The S-normalised temperature error #
The positive increments telescope to T (Nstar β) - θprev. The abstract
amplitude V estimate is applied with an amplitude tending down to the exact
quantity S = √κprev ‖∇θprev‖; the small positive slack handles S = 0 without
adding a nonvanishing-temperature hypothesis.
Euclidean-normed real vectors used in the temperature error L² estimates.
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View a spatial vector in the Euclidean-normed carrier for the temperature estimates.
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Closed time-space unit cell for the temperature error estimates.
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Finite positive-increment telescope in the spacetime gradient norm.
The only quantitative input is the zeroth-word slice of l.V; the base
profile is absent because the difference is the sum over i ≥ 1.
The hTemperatureError leaf with the exact S-normalisation of .
hbase is the scale-S theta profile in the precise shape
consumed by abstract l.V. The flow, coefficient and smallness hypotheses are
likewise kept in the exact shapes consumed there. hCt allows the surrounding
RelativeLeaves record to choose any constant at least the explicit bound.