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Technical note presents a detection protocol testing a cosmological model in astrophysical sources M87 and Sgr A, implying a new analytical method.
Technical Note of the COCM Observational Programme. Presents a four-phase detection protocol for testing Prediction VIII of the Concentric Orbital Cosmological Model using existing ngEHT and EHT archive data from M87 and Sgr A* (2017-2024). No new observations required. Core method: temporal stacking of Stokes parameters (Q, U) to separate persistent geometric polarization floor from stochastic MHD turbulence. Companion to DOI: 10.5281/zenodo.19950582, 10.5281/zenodo.19991607, 10.5281/zenodo.20090596, 10.5281/zenodo.20096465.*
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José Luis Vázquez González (2026) studied this question.
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