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Our result implies that the central dark matter profile of some clusters cannot be described by CDM halos.
Our result implies that the optical depth of the Compton cloud gradually rises as the variability class becomes harder.
Our result implies that the shear-dominated STZs will convert into dilatation-dominated operations at very low temperatures.
For some other families our result implies that matrix coefficients of all irreducible, discrete series representations are Gθ-integrable.
Thus, our result implies that for the stochastic (1.1) the noise dominates the dynamics of the solution.
In addition, our result implies that symmetric three-term recurrence equations are completely equivalent with Jacobi difference equations arising in the discrete calculus of variations.
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