Audit of normalization methods reveals differences in galactic calculations, suggesting implications for cosmic models.
We disentangle two independent normalization choices for the galactic kinetic threshold: Paper VII's a_0-based analytical calibration vs Paper VIII's SPARC best-fit. These differ by a factor ~500 for the same beta, reflecting a genuine physical question about whether the RAR scale emerges as a population-level regularity. We update the Cassini forecast for both calibrations and for B'', and define an operational test protocol (a_eff^knee) deferred to Paper XI.
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Arturo Cerezo (2026) studied this question.
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