Fig. 2: SMSS performance.
From: Quantum-enhanced dark matter detection with in-cavity control: mitigating the Rayleigh curse

Performance (a, b) versus squeezing gain G with NT = 10−2 fixed; c, d versus thermal background photon number NT with G = 40 dB fixed. a, c Advantage (in dB unit) of T-optimized quantum Fisher information rate \({{\mathcal{R}}}^{\star }\equiv \mathop{\max }\limits_{T}{\mathcal{J}}(T)/T\) over vacuum state input; b, d optimal waiting time T⋆ normalized by axion coherence time τA (in log10 scale). Solid lines: T numerically optimized; Dot-dashed lines: asymptotic prediction with \(T=2\sqrt{2{N}_{{\rm{T}}}}{\tau }_{A}/\Gamma {\tau }_{A}G\). Purple dashed lines: asymptotic prediction of linear advantage Eq. (9) assuming non-saturated strong squeezing GSAT ≫ G ≫ GTH, NT ≪ 1, ΓτA ≪ 1. In subplot (a, b) we mark GTH (≃20 dB here) and GSAT (≃55 dB here) by right-pointing triangle and left-pointing triangle respectively. Gray dashed lines: 0dB advantage and G-saturated advantage Eq. (10). Cavity parameters: ΓτA = 10−8.