Abstract
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.
| Original language | English |
|---|---|
| Article number | L041101 |
| Journal | Physical Review D |
| Volume | 106 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - 15 Aug 2022 |
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