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Proper time from a max‑entropy constraint on entangled histories

Alessandro Capurso

Published Jun 25, 2026• 0 citations
Publisher

Abstract

We present a kinematic reconstruction of relativistic proper time in a discrete history-based framework, without assuming a background spacetime manifold. The construction introduces a minimal operational parametrization of unresolved localization and temporal order prior to collapse. Observers are modeled as massive quantum systems decomposed into spatial and temporal history sectors encoding the system and clock degrees of freedom. We assume that the accessible information of a history is given by its max-entropy and scales with the spherical boundary area of its causal cone. This assumption induces a trade-off between spatial and temporal resources. In the coarse-grained regime, the model recovers the standard proper-time relation, the time-dilation formula, and discrete counterparts of the Minkowski interval and of the proper-time functional. The analysis does not assume a specific microscopic dynamics or a field-theoretic completion. The construction shows that relativistic temporal structure can be recovered from informational constraints in a form relevant to operational and information-theoretic approaches to a quantum description of spacetime.

DOI
10.5281/zenodo.20851405

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We present a kinematic reconstruction of relativistic proper time in a discrete history-based framework, without assuming a background spacetime manifold. The construction introduces a minimal operational parametrization of unresolved localization and temporal order prior to collapse. Observers are modeled as massive quantum systems decomposed into spatial and temporal history sectors encoding the system and clock degrees of freedom. We assume that the accessible information of a history is given by its max-entropy and scales with the spherical boundary area of its causal cone. This assumption induces a trade-off between spatial and temporal resources. In the coarse-grained regime, the model recovers the standard proper-time relation, the time-dilation formula, and discrete counterparts of the Minkowski interval and of the proper-time functional. The analysis does not assume a specific microscopic dynamics or a field-theoretic completion. The construction shows that relativistic temporal structure can be recovered from informational constraints in a form relevant to operational and information-theoretic approaches to a quantum description of spacetime.
We present a kinematic reconstruction of relativistic proper time in a discrete history-based framework, without assuming a background spacetime manifold. The construction introduces a minimal operational parametrization of unresolved localization and temporal order prior to collapse. Observers are modeled as massive quantum systems decomposed into spatial and temporal history sectors encoding the system and clock degrees of freedom. We assume that the accessible information of a history is given by its max-entropy and scales with the spherical boundary area of its causal cone. This assumption induces a trade-off between spatial and temporal resources. In the coarse-grained regime, the model recovers the standard proper-time relation, the time-dilation formula, and discrete counterparts of the Minkowski interval and of the proper-time functional. The analysis does not assume a specific microscopic dynamics or a field-theoretic completion. The construction shows that relativistic temporal structure can be recovered from informational constraints in a form relevant to operational and information-theoretic approaches to a quantum description of spacetime.
We develop a top-down counterpart of the minimal proper-time formulation of quantum field theory previously introduced as an effective bottom-up framework. Starting from a deterministic pre-geometric substrate of causally ordered events, we show how coarse-graining over microscopic histories leads, at low energies, to an effective Nambu-like quantum dynamics. The elementary deterministic update is identified with the minimal proper-time step, while the growth of coarse-grained equivalence classes controls both the ultraviolet dissipative correction and the scale dependence of the effective quantization strength, encoded in a running Planck constant. In this way, the proper-time cutoff kernel of the bottom-up formulation acquires a microscopic interpretation as the inverse growth of unresolved deterministic histories. In the infrared limit, the dissipative term vanishes and standard unitary quantum field theory is recovered. The same coarse-grained structure also provides a natural setting for an emergent relativistic spacetime geometry, compatible in the macroscopic limit with Einstein gravity. The resulting picture suggests a common deterministic origin for minimal-scale structure, quantum behavior, and relativistic spacetime.
The nature of time remains a central problem in fundamental physics, spanning quantum mechanics, thermodynamics, and relativity. In this work, we develop an observer-dependent framework in which time is not assumed as a fundamental background parameter, but emerges operationally from restricted access to a globally timeless quantum state. Building on and extending the Page–Wootters mechanism, we introduce a unified relational formula that shows how three traditionally distinct aspects of temporality arise from the same structure: quantum dynamics from conditioning on physical clock states, thermodynamic irreversibility from partial tracing over inaccessible degrees of freedom, and observer-relative time from the locality of the clock subsystem. No modification of unitary quantum mechanics, collapse postulates, or fundamental time flow is required. Analytical arguments and numerical simulations demonstrate that, in the limit of complete information access, all temporal ordering disappears, while effective Schrödinger dynamics and an arrow of time emerge naturally under informational and observational constraints. These results support a central claim: time is not a property of the universe itself, but a property of descriptions generated by physical observers embedded within it.
Paper III — Relativistic Extension of Ordered Information Locality DescriptionExtending the operational locality framework into a relativistic regime, this paper demonstrates how Lorentz-compatible dynamics emerge from ordered information constraints. Without presupposing Minkowski spacetime, relativistic causal structure arises from invariant bounds on influence propagation. This work situates special relativity as an emergent consistency condition within the Ordered-Dynamics Reconstruction Program rather than a fundamental geometric assumption. Keywordsrelativity; Lorentz invariance; operational locality; causal structure; emergent spacetime; quantum foundations
The theories of special relativity and quantum mechanics both rely on continuous rotation groups to describe physical systems, yet one is formulated on a real spacetime manifold while the other employs a complex Hilbert space. This work investigates whether this distinction may arise from the treatment of time itself. By examining the consequences of describing a relativistic system using a single global time parameter, we explore whether such a description naturally requires a mathematical structure capable of encoding observer-dependent proper times as complex phase information. Within this framework, quantum superposition is investigated as a possible coordinate-level representation of unresolved relativistic frame assignments, while wavefunction collapse is conceptualised as the physical resolution of this ambiguity through interaction. exploring whether aspects of the quantum formalism may be understood as consequences of describing the invariant structure of Minkowski spacetime from a local perspective using a rigid notion of time.
This work revisits the long‑standing asymmetry in the treatment of time between quantum theory and general relativity. In quantum theory, time functions as an externally supplied, fine‑grained parameter governing microscopic state updates, whereas in relativity it appears as a coarse‑grained geometric quantity encoded in proper time. This Letter argues that this asymmetry can be understood as a scale‑dependent feature rather than a fundamental inconsistency. By reorganizing the perspective within existing theoretical frameworks—without introducing new physical assumptions—the microscopic time of quantum theory and the macroscopic geometric time of relativity can be interpreted as descriptions operating at different temporal scales. This scale‑dependent viewpoint offers a minimal and conceptually coherent starting point for reconsidering the “problem of time’’ in quantum gravity and provides a basic clue toward bridging quantum theory and relativity. The discussion is intended as a compact conceptual note, and a more detailed mathematical formulation will be presented in a separate work.