
TL;DR
This paper proposes a mesoscopic framework connecting horizon quantum effects, infrared modes, and cosmic-scale phenomena, suggesting a unified infrared structure influences photon equilibrium, baryon balance, and galactic rotation.
Contribution
It introduces a novel mesoscopic approach linking horizon quantum dynamics with large-scale cosmological and galactic phenomena through infrared modes and geometric excitations.
Findings
Infrared modes restore entropy and charge outside the causal wedge.
Photon trajectories form a cosmic cavity with a Planck spectrum.
The mesoscopic scale $\sigma$ relates to cosmic expansion and galactic rotation.
Abstract
We develop a mesoscopic framework in which the cosmological exterior is treated as an open quantum subsystem coupled to horizon degrees of freedom. Although local conservation laws satisfy , transport of baryon number across horizons removes conserved charges from the observer--accessible sector, producing effective depletion in exterior densities. Global unitarity therefore requires compensating source terms in the reduced exterior continuity equations. We show that relativistic causality forces this compensation to occur through long--wavelength geometric excitations: only infrared modes can restore entropy and charge while remaining outside the causal wedge of the infalling matter. An infrared return channel thus emerges as a generic feature of horizon--coupled semiclassical gravity. The second ingredient is a Carnot--Carath\'eodory (CC) tangent…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Pulsars and Gravitational Waves Research
