Magnetic noise in macroscopic quantum spatial superposition induced by inverted harmonic oscillator potential

Abstract

We investigate a Stern-Gerlach type matter-wave interferometer where an inhomogeneous magnetic field couples to an embedded spin in a nanoparticle to create spatial superpositions. Employing a sequence of harmonic and inverted harmonic oscillator potentials created by external magnetic fields, we aim to enhance the one-dimensional superposition of a nanodiamond with mass $\sim 10^{-15}$ kg to $\sim 1 μ$m. However, random fluctuations of the magnetic field stochastically perturbs the interferometer paths and induce dephasing. We quantitatively estimate the susceptibility of the interferometer to white noise arising from magnetic-field fluctuations. Constraining the dephasing rate \(Γ\) to be low enough that the final coherence \(e^{-Γτ}\leq 0.1\) (where \(τ\) is the experimental time duration), we obtain the following bounds on the noise to signal ratios: $δη_\text{IHP}/η_\text{IHP}\lesssim 10^{-13}$, where $η_\text{IHP}$ is the magnetic field curvature that gives rise to the inverted harmonic potential, and $δη_\text{HP}/η_\text{HP}\lesssim 10^{-6}$, where $η_\text{HP}$ is the linear magnetic field gradient that gives rise to the harmonic potential. For such tiny fluctuations, we demonstrate that the Humpty-Dumpty problem arising from a mismatch in position and momentum does not cause a loss in contrast of the interferometer. Further, we show that constraining the dephasing rate leads to stricter bounds on the noise parameters than enforcing a contrast threshold, indicating that good dephasing control ensures high interferometric contrast.