Surpassing the standard quantum limit via gain-assisted auxiliary cavities and parametric amplification

The detection of weak forces plays a crucial role in various fields, from gravitational wave astronomy to biological sensing. A fundamental limitation in such measurements arises from quantum and thermal noise. Here, we present a theoretical scheme for force sensing that incorporates an optical parametric amplifier (OPA) in conjunction with a gain-assisted auxiliary cavity. We show that, in contrast to conventional lossy configurations, the presence of optical gain in the auxiliary cavity enables a substantial enhancement in sensitivity, allowing the system to exceed the standard quantum limit across a broad detection bandwidth. By carefully tuning the gain parameter, cavity-cavity coupling strength, OPA driving phase, and detuning conditions, the system achieves optimal noise suppression. Remarkably, this performance persists even under a twentyfold increase in environmental temperature, underscoring the robustness of the proposed scheme. Detailed noise analysis reveals that the contribution of the gain-assisted auxiliary cavity appears to be a negative value in the noise spectrum, effectively reducing the overall noise level of the system. This study is of significant importance to the design and fabrication of high-performance optomechanical sensors.