Equation 33 · How Fast Can a Horizon Learn Which Path You Took?
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their dimensionless decohering flux. Read the equation part by part below; each part has a contextual explanation and a link to its mathematical background.
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Here C is their dimensionless decohering flux, is surface gravity with inverse-time units in the chosen normalization, and T is the associated Killing time. Their calculation fixes the numerical factor absent from earlier scaling estimates and evaluates C for an observer on the symmetry axis of a Kerr black hole [ 3 ] . The information equations above neither alter C nor derive . They translate a verified overlap into operational thresholds.
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