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

    Sneha Narasimha Moorthy1,2 and Anupam Mazumdar3

    Phys. Rev. A 113, 012419 – Published 9 January, 2026

    DOI: https://doi.org/10.1103/nkr5-9dxr

    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 ≈10−15kg to ≈1µm. 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≥0.1 (where τ is the experimental time duration), we obtain the following bounds on the noise to signal ratios: δηIHP/ηIHP≲10−13, where ηIHP is the magnetic-field curvature that gives rise to the inverted harmonic potential, and δηHP/ηHP≲10−6, where ηHP 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. Furthermore, 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.

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