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Fig. 2.

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Top: Gravitational potential sourced by the axial-symmetric contribution ⟨|ψ|2Φ = ⟨|ψ|2⟩ of the wave function depicted in Fig. 1. Bottom: Relative importance of the potential perturbation sourced by the interference term alone. Neglecting the latter in the computation of the total potential in Eq. (1b) only incurs 𝒪(1 − 10%) errors.

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