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This paper proposes an experimental protocol within relativistic de Broglie-Bohm theory to detect a preferred foliation of spacetime using arrival-time distributions in EPRB-type experiments. If validated, such a signature would challenge the conventional view that quantum equilibrium renders this hidden structure empirically undetectable and could imply superluminal signaling. The work sits at the intersection of foundational quantum mechanics and relativistic constraints rather than addressing practical AI or quantum computing applications.
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Arrival-time distributions as a probe of the preferred foliation in relativistic Bohmian mechanics

arXiv2 min read

arXiv:2604.17507v2 Announce Type: replace Abstract: Relativistic extensions of de Broglie-Bohm theory postulate a preferred foliation of space-time, an additional structure essential for defining simultaneous configurations on Minkowski space-time, but conventionally believed to be empirically undetectable at quantum equilibrium. In this paper, we outline an experimental protocol for empirically detecting the preferred foliation, which is assumed to be flat for simplicity. Building on the arrival-time distributions for spin-1/2 particles predicted by Das and D\"urr, we show that in an EPRB-type experiment with spacelike-separated spin and arrival-time measurements, the observed arrival-time statistics will depend crucially on the temporal order of these measurements relative to the preferred foliation of space-time. This dependence offers a potential experimental signature of the preferred foliation postulated by relativistic Bohmian models. Moreover, it implies the possibility of superluminal signaling.

Abstract:Relativistic extensions of de Broglie-Bohm theory postulate a preferred foliation of space-time, an additional structure essential for defining simultaneous configurations on Minkowski space-time, but conventionally believed to be empirically undetectable at quantum equilibrium. In this paper, we outline an experimental protocol for empirically detecting the preferred foliation, which is assumed to be flat for simplicity. Building on the arrival-time distributions for spin-1/2 particles predicted by Das and Dürr, we show that in an EPRB-type experiment with spacelike-separated spin and arrival-time measurements, the observed arrival-time statistics will depend crucially on the temporal order of these measurements relative to the preferred foliation of space-time. This dependence offers a potential experimental signature of the preferred foliation postulated by relativistic Bohmian models. Moreover, it implies the possibility of superluminal signaling.

arXiv:2604.17507 [quant-ph]

(or arXiv:2604.17507v2 [quant-ph] for this version)

https://doi.org/10.48550/arXiv.2604.17507 Focus to learn more arXiv-issued DOI via DataCite

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Full text under the publisher's open licence · 215 words

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