The inverse of the star discrepancy of a union of randomly shifted Korobov rank-1 lattice point sets depends polynomially on the dimension
Jiarui Du, Josef Dick

TL;DR
This paper demonstrates that unions of Korobov rank-1 lattice point sets with random shifts achieve near-optimal star discrepancy bounds, with the inverse discrepancy depending quadratically on the dimension, using Fourier analysis in integer arithmetic.
Contribution
It extends previous probabilistic results to classical integer settings, providing explicit bounds and reducing the search space for optimal point sets.
Findings
Star discrepancy bounded by O(s log(N_tot) / sqrt(N_tot)) with high probability
Inverse star discrepancy depends quadratically on the dimension s
Results apply to various construction scenarios with random or fixed generators and shifts
Abstract
The inverse of the star discrepancy, , defined as the minimum number of points required to achieve a star discrepancy of at most in dimension , is known to depend linearly on . However, explicit constructions achieving this optimal linear dependence remain elusive. Recently, Dick and Pillichshammer (2025) made significant progress by showing that a multiset union of randomly digitally shifted Korobov polynomial lattice point sets almost achieve the optimal dimension dependence with high probability. In this paper, we investigate the analog of this result in the setting of classical integer arithmetic using Fourier analysis. We analyze point sets constructed as multiset unions of Korobov rank-1 lattice point sets modulo a prime . We provide a comprehensive analysis covering four distinct construction scenarios, combining either random or fixed…
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Taxonomy
TopicsMathematical Approximation and Integration · Polynomial and algebraic computation · Markov Chains and Monte Carlo Methods
