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September 5, 2025Acta Physica SinicaOpen Access

Upgrades and Improvements of Laser Interferometric Gravitational Wave Detectors

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Gravitational wave detectors have improved sensitivity, achieving strain sensitivities of about 10^-24/√Hz.
Key advancements include techniques such as squeezed light and advanced seismic isolation to mitigate noise sources.
LIGO's transition from Initial to Advanced configurations directly led to the first detection of gravitational waves.
Next-generation projects like LIGO Voyager aim for significant improvements in sensitivity for future astronomical research.

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This review highlights upgrades to LIGO, Virgo, and KAGRA, revealing approaches to mitigate noise sources and enhance sensitivity.

Xiaoman et al. (2025) studied this question.

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