Journal
PHYSICAL REVIEW D
Volume 106, Issue 4, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.106.L041101
Keywords
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Funding
- Australian Research Council under the ARC Centre of Excellence for Gravitational Wave Discovery [CE170100004]
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This study aims to enhance the sensitivity of interferometric gravitational-wave detectors through nondegenerate internal squeezing. The research shows that this all-optical technique is stable and tolerant to decoherence from optical detection loss, making broadband sensitivity enhancement feasible.
The detection of kilohertz-band gravitational waves promises discoveries in astrophysics, exotic matter, and cosmology. To improve the kilohertz quantum noise-limited sensitivity of interferometric gravitational -wave detectors, we investigate nondegenerate internal squeezing: optical parametric oscillation inside the signal-recycling cavity with distinct signal-mode and idler-mode frequencies. We use an analytic Hamiltonian model to show that this stable, all-optical technique is tolerant to decoherence from optical detection loss and that it, with its optimal readout scheme, is feasible for broadband sensitivity enhancement.
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