Quantum Model of the Universe Volume II. Book II: "Fundamental Hypotheses and Structural Discoveries"
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| Formato: | Recurso digital |
| Lenguaje: | inglés |
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Zenodo
2026
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| _version_ | 1866901577650929664 |
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| author | Kolesnyak, Serge |
| author_facet | Kolesnyak, Serge |
| contents | <p><strong>Abstract</strong><br>This second volume Book II of the Quantum Model of the Universe (QMU) presents a comprehensive,<br>structurally organized analysis of late-time cosmology, focusing on the emergence, mechanisms, and<br>constraints of cosmic acceleration. Building on the foundational and early-universe regimes developed<br>in Volume I, the present work investigates the structural, geometric, and vacuum–matter interactions that<br>govern accelerated expansion, formulating each hypothesis as a self-contained, logically coherent unit<br>with explicit mathematical, structural, and observational status.<br>The Book II systematically explores the vacuum–structure coupling, multi-sector interactions,<br>phase-space saturation, backreaction effects, and covariant structural constraints that collectively<br>determine the onset and magnitude of cosmic acceleration. Classical ΛCDM dynamics are reinterpreted<br>as limiting cases within a broader structural framework, and the effective dark energy contribution is<br>derived from cumulative vacuum–matter interactions rather than ad hoc postulates. Each mechanism is<br>analyzed for structural necessity, testability, and parameter closure, ensuring that all statements are either<br>mathematically inevitable, observationally falsifiable, or clearly delineated as logically contingent.<br>The collection serves as a rigorous map of admissible cosmological models at late times, highlighting<br>the structural boundaries of accelerated expansion and the universal constraints imposed by relativistic<br>cosmology, vacuum invariance, and gravitational coherence. Volume II situates the QMU contributions as<br>extensions that unify early-universe physics with late-time acceleration, closing previously unresolved<br>logical spaces and providing a robust foundation for observational verification and falsification of the<br>structural acceleration framework.</p> <p><strong>Introduction</strong><br>This work constitutes Book II of the Quantum Model of the Universe (QMU) Volume II, forming the<br>central segment of a three-book structure within the second volume of the QMU framework. While<br>Volume II as a whole addresses the transition from primordial regimes to multi-domain cosmology, Book<br>II specifically develops the structural theory of late-time cosmic acceleration, extending the foundational<br>and early-universe dynamics established in Book I of Volume II.<br>Book II is designed as a self-contained, logically coherent unit, yet it is inseparably linked to the<br>other books: it builds directly upon the physical carriers, vacuum structure, quantum geometry, and<br>early-universe regimes analyzed in Book I, and it provides the necessary structural and multi-domain<br>foundations that are further expanded in Book III. This arrangement preserves a continuous logical<br>and mathematical narrative across Volume II while allowing each book to be read independently for<br>specialized study.<br>The primary objective of Book II is to demonstrate that cosmic acceleration is not an anomaly<br>requiring additional microphysical postulates or ad hoc dark-energy models, but rather a structural<br>necessity emerging from global vacuum–matter interactions, geometric invariants, and relativistic<br>cosmology. Each hypothesis and mechanism is treated as a self-contained unit with explicit<br>mathematical formulation, structural status, and observational interface, consistent with the QMU<br>canonical methodology.<br>The chapters are organized into two interconnected layers. The first layer addresses vacuum–structure<br>interactions, multi-sector coupling, phase-space saturation, parameter closure, and effective cosmological<br>backreaction mechanisms. Classical ΛCDM and phenomenological dark energy models are<br>systematically reinterpreted as limiting or approximate cases within this structural framework.<br>The second layer integrates cumulative and global effects, including external-mass contributions,<br>bubble-in-bubble scenarios, multiverse interactions, and statistical coordination across vacuum sectors,<br>connecting early-universe inheritance to late-time cosmic acceleration.<br>For practical coherence, chapters in Book II are sequentially numbered from 36 to 98, reflecting<br>continuity from Book I and alignment with the overarching Volume II structure. Transition chapters<br>explicitly link the early-universe physics of Book I to the structural acceleration theorems and<br>multi-domain considerations that culminate in Book III.<br>Through rigorous mathematical derivation, structural classification, and observational testability,<br>Book II provides a complete, falsifiable, and publication-ready framework for understanding late-time<br>cosmic acceleration. By situating acceleration as a structurally necessary phenomenon, it closes a key<br>logical gap between early-universe dynamics and the multi-domain cosmology addressed in Book III,<br>firmly embedding Book II as the central segment of Volume II</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18495434 |
| institution | Zenodo |
| language | eng |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Quantum Model of the Universe Volume II. Book II: "Fundamental Hypotheses and Structural Discoveries" Kolesnyak, Serge Cosmic acceleration Late-time expansion Vacuum structure Structural cosmology Quantum Model of the Universe Multi-sector vacuum Effective cosmological term Structural boundaries Covariant geometry Phase-space saturation Gravitational binding Information-theoretic cosmology Entropic acceleration Horizon-scale backreaction Structural necessity <p><strong>Abstract</strong><br>This second volume Book II of the Quantum Model of the Universe (QMU) presents a comprehensive,<br>structurally organized analysis of late-time cosmology, focusing on the emergence, mechanisms, and<br>constraints of cosmic acceleration. Building on the foundational and early-universe regimes developed<br>in Volume I, the present work investigates the structural, geometric, and vacuum–matter interactions that<br>govern accelerated expansion, formulating each hypothesis as a self-contained, logically coherent unit<br>with explicit mathematical, structural, and observational status.<br>The Book II systematically explores the vacuum–structure coupling, multi-sector interactions,<br>phase-space saturation, backreaction effects, and covariant structural constraints that collectively<br>determine the onset and magnitude of cosmic acceleration. Classical ΛCDM dynamics are reinterpreted<br>as limiting cases within a broader structural framework, and the effective dark energy contribution is<br>derived from cumulative vacuum–matter interactions rather than ad hoc postulates. Each mechanism is<br>analyzed for structural necessity, testability, and parameter closure, ensuring that all statements are either<br>mathematically inevitable, observationally falsifiable, or clearly delineated as logically contingent.<br>The collection serves as a rigorous map of admissible cosmological models at late times, highlighting<br>the structural boundaries of accelerated expansion and the universal constraints imposed by relativistic<br>cosmology, vacuum invariance, and gravitational coherence. Volume II situates the QMU contributions as<br>extensions that unify early-universe physics with late-time acceleration, closing previously unresolved<br>logical spaces and providing a robust foundation for observational verification and falsification of the<br>structural acceleration framework.</p> <p><strong>Introduction</strong><br>This work constitutes Book II of the Quantum Model of the Universe (QMU) Volume II, forming the<br>central segment of a three-book structure within the second volume of the QMU framework. While<br>Volume II as a whole addresses the transition from primordial regimes to multi-domain cosmology, Book<br>II specifically develops the structural theory of late-time cosmic acceleration, extending the foundational<br>and early-universe dynamics established in Book I of Volume II.<br>Book II is designed as a self-contained, logically coherent unit, yet it is inseparably linked to the<br>other books: it builds directly upon the physical carriers, vacuum structure, quantum geometry, and<br>early-universe regimes analyzed in Book I, and it provides the necessary structural and multi-domain<br>foundations that are further expanded in Book III. This arrangement preserves a continuous logical<br>and mathematical narrative across Volume II while allowing each book to be read independently for<br>specialized study.<br>The primary objective of Book II is to demonstrate that cosmic acceleration is not an anomaly<br>requiring additional microphysical postulates or ad hoc dark-energy models, but rather a structural<br>necessity emerging from global vacuum–matter interactions, geometric invariants, and relativistic<br>cosmology. Each hypothesis and mechanism is treated as a self-contained unit with explicit<br>mathematical formulation, structural status, and observational interface, consistent with the QMU<br>canonical methodology.<br>The chapters are organized into two interconnected layers. The first layer addresses vacuum–structure<br>interactions, multi-sector coupling, phase-space saturation, parameter closure, and effective cosmological<br>backreaction mechanisms. Classical ΛCDM and phenomenological dark energy models are<br>systematically reinterpreted as limiting or approximate cases within this structural framework.<br>The second layer integrates cumulative and global effects, including external-mass contributions,<br>bubble-in-bubble scenarios, multiverse interactions, and statistical coordination across vacuum sectors,<br>connecting early-universe inheritance to late-time cosmic acceleration.<br>For practical coherence, chapters in Book II are sequentially numbered from 36 to 98, reflecting<br>continuity from Book I and alignment with the overarching Volume II structure. Transition chapters<br>explicitly link the early-universe physics of Book I to the structural acceleration theorems and<br>multi-domain considerations that culminate in Book III.<br>Through rigorous mathematical derivation, structural classification, and observational testability,<br>Book II provides a complete, falsifiable, and publication-ready framework for understanding late-time<br>cosmic acceleration. By situating acceleration as a structurally necessary phenomenon, it closes a key<br>logical gap between early-universe dynamics and the multi-domain cosmology addressed in Book III,<br>firmly embedding Book II as the central segment of Volume II</p> |
| title | Quantum Model of the Universe Volume II. Book II: "Fundamental Hypotheses and Structural Discoveries" |
| topic | Cosmic acceleration Late-time expansion Vacuum structure Structural cosmology Quantum Model of the Universe Multi-sector vacuum Effective cosmological term Structural boundaries Covariant geometry Phase-space saturation Gravitational binding Information-theoretic cosmology Entropic acceleration Horizon-scale backreaction Structural necessity |
| url | https://doi.org/10.5281/zenodo.18495434 |