Under a decorrelation assumption, the homogenization length scale for high-contrast space-time random parabolic equations is at most exp(C log²(1+Λ/λ)) + C√λ.
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Coarse-graining and quantitative stochastic homogenization of parabolic equations in high contrast
Under a decorrelation assumption, the homogenization length scale for high-contrast space-time random parabolic equations is at most exp(C log²(1+Λ/λ)) + C√λ.