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Random acceleration noise on Stern-Gerlach interferometry in a harmonic trap

Sneha Narasimha Moorthy1,2,*, Andrew Geraci3, Sougato Bose4, and Anupam Mazumdar5

  • *Contact author: snehahema1029@gmail.com

APS Open Sci. 1, 000106 – Published 25 August, 2026

DOI: https://doi.org/10.1103/3jjv-vwmv

Abstract

We analyze decoherence in a one-loop Stern-Gerlach-type matter-wave interferometer for a massive nanoparticle embedded with a nitrogen-vacancy-centered nanodiamond evolving under an effective harmonic-oscillator dynamics in a magnetic-field gradient. We assume that the Stern-Gerlach interferometer is subjected to an acceleration a⃗ external to the system, which is at an angle θ0 with respect to the direction of the superposition. For a one-loop interferometer, we quantify dephasing from two noise channels: fluctuations in the external acceleration δa(t) and fluctuations in the tilt angle δθ(t). At the level of the action, we treat these two external sources of noise as stochastic inputs, compute the resulting stochastic phase difference between the interferometer arms, and obtain the dephasing rate Γ. We obtain the transfer function of the interferometer for each of the noise sources. We also show explicit results of constraints on the power spectral density of the noise sources for an interferometer that produces a superposition size of Δx∼1nm of a nanodiamond of mass m=10−15kg by considering white-noise statistics and imposing a coherence target Γτ≤1, where τ≃0.015s. We find Saa≲O(10−11)ms−2Hz−1/2 if we take the external acceleration, a=0ms−2 and θ0=0∘ (along the direction of the superposition), and Sθθ≲O(10−10)radHz−1/2 for a=g=9.81ms−2 and θ0=90∘ (superposition direction is perpendicular to the Earth’s gravity). We have also found an operating regime where the acceleration noise can be minimized by either varying θ0 or a for a fixed set of other experimental parameters.

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References (92)

  1. R. Colella, A. W. Overhauser, and S. A. Werner, Observation of gravitationally induced quantum interference, Phys. Rev. Lett. 34, 1472 (1975).
  2. S. A. Werner, J. L. Staudenmann, and R. Colella, Effect of Earth’s rotation on the quantum mechanical phase of the neutron, Phys. Rev. Lett. 42, 1103 (1979).
  3. H. Rauch and S. A. Werner, Neutron Interferometry: Lessons in Experimental Quantum Mechanics, 2nd ed. (Oxford University Press, Oxford, UK, 2015).
  4. J. B. Fixler, G. T. Foster, J. M. McGuirk, and M. A. Kasevich, Atom interferometer measurement of the Newtonian constant of gravity, Science 315, 74 (2007).
  5. P. Asenbaum, C. Overstreet, T. Kovachy, D. D. Brown, J. M. Hogan, and M. A. Kasevich, Phase shift in an atom interferometer due to spacetime curvature across its wave function, Phys. Rev. Lett. 118, 183602 (2017).
  6. C. Overstreet, P. Asenbaum, J. Curti, M. Kim, and M. A. Kasevich, Observation of a gravitational Aharonov-Bohm effect, Science 375, 226 (2022).
  7. O. Amit, Y. Margalit, O. Dobkowski, Z. Zhou, Y. Japha, M. Zimmermann, M. A. Efremov, F. A. Narducci, E. M. Rasel, W. P. Schleich, and R. Folman, T3 Stern-Gerlach matter-wave interferometer, Phys. Rev. Lett. 123, 083601 (2019).
  8. Y. Margalit, O. Dobkowski, Z. Zhou, O. Amit, Y. Japha, S. Moukouri, D. Rohrlich, A. Mazumdar, S. Bose, C. Henkel, and R. Folman, Realization of a complete Stern-Gerlach interferometer: Toward a test of quantum gravity, Sci. Adv. 7, eabg2879 (2021).
  9. T. Kovachy, Quantum superposition at the half-metre scale, Nature (London) 528, 530 (2015).
  10. M. Arndt, O. Nairz, J. Vos-Andreae, C. Keller, G. van der Zouw, and A. Zeilinger, Wave-particle duality of C60 molecules, Nature (London) 401, 680 (1999).
  11. S. Eibenberger, S. Gerlich, M. Arndt, M. Mayor, and J. Tüxen, Matter-wave interference with particles selected from a molecular library with masses exceeding 10000 amu, Phys. Chem. Chem. Phys. 15, 14696 (2013).
  12. Y. Y. Fein, P. Geyer, P. Zwick, F. Kiałka, S. Pedalino, M. Mayor, S. Gerlich, and M. Arndt, Quantum superposition of molecules beyond 25 kDa, Nat. Phys. 15, 1242 (2019).
  13. S. Pedalino, B. E. Ramírez-Galindo, R. Ferstl, K. Hornberger, M. Arndt, and S. Gerlich, Probing quantum mechanics with nanoparticle matter-wave interferometry, Nature (London) 649, 866 (2026).
  14. M. Arndt and K. Hornberger, Testing the limits of quantum mechanical superpositions, Nat. Phys. 10, 271 (2014).
  15. S. Bose, A. Mazumdar, G. W. Morley, H. Ulbricht, M. Toroš, M. Paternostro, A. Geraci, P. Barker, M. S. Kim, and G. Milburn, Spin entanglement witness for quantum gravity, Phys. Rev. Lett. 119, 240401 (2017).
  16. https://www.youtube.com/watch?v=0Fv-0k13s_k (2016).
  17. C. Marletto and V. Vedral, Gravitationally induced entanglement between two massive particles is sufficient evidence of quantum effects in gravity, Phys. Rev. Lett. 119, 240402 (2017).
  18. D. Biswas, S. Bose, A. Mazumdar, and M. Toroš, Gravitational optomechanics: Photon-matter entanglement via graviton exchange, Phys. Rev. D 108, 064023 (2023).
  19. S. G. Elahi, M. Schut, A. Dana, A. Grinin, S. Bose, A. Mazumdar, and A. Geraci, Diamagnetic microchip traps for levitated nanoparticle entanglement experiments, Phys. Rev. A 112, 063508 (2025).
  20. U. K. Beckering Vinckers, Á. De La Cruz-Dombriz, and A. Mazumdar, Quantum entanglement of masses with nonlocal gravitational interaction, Phys. Rev. D 107, 124036 (2023).
  21. S. Chakraborty, A. Mazumdar, and R. Pradhan, Distinguishing Jordan and Einstein frames in gravity through entanglement, Phys. Rev. D 108, L121505 (2023).
  22. S. Bose, A. Mazumdar, M. Schut, and M. Toroš, Entanglement witness for the weak equivalence principle, Entropy 25, 448 (2023).
  23. A. Bassi, K. Lochan, S. Satin, T. P. Singh, and H. Ulbricht, Models of wave-function collapse, underlying theories, and experimental tests, Rev. Mod. Phys. 85, 471 (2013).
  24. O. Romero-Isart, A. C. Pflanzer, F. Blaser, R. Kaltenbaek, N. Kiesel, M. Aspelmeyer, and J. I. Cirac, Large quantum superpositions and interference of massive nanometer-sized objects., Phys. Rev. Lett. 107, 020405 (2011).
  25. T. W. van de Kamp, R. J. Marshman, S. Bose, and A. Mazumdar, Quantum gravity witness via entanglement of masses: Casimir screening, Phys. Rev. A 102, 062807 (2020).
  26. M. Schut, J. Tilly, R. J. Marshman, S. Bose, and A. Mazumdar, Improving resilience of quantum-gravity-induced entanglement of masses to decoherence using three superpositions, Phys. Rev. A 105, 032411 (2022).
  27. M. Schut, P. Andriolo, M. Toroš, S. Bose, and A. Mazumdar, Expression for the decoherence rate due to air-molecule scattering in spatial qubits, Phys. Rev. A 111, 042211 (2025).
  28. S. Rijavec, M. Carlesso, A. Bassi, V. Vedral, and C. Marletto, Decoherence effects in non-classicality tests of gravity, New J. Phys. 23, 043040 (2021).
  29. M. Schut, A. Grinin, A. Dana, S. Bose, A. Geraci, and A. Mazumdar, Relaxation of experimental parameters in a quantum-gravity-induced entanglement of masses protocol using electromagnetic screening, Phys. Rev. Res. 5, 043170 (2023).
  30. S. N. Moorthy, A. Geraci, S. Bose, and A. Mazumdar, Magnetic noise in macroscopic quantum spatial superpositions, Phys. Rev. A 112, 022416 (2025).
  31. S. Narasimha Moorthy and A. Mazumdar, Magnetic noise in macroscopic quantum spatial superposition induced by an inverted harmonic oscillator potential, Phys. Rev. A 113, 012419 (2026).
  32. P. Fragolino, M. Schut, M. Toroš, S. Bose, and A. Mazumdar, Decoherence of a matter-wave interferometer due to dipole-dipole interactions, Phys. Rev. A 109, 033301 (2024).
  33. D. Leibfried, R. Blatt, C. Monroe, and D. Wineland, Quantum dynamics of single trapped ions, Rev. Mod. Phys. 75, 281 (2003).
  34. M. Toroš, T. W. van de Kamp, R. J. Marshman, M. S. Kim, A. Mazumdar, and S. Bose, Relative acceleration noise mitigation for nanocrystal matter-wave interferometry: Applications to entangling masses via quantum gravity, Phys. Rev. Res. 3, 023178 (2021).
  35. M.-Z. Wu, M. Toroš, S. Bose, and A. Mazumdar, Inertial torsion noise in matter-wave interferometers for gravity experiments, Phys. Rev. D 111, 064004 (2025).
  36. C. Henkel and R. Folman, Internal decoherence in nano-object interferometry due to phonons, AVS Quantum Sci. 4, 025602 (2022).
  37. C. Henkel and R. Folman, Universal limit on spatial quantum superpositions with massive objects due to phonons, Phys. Rev. A 110, 042221 (2024).
  38. Q. Xiang, R. Zhou, S. Bose, and A. Mazumdar, Phonon induced contrast in matter wave interferometer, Phys. Rev. A 110, 042614 (2024).
  39. B. A. Stickler, K. Hornberger, and M. S. Kim, Quantum rotations of nanoparticles, Nat. Rev. Phys. 3, 589 (2021).
  40. B. A. Stickler, B. Papendell, S. Kuhn, B. Schrinski, J. Millen, M. Arndt, and K. Hornberger, Probing macroscopic quantum superpositions with nanorotors, New J. Phys. 20, 122001 (2018).
  41. C. C. Rusconi, M. Perdriat, G. Hétet, O. Romero-Isart, and B. A. Stickler, Spin-controlled quantum interference of levitated nanorotors, Phys. Rev. Lett. 129, 093605 (2022).
  42. Y. Japha and R. Folman, Quantum uncertainty limit for Stern-Gerlach interferometry with massive objects, Phys. Rev. Lett. 130, 113602 (2023).
  43. T. Zhou, S. Bose, and A. Mazumdar, Gyroscopic stability for nanoparticles in Stern-Gerlach interferometry and spin contrast, Phys. Rev. A 112, 013315 (2025).
  44. R. Rizaldy, T. Zhou, S. Bose, and A. Mazumdar, Rotational stability in nanorotor and spin contrast in one-loop interferometry in the Stern-Gerlach setup, Phys. Rev. Res. 7, 043095 (2025).
  45. O. Romero-Isart, Quantum superposition of massive objects and collapse models, Phys. Rev. A 84, 052121 (2011).
  46. K. Hornberger, S. Gerlich, P. Haslinger, S. Nimmrichter, and M. Arndt, Colloquium: Quantum interference of clusters and molecules, Rev. Mod. Phys. 84, 157 (2012).
  47. B. Englert, J. Schwinger, and M. O. Scully, Is spin coherence like Humpty-Dumpty? I. Simplified treatment, Found. Phys. 18, 1045 (1988).
  48. J. Schwinger, M. O. Scully, and B. G. Englert, Is spin coherence like Humpty-Dumpty? Z. Phys. D 10, 135 (1988).
  49. M. O. Scully, B.-G. Englert, and J. Schwinger, Spin coherence and Humpty-Dumpty. III. The effects of observation, Phys. Rev. A 40, 1775 (1989).
  50. M. W. Doherty, N. B. Manson, P. Delaney, F. Jelezko, J. Wrachtrup, and L. C. Hollenberg, The nitrogen-vacancy colour centre in diamond, Phys. Rep. 528, 1 (2013).
  51. U. Delić, M. Reisenbauer, K. Dare, D. Grass, V. Vuletić, N. Kiesel, and M. Aspelmeyer, Cooling of a levitated nanoparticle to the motional quantum ground state, Science 367, 892 (2020).
  52. J. Piotrowski, D. Windey, J. Vijayan, C. Gonzalez-Ballestero, A. de los Ríos Sommer, N. Meyer, R. Quidant, O. Romero-Isart, R. Reimann, and L. Novotny, Simultaneous ground-state cooling of two mechanical modes of a levitated nanoparticle, Nat. Phys. 19, 1009 (2023).
  53. M. Kamba, R. Shimizu, and K. Aikawa, Nanoscale feedback control of six degrees of freedom of a near-sphere, Nat. Commun. 14, 7943 (2023).
  54. D. S. Bykov, L. Dania, F. Goschin, and T. E. Northup, 3D sympathetic cooling and detection of levitated nanoparticles, Optica 10, 438 (2023).
  55. M. Perdriat, C. C. Rusconi, T. Delord, P. Huillery, C. Pellet-Mary, A. Durand, B. A. Stickler, and G. Hétet, Rotational locking of charged microparticles in quadrupole ion traps, Phys. Rev. Lett. 133, 253602 (2024).
  56. J.-F. Hsu, P. Ji, C. W. Lewandowski, and B. D’Urso, Cooling the motion of diamond nanocrystals in a magneto-gravitational trap in high vacuum, Sci. Rep. 6, 30125 (2016).
  57. We use the terms decoherence and dephasing interchangeably in this paper—We are referring to the phase accumulated due to stochastic noise in the environment that enters the phase measurement and affects the subsequent averaging over experimental runs.
  58. S. A. Hughes and K. S. Thorne, Seismic gravity-gradient noise in interferometric gravitational-wave detectors, Phys. Rev. D 58, 122002 (1998).
  59. P. R. Saulson, Terrestrial gravitational noise on a gravitational wave antenna, Phys. Rev. D 30, 732 (1984).
  60. K. S. Thorne and C. J. Winstein, Human gravity-gradient noise in interferometric gravitational-wave detectors, Phys. Rev. D 60, 082001 (1999).
  61. J. Harms, Terrestrial gravity fluctuations, Liv. Rev. Relativ. 22, 6 (2019).
  62. M.-Z. Wu, Acceleration noise induced decoherence in Stern-Gerlach interferometers for gravity experiments, Phys. Rev. Res. 8, 023115 (2026).
  63. The choice of the mass is based on the QGEM experiment (see Refs. [64, 65]). We can vary the mass in our analysis.
  64. M. Schut, A. Geraci, S. Bose, and A. Mazumdar, Micrometer-size spatial superpositions for the QGEM protocol via screening and trapping, Phys. Rev. Res. 6, 013199 (2024).
  65. M. Schut and A. Mazumdar, Parameter scanning in a quantum-gravity-induced entanglement of masses (QGEM) experiment with electromagnetic screening, arXiv:2502.12474.
  66. J. S. Pedernales, G. W. Morley, and M. B. Plenio, Motional dynamical decoupling for interferometry with macroscopic particles, Phys. Rev. Lett. 125, 023602 (2020).
  67. R. J. Marshman, A. Mazumdar, R. Folman, and S. Bose, Constructing nano-object quantum superpositions with a Stern-Gerlach interferometer, Phys. Rev. Res. 4, 023087 (2022).
  68. The dependence of Bxj on the interferometer arm accounts for nonuniform magnetic fields of the form Bx≃B0+η1x.
  69. S⃗·B⃗ term gives rise to a spin-dependent potential. This allows for entangling spin and position degrees of freedom, thus creating the two arms of the interferometer.
  70. A. Gruber, A. Dräbenstedt, C. Tietz, L. Fleury, J. Wrachtrup, and C. von Borczyskowski, Scanning confocal optical microscopy and magnetic resonance on single defect centers, Science 276, 2012 (1997).
  71. The orientation of the NV axis and the biased magnetic field are taken to be along the interferometer axis to avoid precession. This allows us to assume one-dimensional dynamics for the present analysis.
  72. P. Storey and C. Cohen-Tannoudji, The Feynman path integral approach to atomic interferometry. A tutorial, J. Phys. II 4, 1999 (1994).
  73. R. P. Feynman and A. R. Hibbs, Quantum Mechanics and Path Integrals, International Series in Pure and Applied Physics (McGraw-Hill, New York, 1965).
  74. In Eq. (11), δxj2 is the fluctuation in xj2, not the square of the first-order fluctuation.
  75. P. W. Bowen and J. G. Milburn, Quantum Optomechanics (CRC Press, Boca Raton, 2015).
  76. N. Wiener, Generalized harmonic analysis, Acta Math. 55, 117 (1930).
  77. A. Khintchine, Korrelationstheorie der stationären stochastischen prozesse, Math. Ann. 109, 604 (1934).
  78. The notation we use is δζ̃τ̃(ω)=12π∫−τ̃τ̃δζ(t)eiωtdt.
  79. We note that the units of the effective transfer functions are the inverse of that of the power spectral density. The units of the PSD depend only on the parameter being perturbed, δζ(t)/noise source.
  80. The Fourier space contains positive and negative frequencies. Mathematically, both are required to describe an arbitrary complex function in the time domain. To obtain a real function in the time domain, the Fourier conjugate must follow ζ̃(−ω)=ζ̃*(ω). Thus, the negative-frequency components are not independent.
  81. xj+δxj is the trajectory obtained from the equations of motion derived from the modified Lagrangian, Lj+δLj.
  82. Correlation of noise statistics between the two arms will contribute to dephasing. It is likely that the two arms will have correlated noise statistics since the source of fluctuation is the same. If we assume that the noise source is far from the interferometer compared to the distance between the interferometer arms, then the correlation is likely positive, leading to a decrease in the dephasing rate. However, we are not dealing with any particular model for the noise source, and hence compute the dephasing for the uncorrelated case to obtain the upper bound on the dephasing rate, given the system parameters. Refer to Appendix pp2. For noise analysis of completely correlated acceleration fluctuations, refer to Ref. [62].
  83. For several fluctuation sources {δζj}j=1n, with individual dephasing rates Γj, the total dephasing can be conservatively bounded without assuming decorrelation by applying the triangle inequality to the corresponding phase fluctuations: Γ≤∑j=1nΓj2.
  84. Recall that Cj=(Sxjℏγe−χρmμ0B0) and C̃j=Cjη0−macosθ0. We note that in the term Cj, −(χρm/μ0)B0 term is order of 2 times greater than Sxjℏγe. Further, the former is interferometer arm independent, while the latter is interferometer arm dependent. Hence, minimizing C̃j in Eq. (7) corresponds to tuning macosθ0 to cancel the contribution of −(χρm/μ0)B0. Physically, this occurs because the spin-independent magnetic force [−(χρm/μ0)B0η0] can be tuned to cancel the effective inertial force (masinθ0), yielding the net force along the interferometer axis to arise only from spin-dependent force Sxjℏγeη0.
  85. A coherence measure of CM=0.9 corresponds to Γτ∼0.1.
  86. C. Timberlake, G. Gasbarri, A. Vinante, A. Setter, and H. Ulbricht, Acceleration sensing with magnetically levitated oscillators above a superconductor, Appl. Phys. Lett. 115, 224101 (2019).
  87. C. W. Lewandowski, T. D. Knowles, Z. B. Etienne, and B. D’Urso, High-sensitivity accelerometry with a feedback-cooled magnetically levitated microsphere, Phys. Rev. Appl. 15, 014050 (2021).
  88. F. Monteiro, W. Li, G. Afek, C.-L. Li, M. Mossman, and D. C. Moore, Force and acceleration sensing with optically levitated nanogram masses at microkelvin temperatures, Phys. Rev. A 101, 053835 (2020).
  89. F. Monteiro, S. Ghosh, A. G. Fine, and D. C. Moore, Optical levitation of 10-ng spheres with nano-g acceleration sensitivity, Phys. Rev. A 96, 063841 (2017).
  90. M. Armano et al., Sub-femto-g free fall for space-based gravitational wave observatories: LISA Pathfinder results, Phys. Rev. Lett. 116, 231101 (2016).
  91. A. Allocca et al., Picoradiant tiltmeter and direct ground tilt measurements at the Sos Enattos site, Eur. Phys. J. Plus 136, 1069 (2021).
  92. S. Narasimha Moorthy, A. Geraci, S. Bose, and A. Mazumdar, Data and related Python codes, GitHub, 2026, https://github.com/SciPhyl-Sneha/Acceleration_and_tilt-angle_fluctuations.

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