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Quantum Completion of Quantum Vacuum Polarization Gravity (QVP-G) via the Information Resonance Network (IRN)

Đulović, Damir

Published Dec 2, 2025• 0 citations
Publisher

Abstract

This paper develops the quantum completion of Quantum Vacuum Polarization Gravity (QVP-G) by introducing the Information Resonance Network (IRN) as an underlying quantum substrate. While the macroscopic QVP-G framework describes gravity as an emergent effect of vacuum polarization encoded in a scalar field P(x), the present work provides an ontological and dynamical picture of how quantum states, decoherence, and the Born rule arise from microscopic IRN degrees of freedom. We model the IRN as a many-body quantum system on a graph whose nodes carry localized information degrees of freedom and whose edges encode resonance couplings. Quantum states of matter and of the polarization field are reinterpreted as collective excitation patterns of this network. Within the open-quantum-systems framework, we identify the relevant system–environment split, derive an influence functional for the IRN environment, and obtain effective master equations for macroscopic matter degrees of freedom coupled to the polarization field. In the quasi-static, Markovian regime we show that IRN-induced decoherence rates are governed by a polarization energy functional E_P[Δρ] of the mass-density difference between superposed configurations, leading to scalings of the form Γ_IRN ∝ E_P[Δρ]/ħ. In suitable limits the polarization energy E_P[Δρ] reduces to the gravitational self-energy |E_G[Δρ]|, and the IRN-induced decoherence channel reproduces a Diósi–Penrose-type scaling Γ ∝ |E_G|/ħ as a derived property rather than a phenomenological postulate. We analyse the conditions under which this mechanism can dominate over conventional environmental decoherence, and delineate the parameter range compatible with laboratory interferometry constraints and cosmological observations within the validity of the effective field theory. A detailed case study of the double-slit experiment is presented in the IRN picture. Interference patterns, which-path detection, and measurement outcomes are described in terms of competing IRN branches, each corresponding to macroscopically distinct polarization configurations correlated with different detector states. The Born rule emerges from the combinatorics and relative stability of IRN microstate ensembles under coarse-graining, rather than being imposed as a separate axiom. Classical trajectories, pointer states, and quasi-localized “worlds” appear as robust IRN patterns stabilized by resonance structure and network connectivity. We compare the QVP-G/IRN completion to leading collapse and decoherence models such as the Diósi–Penrose proposal and Continuous Spontaneous Localization (CSL), highlighting similarities in the dependence on gravitational or polarization energies but emphasising the different ontological status of the underlying degrees of freedom. The IRN framework provides a single unified language for modified gravity, decoherence, and quantum foundations, tightly linked to the macroscopic QVP-G phenomenology on galactic and cosmological scales. This quantum-layer preprint is part of a coordinated QVP-G/IRN series: it builds on (i) the core QVP-G effective field theory unifying dark matter and dark energy, (ii) the cosmological background and linear perturbations paper (Boltzmann-code implementation), and (iii) the microscopic mQVP-G papers on gravitational “chemistry” and near-critical MOND behaviour, and provides the quantum completion that connects polarization fields, decoherence, and the structure of quantum theory. The author gratefully acknowledges the use of a novel multi-agent artificial intelligence system based on iterative Socratic dialogue as a conceptual support tool in the development of this work.

DOI
10.5281/zenodo.17789341

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The gravitational decoherence field studies the suppression of coherence in quantum systems caused by effects rooted in the gravitational interaction. This models are not just important to yield interesting ideas about the search, in regimes others than the Planck scale, for the interplay between quantum mechanics and general relativity, but also from a theoretical point of view. The fact that the gravitational field can not be shielded opens the question of how strong will the gravitational ‘environment’ decohere a quantum system? and if this decoherence can somehow explain the absence of macroscopical super- positions? This thesis studies in depth the ‘Classical Channel Gravity’ (CCG) model, a recent proposal of gravitational decoherence that assumes that the gravitational interac- tion is always accompanied with an intrinsic decoherence mechanism which ensures that there is no transmission of quantum information between the parties involved. This model can be understood a series of weak continuous quantum measurements accompanied with a feedback term produced by some underlying hidden gravitational degrees of freedom. We first study all the possible emergent dynamics from collisional Markovian dynamics; these ones range from exact unitary to arbitrary fast decoherence (Zeno effect). The second part of the thesis is devoted to study the Newtonian and post Newtonian limits of the CCG model, with particular focus on the testability features of CCG. In particular, we apply this model to coupled clocks and find that the amount of decoherence predicted by CCG is the same as the decoherence that an ‘environment of clocks’ will imprint in a single clock in the context of unitary evolution. On the other hand, we find that this effect is far from being detectable with the current achieved time accuracy. However, CCG as a model for multi partite systems and two systems with very different masses seems to yield an amount of decoherence that is not only able to be detectable with current experiments but also seems to indicate that this model is ruled out. Nevertheless, we also mention potential caveats with our assumptions and discuss other physically motivated directions to further study this result. Finally, we also explore the extension of CCG for the cosmological scenario. In this context the scale factor is being decohered by test particles ‘sitting’ on spacetime. We find that this decoherence will be seen by an observer unaware of the CCG fundamental mechanism as an emergent form of dark energy filling the universe.
We propose a unified physical framework in which four-dimensional spacetime vacuum is the unique physical reality, and all quanta are its localized topological excitations. Matter particles correspond to stable knot-like configurations, while radiation quanta correspond to weak propagating ripples of the same substrate. From this single ontological commitment, we derive: (1) wave–particle duality is resolved—particle behavior belongs to the localized excitation, wave behavior to the disturbance field it generates in spacetime; (2) double-slit interference arises from coherent superposition between a quantum's newly sourced disturbance and its own historical disturbance field, not from ontological self-superposition; (3) the wave function is a statistical tool encoding ensemble distributions of trajectories modulated by disturbance feedback, and collapse is epistemic convergence rather than a physical process; (4) quantum entanglement corresponds to Planck-scale topological connectivity (microscopic Einstein–Rosen bridges), preserving relativistic causality; (5) gravity is the macroscopic accumulation of universal but individually weak quantum–vacuum couplings, explaining both its microscopic weakness and macroscopic dominance without requiring a graviton; (6) the four fundamental interactions are differentiated coupling modes of quanta to one spacetime vacuum field; and (7) apparent dark matter and dark energy are reinterpreted as collective topological curvature and large-scale vacuum self-relaxation, respectively. We formulate falsifiable predictions at both laboratory and cosmological scales, including disturbance–corpuscle separation interferometry, tunable decoherence threshold measurements, and galaxy rotation–topology correlations. The framework compresses the conventional axiomatic structure of quantum mechanics and cosmology into one master axiom and eliminates at least twenty-eight independent interpretive assumptions.
This work proposes a phenomenological framework linking quantum localization to weak-field gravitational response through informational load functionals. The central idea is that the degree of spatial localization of a quantum state may be associated with an effective participation factor governing how strongly that state contributes to inertial and gravitational phenomena. Localization is quantified using standard measures such as the inverse participation ratio (IPR), combined with reference scales that render localization dimensionless. A monotonic substrate response function is introduced to map localization load to observable effects. In the weak-field regime, a linear response approximation recovers familiar gravitational scaling relations. The framework does not modify Schrödinger dynamics, introduce new particles, or attempt a full theory of quantum gravity. Instead, it explores whether aspects of gravity normally described geometrically can be reinterpreted as state-dependent informational load. Illustrative empirical connections are discussed using known atomic ionization data to show how varying localization regimes may correspond to different participation factors. These examples are intended as phenomenological consistency checks rather than precision derivations. Scope and Status: This work is exploratory and interpretational. It is intended as a conceptual bridge between quantum and gravitational descriptions, not as a completed fundamental theory. Predictions are restricted to weak-field regimes, and strong-field behavior is left open. Key Points: Treats mass-like behavior as state-dependent participation Uses established localization measures (IPR) Introduces substrate response only phenomenologically Does not invoke gravitons or modify QM equations Suggests testable scaling relations in principle Purpose: The goal is to stimulate discussion on whether gravitational response might be expressible in informational or localization terms, providing an alternative viewpoint on the QM–GR interface.Update in this version: Reference to the Effective Mass Theory.Reference to the Objective Collapse Theory
This work presents an effective theoretical framework in which quantum dynamics emerges from a homogeneous scalar compression field endowed with an internal infinite structure. The model reproduces Schrödinger-type dynamics, the continuity equation, and the quantum potential as structural consequences of the underlying field description. Within this formulation, the Born rule arises as an equilibrium condition associated with coarse-graining over unresolved internal degrees of freedom rather than as a fundamental postulate. The same field structure naturally admits a vacuum energy interpretation consistent with dark energy phenomenology. Additionally, under a conformal effective metric hypothesis, the framework yields an emergent gravitational sector compatible with the weak-field parametrized post-Newtonian (PPN) limit, reproducing standard results for light deflection, Shapiro time delay, and perihelion precession at leading order. The theory preserves local dynamical evolution while allowing globally correlated states, providing an alternative interpretational perspective consistent with effective field theory principles. The work is positioned as a foundational and conceptual investigation rather than a replacement for established quantum or gravitational theories.
Description This work develops a phenomenological framework that relates quantum localization to weak-field inertial and gravitational response using scalar “informational load” functionals. The central proposal is that mass-like behavior can be treated as a state-dependent property: more spatially localized quantum states couple more strongly to inertial and gravitational effects than delocalized states. Localization is quantified using standard concentration measures, primarily the inverse participation ratio (IPR). A dimensionless load variable is constructed and mapped to observable effects through a monotonic response function. In the linear (weak-load) regime, this construction reproduces familiar post-Newtonian scaling for time dilation and light propagation, providing consistency with weak-field general relativity. The framework is strictly diagnostic and interpretational. It does not modify Schrödinger or Dirac dynamics, does not introduce new particles or forces, and does not propose a microscopic theory of quantum gravity. Instead, it provides an effective scalar language for organizing how localization may influence inertial and gravitational response. As a simple phenomenological check, atomic ionization energies are used to estimate relative participation factors across different localization regimes. These examples illustrate consistency of the scaling picture rather than serving as precision tests. Scope and status • Valid only in weak-field / post-Newtonian regimes • Coarse-grained and phenomenological • No claims regarding strong gravity or full quantum gravity • Intended as an organizational and interpretive framework Key features • Mass-like response treated as a state-dependent participation factor • Uses established localization diagnostics (IPR) • Introduces only effective response functions • Compatible with standard quantum mechanics and general relativity • Suggests qualitative scaling relations that may be testable in principle Purpose The goal is to provide a compact conceptual bridge between quantum localization and gravitational response, and to encourage discussion of whether weak-field gravitational behavior can be expressed in terms of state-dependent informational or localization measures.
This work proposes a phenomenological framework linking quantum localization to weak-field gravitational response through informational load functionals. The central idea is that the degree of spatial localization of a quantum state may be associated with an effective participation factor governing how strongly that state contributes to inertial and gravitational phenomena. Localization is quantified using standard measures such as the inverse participation ratio (IPR), combined with reference scales that render localization dimensionless. A monotonic substrate response function is introduced to map localization load to observable effects. In the weak-field regime, a linear response approximation recovers familiar gravitational scaling relations. The framework does not modify Schrödinger dynamics, introduce new particles, or attempt a full theory of quantum gravity. Instead, it explores whether aspects of gravity normally described geometrically can be reinterpreted as state-dependent informational load. Illustrative empirical connections are discussed using known atomic ionization data to show how varying localization regimes may correspond to different participation factors. These examples are intended as phenomenological consistency checks rather than precision derivations. Scope and Status: This work is exploratory and interpretational. It is intended as a conceptual bridge between quantum and gravitational descriptions, not as a completed fundamental theory. Predictions are restricted to weak-field regimes, and strong-field behavior is left open. Key Points: Treats mass-like behavior as state-dependent participation Uses established localization measures (IPR) Introduces substrate response only phenomenologically Does not invoke gravitons or modify QM equations Suggests testable scaling relations in principle Purpose: The goal is to stimulate discussion on whether gravitational response might be expressible in informational or localization terms, providing an alternative viewpoint on the QM–GR interface.Update in this version: Reference of Effective Mass Theory. Noticed there exist the effe