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arXiv:2603.27311 · Physical review. D/Physical review. D.

Time of arrival on a ring and relativistic quantum clocks

Iason Vakondios, Charis Anastopoulos

quant-phhep-thSubmitted Mar 28, 2026• Announced Mar 31, 2026• 0 citations
v1 · Mar 28, 2026v2 · Aug 21, 2026
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Abstract

We study the time-of-arrival problem for relativistic particles constrained to move on a ring, formulating the problem entirely within Quantum Field Theory (QFT). In contrast to its counterpart for motion in a line, the circle topology implies that particles may encounter the detector multiple times before detection, making a field-theoretic treatment of the measurement interaction essential. We employ the Quantum Temporal Probabilities (QTP) method to derive a class of Positive-Operator-Valued Measures (POVMs) for time-of-arrival observables directly from QFT. We analyze the resulting detection probabilities in both semiclassical and fully quantum regimes, identifying the relevant timescales and their dependence on the field-theoretic parameters. For ensembles of particles, the detection signal is a periodic function, providing a realization of a quantum clock whose operation reflects the local spacetime structure. We also extend the formalism to rotating rings and show that rotation induces additional noise in detection probabilities, interpretable as a manifestation of the rotational Unruh effect. Finally, we investigate multi-time measurements and demonstrate the emergence of non-classical temporal correlations due to entanglement.

DOI
10.1103/2dtk-q4wp
Comments
20 pages, 4 figures

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We study the time-of-arrival problem for relativistic particles constrained to move on a ring, formulating the problem entirely within Quantum Field Theory (QFT). In contrast to its counterpart for motion in a line, the circle topology implies that particles may encounter the detector multiple times before detection, making a field-theoretic treatment of the measurement interaction essential. We employ the Quantum Temporal Probabilities (QTP) method to derive a class of Positive-Operator-Valued Measures (POVMs) for time-of-arrival observables directly from QFT. We analyze the resulting detection probabilities in both semiclassical and fully quantum regimes, identifying the relevant timescales and their dependence on the field-theoretic parameters. For ensembles of particles, the detection signal is a periodic function, providing a realization of a quantum clock whose operation reflects the local spacetime structure. We also extend the formalism to rotating rings and show that rotation induces additional noise in detection probabilities, interpretable as a manifestation of the rotational Unruh effect. Finally, we investigate multi-time measurements and demonstrate the emergence of non-classical temporal correlations due to entanglement.
Constructing observables that describe the localization of relativistic particles is an important foundational problem in relativistic quantum field theory (QFT). The description of localization in terms of single-time observables leads to conflict with the requirement of causality. In this paper, we describe particle localization in terms of time-of-arrival observables, defined in terms of the interaction between a quantum field and a measuring apparatus. The resulting probabilities are linear functionals of QFT correlation functions. Specializing to the case of a scalar field, we identify several time-of-arrival observables differing on the way that the apparatus localizes particle-detection records. Maximum localization is obtained for a unique observable that is related to the Newton-Wigner position operator. Finally, we define a measure of localizability for relativistic particles in terms of a novel time-energy uncertainty relation for the variance of the time of arrival.
The definition of time observables in quantum theory remains conceptually unsettled. In nonrelativistic quantum mechanics, Pauli-type arguments obstruct the existence of a self-adjoint time operator conjugate to energy, while in relativistic quantum field theory (QFT) localization, causality, and observer dependence further complicate the notion of time-of-arrival (TOA). Existing approaches—such as POVM-based constructions and detector models—are operationally effective but typically depend on specific measurement schemes or preferred time parameters. This work introduces a relational and manifestly covariant formulation of time-of-arrival in QFT. Rather than postulating a universal time operator, TOA is defined as a field-functional constructed from two conserved structures:(i) a conserved matter current encoding detector crossings, and(ii) a conserved event current whose integral defines a discrete event-count clock. Under controlled coarse-graining, the discrete clock admits a continuum limit described by a scalar clock field governed by an effective field theory (EFT). This provides a unified ultraviolet–infrared hierarchy linking integer-valued event counts to smooth clock readings, while remaining compatible with Hamiltonians bounded from below. A general relational TOA distribution is derived by binning detector flux with respect to the physical clock field evaluated on the detector world-tube. The resulting observable is covariant and independent of detector microphysics up to the detector geometry and matter current. In a worked 1+11+11+1-dimensional example, the TOA distribution appears explicitly as a convolution of the semiclassical matter flux with clock-sector correlations, yielding predictive arrival-time broadening. The variance is fixed by clock fluctuations, while early-arrival contributions are shown to be exponentially suppressed with a scale determined by the clock-sector mass parameter. An appendix derives this exponential envelope from standard massive propagator asymptotics, clarifying the distinction between local (Gaussian) clock noise and nonlocal correlation bounds. A concrete realization motivated by Swirl-String Theory (SST) is presented as an example, identifying the event current with defect worldlines and the clock field with a foliation scalar, though the relational construction itself remains model-independent. The framework isolates a sharpened notion of detector-independence and provides a predictive, falsifiable program for time-of-arrival observables in relativistic quantum theory, with direct applicability to analytical and numerical studies across resolutions. Keywords time of arrival; relational time; quantum time observables; covariant observables; event currents; quantum field theory; effective field theory Notes Single-file LaTeX source (Springer sn-jnl class) Includes worked example and analytic appendix Suitable for Foundations of Physics, Annals of Physics, or related journals License © 2025 Omar Iskandarani.This work is made available for academic reading and citation. Redistribution or derivative works are not permitted without explicit permission. (Adjust if you prefer a Creative Commons license.) Citation O. Iskandarani, Relational Time-of-Arrival as a Covariant Field Observable: From Event Currents to a Continuum Clock Limit, Zenodo (2025).
The formulation of a consistent measurement theory for relativistic quantum fields has become a problem of growing foundational and practical significance. Standard non-relativistic measurement models fail to incorporate the essential relativistic principles of locality, causality, and Lorentz covariance, and are therefore inadequate for quantum field theoretic settings. While most existing work focuses on scalar fields, realistic particles possess spin, polarization, and internal degrees of freedom that introduce new conceptual and operational challenges. To this end, we employ the Quantum Temporal Probabilities (QTP) framework for relativistic measurements to describe electromagnetic, Dirac, and internally structured scalar fields. Our results include probabilities for the time-of-arrival that take spin/polarization into account, generalized photodetection formulas beyond Glauber's theory, an unambiguous derivation of the particle oscillation formula together with its limitations, and a first-principles analysis of relativistic qudits.
We analyze time-of-arrival probability distributions for relativistic particles in the context of quantum field theory (QFT). We show that QFT leads to a unique prediction, modulo post-selection that incorporates properties of the apparatus into the initial state. We also show that an experimental distinction of different probability assignments is possible especially in near-field measurements. We also analyze causality in relativistic measurements. We consider a quantum state obtained by a spacetime-localized operation on the vacuum, and we show that detection probabilities are typically characterized by small transient non-causal terms. We explain that these terms originate from Feynman propagation of the initial operation, because the Feynman propagator does not vanish outside the light cone. We discuss possible ways to restore causality, and we argue that this may not be possible in measurement models that involve switching the field–apparatus coupling on and off.
The question of how to interpret and compute arrival-time distributions in quantum mechanics remains unsettled, reflecting the longstanding tension between treating time as a quantum observable or as a classical parameter. While recent studies have primarily contrasted arrival-time predictions across different interpretations of quantum mechanics, here we investigate this ambiguity within the standard quantum-mechanical framework itself. Moreover, most previous studies have focused on the single-particle case in the far-field regime, where these distinct approaches yield very similar arrival-time distributions and a semi-classical analysis typically suffices. Recent advances in atom-optics technologies now make it possible to experimentally investigate arrival-time distributions for entangled multi-particle systems in the near-field regime, where a deeper analysis beyond semi-classical approximations is required. Even in the far-field regime, due to quantum non-locality, the semi-classical approximation cannot generally hold in multi-particle systems. Therefore, in this work, two fundamental approaches to the arrival-time problem---namely, the time-parameter and time-operator approaches---are extended to multi-particle systems. Using these extensions, we propose a feasible two-particle arrival-time experiment and numerically evaluate the corresponding joint distributions. Our results reveal regimes in which the two approaches yield inequivalent predictions, highlighting conditions under which experiments could shed new light on distinguishing between competing accounts of time in quantum mechanics. Our findings also provide important insights for the development of quantum technologies that use entanglement in the time domain, including non-local temporal interferometry, temporal ghost imaging, and temporal state tomography in multi-particle systems.
We formulate quantum tunneling as a time-of-arrival problem: we determine the detection probability for particles passing through a barrier at a detector located a distance L from the tunneling region. For this purpose, we use a positive-operator-valued measure (POVM) for the time of arrival determined in C. Anastopoulos and N. Savvidou, J. Math. Phys. 47, 122106 (2006). This only depends on the initial state, the Hamiltonian, and the location of the detector. The POVM above provides a well-defined probability density and an unambiguous interpretation of all quantities involved. We demonstrate that for a class of localized initial states, the detection probability allows for an identification of tunneling time with the classic phase time. We also establish limits to the definability of tunneling time. We then generalize these results to a sequential measurement setup: the phase-space properties of the particles are determined by an unsharp sampling before their attempt to cross the barrier. For such measurements the tunneling time is defined as a genuine observable. This allows us to construct a probability distribution for its values that is definable for all initial states and potentials. We also identify a regime in which these probabilities correspond to a tunneling-time operator.