2024 (v1)
Publication
The sensitivity of future gravitational wave (GW) detectors, such as the Einstein Telescope (ET), is constrained by quantum noise across the entire frequency range (10 Hz–10 kHz) and by magnetic noise at low frequencies (a few Hz to around 100 Hz). This article examines optimizing mechanisms to achieve efficient squeezing for reducing quantum...
Uploaded on: September 6, 2024