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arXiv:2610.38840

Gravitationally Mediated Entanglement in Interferometers with Repeated Splitting

Riccardo Zampieri, Sougato Bose

quant-phSubmitted Oct 28, 2026• Announced Oct 30, 2026• 0 citations
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Abstract

Proposals to probe the quantum nature of gravity through entanglement between spatially separated masses have attracted considerable interest. In such schemes, spatial superpositions are prepared through controlled splitting operations that produce several interferometric branches. Here we propose and analyse protocols involving repeated splitting stages, each of which doubles the number of occupied paths. We show that the density matrix after $n$ splitting stages is related to that of the $(n-1)$-splitting protocol through local parity dephasing. Two of the resulting sectors reproduce the preceding state, while the other two acquire additional gravitational phases. Removing the locally generated parts gives an exact lower bound on the change in negativity, expressed in terms of the preceding state's negative partial-transpose eigenspace. For two splitting stages, this leads to an explicit condition on three gravitational phases under which the additional split cannot reduce negativity. We also show that further splitting cannot shorten the lifetime of the generated entanglement. If the local internal system preserves the full branch label, the positional entanglement is retained upon recombination. We describe an implementation using a reusable two-level system and local memories, and compare it with a readout without a memory register. For the latter, we derive an exact condition for when an additional splitting stage improves the readout, based on a $2\times 2$ Schur complement. Numerical simulations show an advantage in positional negativity over the rates considered, with an improvement surviving the restricted readout at all decoherence rates considered at the final readout time.

AI Summary

The paper asks whether repeated binary splitting of two spatially superposed masses can improve gravity-mediated entanglement, and how much survives recombination. It models diagonal Newtonian interactions along finite-duration interferometer trajectories, with independent, separation-dependent local dephasing. Local parity dephasing decomposes the $n$-stage state into four equally weighted sectors: two reproduce the preceding protocol at the same time, while two acquire additional gravitational phases. Removing local phases and applying the variational characterization of negativity gives a sufficient non-decrease witness using the parent state's negative partial-transpose eigenspace. Independently, $\mathcal N(\rho_n(t))\ge\tfrac12\mathcal N(\rho_{n-1}(t))$, so another split cannot eliminate existing negativity within this model. For two stages and an entangled parent with $0<\Phi_1<2\pi$, a sufficient non-decrease condition is $\sin(\Phi_+/2)+\sin(\Phi_-/2)\ge2\sin(\Phi_1/2)$. A local internal register retaining all $2^n$ branch labels preserves branch-space negativity upon ideal recombination. Without memory, the selected two-qubit readout is probabilistic; improvement in conditioned negativity is characterized exactly through a $2\times2$ Schur complement. In an illustrative simulation at $10$ s and dephasing rate $0.030\,\mathrm{s}^{-1}$, a second split increases branch-space negativity from $0.02199$ to $0.16978$, and conditioned readout negativity to $0.06489$, with success probability $0.06081$. The comparison uses chosen rather than optimized geometries and phenomenological decoherence rates. It omits control imperfections, recombination misalignment, technical noise, and residual electromagnetic interactions, and assumes fast recombination. The stated magnetic gradients remain experimentally challenging; conditioned entanglement gains do not directly establish improved experimental yield.

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21 pages, 3 figures

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Proposals to probe the quantum nature of gravity through entanglement between spatially separated masses have attracted considerable interest. In such schemes, spatial superpositions are prepared through controlled splitting operations that produce several interferometric branches. Here we propose and analyse protocols involving repeated splitting stages, each of which doubles the number of occupied paths. We show that the density matrix after nnn splitting stages is related to that of the (n−1)(n-1)(n−1)-splitting protocol through local parity dephasing. Two of the resulting sectors reproduce the preceding state, while the other two acquire additional gravitational phases. Removing the locally generated parts gives an exact lower bound on the change in negativity, expressed in terms of the preceding state's negative partial-transpose eigenspace. For two splitting stages, this leads to an explicit condition on three gravitational phases under which the additional split cannot reduce negativity. We also show that further splitting cannot shorten the lifetime of the generated entanglement. If the local internal system preserves the full branch label, the positional entanglement is retained upon recombination. We describe an implementation using a reusable two-level system and local memories, and compare it with a readout without a memory register. For the latter, we derive an exact condition for when an additional splitting stage improves the readout, based on a 2×22\times 22×2 Schur complement. Numerical simulations show an advantage in positional negativity over the rates considered, with an improvement surviving the restricted readout at all decoherence rates considered at the final readout time.
The paper asks whether repeated binary splitting of two spatially superposed masses can improve gravity-mediated entanglement, and how much survives recombination. It models diagonal Newtonian interactions along finite-duration interferometer trajectories, with independent, separation-dependent local dephasing.
Local parity dephasing decomposes the nnn-stage state into four equally weighted sectors: two reproduce the preceding protocol at the same time, while two acquire additional gravitational phases. Removing local phases and applying the variational characterization of negativity gives a sufficient non-decrease witness using the parent state's negative partial-transpose eigenspace. Independently, N(ρn(t))≥12N(ρn−1(t))\mathcal N(\rho_n(t))\ge\tfrac12\mathcal N(\rho_{n-1}(t))N(ρn​(t))≥21​N(ρn−1​(t)), so another split cannot eliminate existing negativity within this model. For two stages and an entangled parent with 0<Φ1<2π0<\Phi_1<2\pi0<Φ1​<2π, a sufficient non-decrease condition is sin⁡(Φ+/2)+sin⁡(Φ−/2)≥2sin⁡(Φ1/2)\sin(\Phi_+/2)+\sin(\Phi_-/2)\ge2\sin(\Phi_1/2)sin(Φ+​/2)+sin(Φ−​/2)≥2sin(Φ1​/2).
A local internal register retaining all 2n2^n2n branch labels preserves branch-space negativity upon ideal recombination. Without memory, the selected two-qubit readout is probabilistic; improvement in conditioned negativity is characterized exactly through a 2×22\times22×2 Schur complement. In an illustrative simulation at 101010 s and dephasing rate 0.030 s−10.030\,\mathrm{s}^{-1}0.030s−1, a second split increases branch-space negativity from 0.021990.021990.02199 to 0.169780.169780.16978, and conditioned readout negativity to 0.064890.064890.06489, with success probability 0.060810.060810.06081.
The comparison uses chosen rather than optimized geometries and phenomenological decoherence rates. It omits control imperfections, recombination misalignment, technical noise, and residual electromagnetic interactions, and assumes fast recombination. The stated magnetic gradients remain experimentally challenging; conditioned entanglement gains do not directly establish improved experimental yield.
This work presents an explicit Newtonian gravitational phase model for two masses placed in spatial superposition and demonstrates that the resulting phase structure produces a non-zero plaquette invariant. Numerical simulations show that the plaquette phase scales with branch separation, generates entanglement according to analytic mappings, and vanishes under loop-removal kill tests. These results provide a fully operational demonstration that Newtonian gravitational phase accumulation produces the non-factorable loop structure required for gravity-mediated entanglement.
We present a falsifiable framework for generating and detecting path entanglement mediatedby Newtonian gravity between two mesoscopic masses using pure motional interferometry. Eachmass is prepared in a spatial superposition of two paths with separation ∆x, the pair is heldfor an interaction time T at mean separation r, and then recombined locally. The gravita-tional interaction imprints branch-dependent phases ϕij = (Gm1m2T /ℏ) r−1ij on the four branches(i, j) ∈ {+, −}2, yielding a two-qubit controlled-phase operation whose gauge-invariant nonlocalphase is ∆ϕ = ϕ++ + ϕ−− − ϕ+− − ϕ−+ = (Gm1m2T /ℏ)(r−1++ + r−1−− − r−1+− − r−1−+). For a symmet-ric r ± ∆x geometry, ∆ϕ = (Gm2T /ℏ)(2/r − 1/(r + ∆x) − 1/(r − ∆x)) ≈ −2Gm2T ∆x2/(ℏr3) for∆x ≪ r. We show how ∆ϕ(r, ∆x, T ) appears as a geometry-modulated template in joint outputstatistics after recombination, and we formulate an inference protocol based on (i) template regres-sion across controlled modulations of r, ∆x, T and (ii) independent bounds and control experimentsthat constrain nongravitational interactions below the fitted template amplitude. Because the oper-ating point of interest can lie in the weak-phase regime (|∆ϕ| ≪ 1), we treat Bell-inequality violationas optional rather than primary; the escalation to an entanglement claim is framed in terms of ex-perimentally accessible two-qubit witnesses obtained from multi-basis correlation measurements onthe path degrees of freedom, together with a quantitative “no-template-match” falsifier.
This note studies the role of a quantum mediator in gravitationally induced entanglement and decoherence using an exactly solvable dynamical mediator model. Two masses in spatial superposition interact through a mediator mode described by a displaced-oscillator Hamiltonian. The model provides a unified description of two regimes: when the mediator returns to its original state, it leaves behind pure entanglement between the masses through virtual excitation; when the mediator carries which-path information, it becomes a physical record that reduces coherence and suppresses entanglement. The work proves an exact record–decoherence relation: the loss of coherence of each subsystem equals the information stored in the rest of the universe, combining entanglement generation and decoherence into a single information budget. The paper also establishes a classical-channel dichotomy. A measure-and-feedforward channel calibrated to reproduce the same interaction produces no entanglement, while introducing additional noise. This provides an exact solvable distinction between a genuinely quantum mediator and a classical communication channel. The causal structure of mediation is studied in a multi-mode chain, where entanglement appears only after the mediator excitation reaches the relevant region, establishing a finite propagation constraint in the model. The work also proves analytically the separability boundary for partially coherent sources, including the condition relating source coherences required for entanglement generation. The results provide an exactly solvable framework connecting gravitationally induced entanglement, mediator quantum information, which-path records, decoherence, and quantum versus classical mediation. The declared limits are finite models, linear mediator coupling, and no claim of a complete theory of dynamical quantum gravity. Verification and reproducibility materials are included.
Recently, a protocol called quantum-gravity-induced entanglement of masses (QGEM) that aims to test the quantum nature of gravity using the entanglement of two qubits was proposed. The entanglement can arise only if the force between the two spatially superposed masses is occurring via the exchange of a mediating virtual graviton. In this paper we examine a possible improvement of the QGEM setup by introducing a third mass with an embedded qubit so that there are now three qubits to witness the gravitationally generated entanglement. We compare the entanglement generation for different experimental setups with two and three qubits and find that a three-qubit setup where the superpositions are parallel to each other leads to the highest rate of entanglement generation within $\ensuremath{\tau}=5\phantom{\rule{4pt}{0ex}}\mathrm{s}$. We show that the three-qubit setup is more resilient to the higher rate of decoherence. The entanglement can be detected experimentally for the two-qubit setup if the decoherence rate $\ensuremath{\gamma}$ is $\ensuremath{\gamma}<0.11\phantom{\rule{4pt}{0ex}}\mathrm{Hz}$ compared to $\ensuremath{\gamma}<0.16\phantom{\rule{4pt}{0ex}}\mathrm{Hz}$ for the three-qubit setup. However, the introduction of an extra qubit means that more measurements are required to characterize entanglement in an experiment. We conduct experimental simulations and estimate that the three-qubit setup would allow detecting the entanglement in the QGEM protocol at a 99.999.9%99.9 certainty with O(104)−−O(105)O({10}^{4})--O({10}^{5})O(104)−−O(105) measurements when $\ensuremath{\gamma}\ensuremath{\in}[0.1,0.15]\phantom{\rule{4pt}{0ex}}\mathrm{Hz}$. Furthermore, we find that the number of needed measurements can be reduced to O(103)−−O(105)O({10}^{3})--O({10}^{5})O(103)−−O(105) if the measurement schedule is optimized using joint Pauli basis measurements. For $\ensuremath{\gamma}>0.06\phantom{\rule{4pt}{0ex}}\mathrm{Hz}$ the three-qubit setup is favorable compared to the two-qubit setup in terms of the minimum number of measurements needed to characterize the entanglement. Thus, the proposed setup here provides a promising avenue for implementing the QGEM experiment.
We show that gravitational curvature can control the generation of nonlocal quantum correlations in a hybrid qubit-mechanical device. The tidal field of a nearby source mass modifies the susceptibility of a shared mechanical oscillator, thereby tuning an oscillator-mediated qubit-qubit interaction and the resulting entangling phase. An exact treatment of the dynamics reveals stroboscopic geometric gates whose accumulated phase is directly sensitive to gravitational curvature. Treating the curvature as an unknown parameter, we derive the ultimate quantum limit for its estimation and identify a parity-based measurement that saturates this bound. Solving the full master equation with the mechanical mode retained explicitly, we find that thermal occupation of the mediator suppresses entanglement between the closure times but is undone at each closure, exactly in the unitary limit for any initial mechanical temperature, so that ground-state cooling of the oscillator is not a prerequisite for the protocol. Mechanical damping and qubit dephasing behave differently: they leak branch information irreversibly to the environment, and it is the heating and dephasing rates, rather than the bath occupation alone, that limit the entanglement visibility and the number of usable interrogation loops. In contrast to gravity-mediated entanglement proposals, entanglement is generated by the mechanical oscillator while gravity acts solely as a classical control field. We quantify the achievable curvature parameters; all curvature dependencies are analytic, allowing for exact rescaling of the results. The scheme therefore demonstrates gravitational control of a quantum interaction and provides a route to curvature sensing based on a nonlocal two-qubit phase rather than on local phase measurements.
Abstract Witnessing the quantum nature of gravity through the entanglement of two masses has recently been proposed. Both non-Gaussian and Gaussian protocols have been shown to be useful for this purpose. In non-Gaussian protocols the complete 1 / r gravitational interaction can in principle be utilized for entanglement generation, as long as quantum superpositions of a spatial splitting Δ x comparable to the distance d between two masses can be generated. In practice, however, all non-Gaussian protocols proposed to date rely on embedded qubits—typically spins—to read out the entanglement: spin correlations are used to witness the entanglement developed between the masses during interferometry. Here we show that if superpositions of distinct spatially localized states of each mass can be created, then a spinless version of the non-Gaussian protocol is possible: simple position correlation measurements alone can yield a spatial qubit witness of the entanglement between the masses. We find that the principal new requirement for the viability of this protocol is a position squeezing of the wavefunction by approximately seven orders of magnitude, applied at a specific stage of the experiment.