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This study optimizes matter-wave interferometer geometries to maximize the detection of gravitationally induced entanglement, demonstrating that specific parallel-arm configurations significantly outperform standard setups in phase accumulation and robustness against fabrication errors. By deriving exact analytical expressions for gravitational phases, the authors provide a critical design framework for near-term experiments aiming to probe the quantum nature of gravity.
Source coveringarXiv

Improving Gravitationally Induced Entanglement in Interferometric Configurations

arXiv3 min read

arXiv:2611.07153v1 Announce Type: new Abstract: Proposals to detect gravitationally induced entanglement between massive particles offer a promising pathway toward probing the quantum nature of gravity. We perform a systematic geometric optimization and comparative analysis of Stern--Gerlach (SG) and Mach--Zehnder (MZ) matter-wave interferometers for this purpose, deriving exact analytical expressions for the gravitational phase of each configuration. Our first key result is that geometric optimization is indispensable. For commonly assumed experimental parameters, neglecting the optimization of geometric ratios can suppress the accumulated phase, and hence the detectability of entanglement, by up to several orders of magnitude. Second, we provide a complete comparative analysis of two SG orientations (linear and parallel) and three MZ orientations (translation-symmetric, mirror-symmetric, and parallel-arms). The parallel-arms SG and MZ configurations tend to yield the largest phase accumulations and are nearly equivalent in performance, whereas the translation-symmetric MZ setup exhibits destructive-interference nulls that act as blind operating points where detection becomes ineffective. These observations highlight the importance of geometry-aware design. A Monte Carlo error analysis of realistic fabrication tolerances indicates that the parallel-arms configurations are generally more robust, maintaining low relative phase uncertainty over broad parameter intervals. Furthermore, an evaluation of Bell violations assesses the feasibility and signal-to-noise ratio of each configuration. Our results identify geometric optimization, particularly through parallel-arms designs, as an important consideration for near-term experiments targeting gravitationally induced entanglement.

Abstract:Proposals to detect gravitationally induced entanglement between massive particles offer a promising pathway toward probing the quantum nature of gravity. We perform a systematic geometric optimization and comparative analysis of Stern--Gerlach (SG) and Mach--Zehnder (MZ) matter-wave interferometers for this purpose, deriving exact analytical expressions for the gravitational phase of each configuration. Our first key result is that geometric optimization is indispensable. For commonly assumed experimental parameters, neglecting the optimization of geometric ratios can suppress the accumulated phase, and hence the detectability of entanglement, by up to several orders of magnitude. Second, we provide a complete comparative analysis of two SG orientations (linear and parallel) and three MZ orientations (translation-symmetric, mirror-symmetric, and parallel-arms). The parallel-arms SG and MZ configurations tend to yield the largest phase accumulations and are nearly equivalent in performance, whereas the translation-symmetric MZ setup exhibits destructive-interference nulls that act as blind operating points where detection becomes ineffective. These observations highlight the importance of geometry-aware design. A Monte Carlo error analysis of realistic fabrication tolerances indicates that the parallel-arms configurations are generally more robust, maintaining low relative phase uncertainty over broad parameter intervals. Furthermore, an evaluation of Bell violations assesses the feasibility and signal-to-noise ratio of each configuration. Our results identify geometric optimization, particularly through parallel-arms designs, as an important consideration for near-term experiments targeting gravitationally induced entanglement.

arXiv:2611.07153 [quant-ph]

(or arXiv:2611.07153v1 [quant-ph] for this version)

https://doi.org/10.48550/arXiv.2611.07153 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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Full text under the publisher's open licence · 310 words

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