Quantum Phase Propagation, Light-Cone Invariance (∆τ = 0), and the Thermodynamic Emergence of Spacetime: A Vacuum Statistical Mechanics Mechanism for the Cosmological Constant Scale and Unitary Information Conservation

The 120-orders-of-magnitude discrepancy in the estimation of the quantum vacuum energy densityreflects a fundamental disconnect between Quantum Field Theory in flat space and the holographicconstraints imposed by Emergent Gravity. In this paper, we reevaluate the zero-point energycalculation starting from the induced gravity formalism and the UV/IR coupling proposed byCohen, Kaplan, and Nelson. We demonstrate that requiring the total vacuum energy within avolume of cosmological radius L ∼ H−10 not to exceed the mass of the corresponding black holeestablishes a non-local link between the ultraviolet cutoff scale (kUV) and the infrared cosmologicallimit (kIR). We analyze the complementary role of the null proper time condition (∆τ = 0) as afilter of radiative observability on the mass shell and show how Newton’s constant G emerges fromvacuum dynamics via Sakharov induction. Finally, we extend the model to unitary informationpreservation in gravitational collapse horizons and refine the proposed Q-VLBI interferometricprotocol for experimental verification.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-08-21
DOI
https://doi.org/10.5281/zenodo.21812399
Primary Topic
Noncommutative and Quantum Gravity Theories
Type
preprint
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preprint

Quantum Phase Propagation, Light-Cone Invariance (∆τ = 0), and the Thermodynamic Emergence of Spacetime: A Vacuum Statistical Mechanics Mechanism for the Cosmological Constant Scale and Unitary Information Conservation

Jefferson William Martinelli
Zenodo (CERN European Organization for Nuclear Research)
Noncommutative and Quantum Gravity Theories
preprint

Quantum Phase Propagation, Light-Cone Invariance (∆τ = 0), and the Thermodynamic Emergence of Spacetime: A Vacuum Statistical Mechanics Mechanism for the Cosmological Constant Scale and Unitary Information Conservation

Jefferson William Martinelli
preprint en

Abstract

The 120-orders-of-magnitude discrepancy in the estimation of the quantum vacuum energy densityreflects a fundamental disconnect between Quantum Field Theory in flat space and the holographicconstraints imposed by Emergent Gravity. In this paper, we reevaluate the zero-point energycalculation starting from the induced gravity formalism and the UV/IR coupling proposed byCohen, Kaplan, and Nelson. We demonstrate that requiring the total vacuum energy within avolume of cosmological radius L ∼ H−10 not to exceed the mass of the corresponding black holeestablishes a non-local link between the ultraviolet cutoff scale (kUV) and the infrared cosmologicallimit (kIR). We analyze the complementary role of the null proper time condition (∆τ = 0) as afilter of radiative observability on the mass shell and show how Newton’s constant G emerges fromvacuum dynamics via Sakharov induction. Finally, we extend the model to unitary informationpreservation in gravitational collapse horizons and refine the proposed Q-VLBI interferometricprotocol for experimental verification.

Zenodo (CERN European Organization for Nuclear Research)
Noncommutative and Quantum Gravity Theories
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