Effective Carrier Routing, Control Work, and Stress in a Finite WRRA Model
Abstract
We construct an effective carrier model within the Worldline–Residue–Resource–Action framework. Two conditionally independent registers encode prime-factor multiplicities. A label-symmetric equality projector controls a common source coupled to two supplied particle-pair channels. One pulse generates the earlier collision-statistic probabilities without address-dependent interaction strength. A restricted single-register obstruction and a classification of diagonal permutation-invariant effects specify the construction’s resource assumptions. The implementation reproduces species probabilities, but not the preceding interface’s coherent output channel. Bare-energy conservation holds at the calibrated reference volume; detuning away from resonance requires interaction energy and switching work. A response identity relates the reference pressure-volume moment to the logarithmic-volume derivative of mean pulse work. Composition with the implemented muon-decay kernel recovers energy and pressure histories at full conversion. This is an executable effective interaction candidate and compatibility analysis; lepton identities, weak interactions, and the full fifteen-channel carrier are not derived from arithmetic alone. Version 0.2, editorial revision of 9 October 2026. Includes the English manuscript, Korean guide, and reproducibility archive. The 123 carrier-level checks are internal consistency checks, not experimental validation or external journal peer review. The manuscript was prepared before this deposit; its preparation-time statement that no public DOI had been assigned is superseded by this record. Preceding WRRA records: r11, https://doi.org/10.5281/zenodo.23237629; particle interface v0.2, https://doi.org/10.5281/zenodo.23241511; dynamic decays v0.2, https://doi.org/10.5281/zenodo.23246308. Correction release 0.2-r1 (9 October 2026): Table 3 now states that the hot electron branch has a positive pressure-volume moment; the antielectron-neutrino overbar in Section 6.2 is correctly rendered in the PDF. The scientific model, reproduction code and numerical results are unchanged. The manuscript retains its v0.2 designation and filenames; 0.2-r1 identifies this corrected deposit. A third Astra medium AI internal review and post-correction check examined the final files. Both required corrections were resolved, with no further mandatory technical corrections identified. The review report is included. This is not external journal peer review or acceptance. Earlier statements in the guide/review about two review rounds describe the historical pre-correction state.
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Authors: Wonsik Choi, Jeongin Choi