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On inference of quantization from gravitationally induced entanglement (2206.00558v2)

Published 1 Jun 2022 in quant-ph and gr-qc

Abstract: Observable signatures of the quantum nature of gravity at low energies have recently emerged as a promising new research field. One prominent avenue is to test for gravitationally induced entanglement between two mesoscopic masses prepared in spatial superposition. Here we analyze such proposals and what one can infer from them about the quantum nature of gravity, as well as the electromagnetic analogues of such tests. We show that it is not possible to draw conclusions about mediators: even within relativistic physics, entanglement generation can equally be described in terms of mediators or in terms of non-local processes -- relativity does not dictate a local channel. Such indirect tests therefore have limited ability to probe the nature of the process establishing the entanglement as their interpretation is inherently ambiguous. We also show that cosmological observations already demonstrate some aspects of quantization that these proposals aim to test. Nevertheless, the proposed experiments would probe how gravity is sourced by spatial superpositions of matter, an untested new regime of quantum physics.

Summary

  • The paper demonstrates that gravitationally induced entanglement arises from non-relativistic quantum mechanics, challenging definitive proof of graviton quantization.
  • It compares local mediator roles in the Lorentz gauge with non-local Coulomb gauge formulations, highlighting key methodological differences.
  • The study implies that while GIE experiments confirm quantum features of Newtonian potentials, they do not decisively establish graviton mediation.

On Inference of Quantization from Gravitationally Induced Entanglement

Introduction

The paper of quantum gravity seeks to reconcile quantum mechanics with general relativity. A promising avenue is gravitationally induced entanglement (GIE), which involves testing gravitational fields' quantum nature through two masses prepared in spatial superposition. The interaction of these masses via a Newtonian gravitational potential might entangle their quantum states, supposedly hinting at quantum gravity. This essay investigates whether such experiments unambiguously indicate quantum gravity, or more specifically, the existence of gravitons as mediators, and examines analogous tests in electromagnetism.

Non-relativistic Quantum Mechanics

In quantum mechanics, the gravitational potential can be expressed as an operator owing to the quantized nature of its sources, such as masses in superposition. For two interacting particles, the Hamiltonian includes their kinetic and potential energy terms. However, given this setup, conclusions regarding mediators' nature remain elusive; gravitons do not manifest in this framework. Consequently, this non-relativistic limit suffices to predict GIE proposals, highlighting the inherently non-local nature of Newtonian interactions.

Electromagnetic Field Propositions

Local Mediators in Lorentz Gauge:

In QED's Lorentz gauge, all components of the electromagnetic field are quantized, localizing the interaction Lagrangian. The presence of scalar and longitudinal "virtual" photons here facilitates entanglement yet is unobservable directly. These mediators are responsible for local interaction, meaning entanglement and local operations demand that these auxiliary fields are quantized. Figure 1

Figure 1: Schematic of an experimental setup to test for gravitationally induced entanglement.

Non-locality in Coulomb Gauge:

In contrast, Coulomb gauge formulations highlight non-local entanglement generation, bypassing mediators. The interaction Hamiltonian involves merely the Coulomb potential, emphasizing direct entanglement without traversing quantized fields. This renders LOCC arguments ineffectual for proving quantized mediators, revealing that the locality requirement isn't strictly necessary for entanglement given relativistic causality.

QED as Absorber Theory:

For further ambiguity resolution, considering absorber formulations such as Wheeler-Feynman's, where interactions have non-local character without fields, aligns with QED predictions. Indirect inferences from LOCC fail here, and the gravitational analogue faces similar issues.

Weak-field Quantum Gravity

Local Mediators in Lorentz Gauge:

In gravity's weak-field limit, quantum gravity parallels electromagnetic methods, with auxiliaries arising in Lorentz gauge quantization. Although auxiliary gravitons mediate entanglement, they, too, elude direct observation, echoing QED's dynamics without assuring graviton quantization.

Non-local Alternatives and Absorber Theories:

Poisson gauge formulations of gravity underscore non-local entanglement minus quantized mediators' necessity. Coupled with potential gravitational absorber theories in weak fields, these show further ambiguity in any definite quantization conclusion. However, this framework currently lacks a non-perturbative general relativity form.

Implications of GIE Experiments

The inferences from GIE tests are mainly ambiguous due to alternative theoretical formulations. Directly, successful GIE probes show masses in superposition source Newtonian fields, allowing further conclusions contingent on prior theoretical suppositions. Pre-existing cosmological evidence already points toward the quantum nature of gravity in similar contexts. Figure 2

Figure 2: Left: Bronstein cube organizing various theories based on dependence on ,G\hbar, G, and cc.

Conclusion

GIE experiments, while revolutionary in potentially capturing quantum gravitational phenomenon, offer limited insights beyond proving the quantum mechanical nature of Newtonian potentials sourced by superposed masses. Graviton quantization is not verifiable without presuming specific local interactions, as alternatives exist for non-local processes consistent with known physics and current cosmological understandings. Thus, even successful GIE results might inform existing assumptions more than unearth novel explanations or affirm the quantization of gravitational interactions definitively.

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Knowledge Gaps

Knowledge gaps, limitations, and open questions

Below is a concise list of unresolved issues, ambiguities, and missing analyses that the paper identifies or implies—articulated so future work can directly address them.

  • Lack of an absorber-type formulation of full (nonlinear) general relativity: Is there a consistent Wheeler–Feynman–style, action-at-a-distance theory for gravity beyond the relativistic weak-field limit, and can it be quantized (canonically or via path integrals) without introducing gravitational field degrees of freedom?
  • Experimental indistinguishability of ontologies: What concrete experimental protocol (if any) could empirically distinguish (i) local, quantized mediators, (ii) non-local but still relativistic formulations (e.g., Coulomb-type), and (iii) absorber theories, when testing gravitationally induced entanglement?
  • Mediation channel diagnosis in gravity: In linearized gravity, which gauge components (transverse-traceless vs scalar/longitudinal) actually carry the near-field entangling interaction, and can a measurable signature isolate (or rule out) contributions from physical gravitons?
  • Regimes where real radiation matters: What parameter ranges (masses, separations, interaction times) push GIE-like experiments beyond the near-field regime such that on-shell radiation (photons/gravitons), radiation reaction, or memory effects measurably contribute to (or modify) entanglement?
  • Operational LOCC in gauge theories: How should “local operations and classical communication” be rigorously defined in constrained relativistic gauge theories so that the LOCC no-entanglement theorem can be applied without gauge-ambiguity?
  • Causality proofs for gravity analogs: The paper discusses causal consistency for EM non-local formulations; an explicit, gravity-analog derivation (showing retarded, gauge-invariant fields emerge from seemingly instantaneous constraints) is missing.
  • Path-integral unification with constraints: A full path-integral treatment that cleanly connects the nonrelativistic Newtonian operator potential, different gauge choices in linearized gravity, and absorber-like non-local actions—clarifying what is assumed at each step—remains to be provided.
  • Canonical quantization of non-local actions: For action-at-a-distance formulations (EM and gravity), provide a complete canonical quantization framework (beyond toy or perturbative limits) that ensures unitarity, causality, and a well-defined Hamiltonian.
  • Cosmological inference of coherent sourcing: The claim that cosmological observations already demonstrate coherent sourcing of Newtonian fields by quantum superpositions needs a precise mapping—what specific observables (e.g., CMB two-point/phase correlations, squeezed states) imply this, under what assumptions, and with what robustness to alternative classical or semiclassical models?
  • Discriminating GIE from semiclassical or collapse models: Develop explicit, falsifiable predictions (beyond mean-field failures) for semiclassical gravity and objective collapse theories in the GIE regime, including noise budgets and witness statistics that can rule them out.
  • Direct measurability of the Newtonian field operator: Propose operational schemes to probe the operator nature of the Newtonian potential (e.g., field tomography via probe superpositions) rather than inferring it indirectly from two-body entanglement.
  • Gravitational gauge-fixing dependence: Perform explicit, side-by-side calculations of entanglement generation in linearized gravity under different gauges to quantify which features are gauge artifacts and which are gauge-invariant (and potentially observable).
  • Near-field vs retarded-field crossovers: Provide quantitative criteria and scaling laws for when retardation, post-Newtonian corrections, or radiative modes become non-negligible in mesoscopic GIE experiments, and how these modify the entanglement phase and witness outcomes.
  • Soft-graviton/memory observables in tabletop setups: Assess whether gravitational memory or soft-theorem-related signatures could be leveraged in modified GIE protocols to access genuinely radiative (and hence mediator-specific) gravitational effects.
  • Robust entanglement witnesses under realistic noise: Derive witnesses or protocols that remain conclusive in the presence of dominant non-gravitational couplings (residual EM, Casimir–Polder, patch potentials), motional decoherence, and thermal noise, and quantify their discriminating power against alternative channels.
  • Resource accounting under different ontologies: In an information-theoretic framework, characterize the “resource” cost (e.g., communication, ancillary systems) of establishing entanglement in local-mediator vs non-local-interaction vs absorber pictures, and identify any operational differences that could lead to testable distinctions.
  • Gravitational time-dilation effects in GIE: Systematically include relativistic time-dilation and internal energy contributions (mass–energy equivalence) in GIE calculations to determine whether they produce measurable corrections or confounds to the entangling phase.
  • Multi-body and networked GIE: Extend the theory from two-body setups to many-body or networked superpositions to see if higher-order correlations, monogamy constraints, or entanglement structure can reveal features of the underlying channel not visible in two-body experiments.
  • Explicit second-order calculations in gravity: Provide complete perturbative calculations (analogous to the EM oscillator example) for gravitationally coupled systems that include all intermediate matter and field states, clarifying whether omissions change conclusions about the “mediator” role.
  • Cosmological boundary conditions for gravitational absorber theories: If a gravitational absorber theory is to be viable, specify the necessary cosmological boundary conditions (e.g., in expanding spacetimes with dark energy) and test whether they are compatible with observations.
  • Post-Newtonian corrections to entanglement witness thresholds: Compute how 1PN/2PN corrections shift the maximally entangling phases, interaction times, or separations, and whether these corrections could mimic or mask signatures ascribed to mediator quantization.
  • Equivalence principle in superpositions: Analyze whether coherent sourcing by quantum superpositions induces any measurable deviations or subtleties in equivalence-principle tests, and propose GIE-adjacent experiments to probe them.
  • Clear no-go/yes-go criteria for mediator inference: Formulate precise axiomatic conditions under which observing entanglement does imply quantized mediators, and identify which assumptions (locality, microcausality, gauge structure) are indispensable vs optional.
  • Practical routes to suppress EM confounds below gravity: Provide a concrete engineering roadmap (materials, charge control, shielding, trap design) with quantified targets ensuring that EM and other non-gravitational interactions remain subdominant to gravitationally induced entanglement in realistic deployments.
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