this proceeding, I review the current status in developements for the next-generation squeezed-light sources for future gravitational-wave detectors. A newly designed doubly-resonant squeezed light source is discussed, as well as squeezed light generated at the wavelengths of 1550 nm and 532 nm. Furthermore, high­ efficiency second harmonic generation of laser light for gravitational wave detectors will be presented. The injection of squeezed light as a key technology is well on schedule for improving the sensitivity of future gravitational-wave detectors.