Late-Time Cosmic Acceleration as a Structural Necessity of Relativistic Cosmology

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Authors: Serge Kolesnyak
Cited by: 0

Abstract

Description Volume 12 studies the points at which the precision of modern cosmology becomes a test of its theoretical limits. Cosmic tensions are treated as structural diagnostics rather than automatic refutations of established physics. The central question is whether a deeper description of the Universe can remain simultaneously compatible with precision cosmology, early-Universe chronology, strong-field gravity, black-hole thermodynamics, entropy bounds, quantum information, and recovery of successful classical and semiclassical limits. The volume treats discrepancies between early- and late-Universe determinations, expansion and growth, high-redshift structure, and theoretical reconstruction as admissibility tests. A tension acquires deeper significance only when systematic errors, calibration, selection, ordinary astrophysical explanations, reconstruction assumptions, and competing parameter freedoms have been exposed sufficiently to make the remaining disagreement physically informative. A major part of the analysis concerns temporal sufficiency. High-redshift galaxies, rapidly growing black holes, energetic transients, star formation, enrichment, compact-object production, and accretion all consume the same limited early-Universe time budget. The question is therefore not whether an isolated unusual object can be accommodated, but whether one physically coherent chronology can realize the observed population while preserving all relevant formation, feedback, and selection constraints. Black holes provide an additional theory-space filter. Their exterior geometry, horizon thermodynamics, ringdown behavior, population history, entropy, information content, and semiclassical limits join gravitational, thermodynamic, quantum, and observational reasoning. Holography, quantum error correction, soft sectors, islands, and Page-curve methods are treated as controlled mechanisms or constraints in their proper domains rather than as universal proofs about spacetime. Within the sixteen-volume QMU architecture, Volumes 1–10 establish the empirical map, admissibility rules, bounded extensions, observational interfaces, constants, and operational reconstruction machinery. Volume 11 then connects the measurable Universe to initial conditions and microphysical foundations. Volume 12 occupies the transition from those measurable and microphysical constraints toward the information-theoretic and reconstruction questions of Volume 13: its specific role is to narrow theory-space through cosmic tensions, early-Universe chronology, black-hole observations, singularity limits, entropy bounds, and holographic consistency. Volume 14 then gathers these restrictions into the final scientific synthesis, while Volumes 15–16 translate the completed programme into broader explanatory forms.

Fields of Study & Subjects

Cosmology and Gravitation Theories Black Holes and Theoretical Physics Noncommutative and Quantum Gravity Theories

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
27 January 2026
Language
EN