Dynamic Decays and Nonequilibrium State Transitions in a Finite WRRA Model

When an unstable microscopic state refines a coarse energy sector, conservation of its reference energy does not guarantee preservation of its pressure. We construct a finite dynamical extension of an arithmetic particle readout within the Worldline–Residue–Resource–Action framework. Archived address distributions determine an initial electron-pair versus muon-pair allocation. Measured masses and a supplied muon lifetime calibrate the physical scale, while a positive finite quadrature of the tree-level three-body decay supplies daughter energies and momenta. A finite-step population map includes both charge-conjugate decay channels and retains daughter birth records during volume evolution. We establish eventwise conservation, a discrete energy–work identity, and a dynamic criterion for an aggregate to preserve both evolution and stress observables. At fixed volume, the construction conserves energy while converting cold muons into a positive-pressure daughter population. For the baseline address preparation, the dimensionless pressure rises from 0.246350 to 0.332735 over five muon lifetimes. A prescribed-expansion calculation verifies work closure and first-order convergence independently of the decay normalization. The extension removes frozen occupation as an execution restriction but does not restore the original dust equation of state. Its contribution is an explicit connection from retained arithmetic distinctions to evolving particle counts, energy transfer, and stress, with a precise account of which distinctions can be discarded. Two positive cohort mixtures share present number, energy, and stress but acquire different future moments under identical redshift. It is a calibrated finite kinetic model, not a derivation of the weak interaction or a fitted cosmological population history. Version 0.2 preprint, with reproducibility code and data. The effective decay kernel is tree-level with massless neutrinos; radiative corrections are not implemented. Source and reproducibility materials: https://github.com/Wonsik-Choi-janefather/wrra-m-0.1/tree/main/publication/WRRA_Dynamic_Decays_v0_2Preceding r11 model: https://doi.org/10.5281/zenodo.23237629

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-10-08
DOI
https://doi.org/10.5281/zenodo.23246307
Primary Topic
Cosmology and Gravitation Theories
Type
preprint
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
preprint

Dynamic Decays and Nonequilibrium State Transitions in a Finite WRRA Model

Wonsik Choi, Jeongin Choi
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
preprint

Dynamic Decays and Nonequilibrium State Transitions in a Finite WRRA Model

Wonsik Choi, Jeongin Choi
preprint en

Abstract

When an unstable microscopic state refines a coarse energy sector, conservation of its reference energy does not guarantee preservation of its pressure. We construct a finite dynamical extension of an arithmetic particle readout within the Worldline–Residue–Resource–Action framework. Archived address distributions determine an initial electron-pair versus muon-pair allocation. Measured masses and a supplied muon lifetime calibrate the physical scale, while a positive finite quadrature of the tree-level three-body decay supplies daughter energies and momenta. A finite-step population map includes both charge-conjugate decay channels and retains daughter birth records during volume evolution. We establish eventwise conservation, a discrete energy–work identity, and a dynamic criterion for an aggregate to preserve both evolution and stress observables. At fixed volume, the construction conserves energy while converting cold muons into a positive-pressure daughter population. For the baseline address preparation, the dimensionless pressure rises from 0.246350 to 0.332735 over five muon lifetimes. A prescribed-expansion calculation verifies work closure and first-order convergence independently of the decay normalization. The extension removes frozen occupation as an execution restriction but does not restore the original dust equation of state. Its contribution is an explicit connection from retained arithmetic distinctions to evolving particle counts, energy transfer, and stress, with a precise account of which distinctions can be discarded. Two positive cohort mixtures share present number, energy, and stress but acquire different future moments under identical redshift. It is a calibrated finite kinetic model, not a derivation of the weak interaction or a fitted cosmological population history. Version 0.2 preprint, with reproducibility code and data. The effective decay kernel is tree-level with massless neutrinos; radiative corrections are not implemented. Source and reproducibility materials: https://github.com/Wonsik-Choi-janefather/wrra-m-0.1/tree/main/publication/WRRA_Dynamic_Decays_v0_2Preceding r11 model: https://doi.org/10.5281/zenodo.23237629

Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.