Halo first crossing with a finite variance cutoff

ID: halo-first-crossing-with-a-finite-variance-cutoff

A small-scale spectral cutoff bounds the smoothing variance by . A sharp-k excursion remains Brownian up to this terminal variance, with total crossed fraction . The ordinary first-crossing density remains valid before the cutoff. Below the sharp-filter cutoff radius the variance is constant, so there are no new crossings and the idealized differential halo abundance vanishes. The missing fraction need not be artificially renormalized to one.

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