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Construction of Good Rank-1 Lattice Rules Based on the Weighted Star Discrepancy

In: Monte Carlo and Quasi-Monte Carlo Methods 2004

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  • Stephen Joe

    (University of Waikato, Department of Mathematics)

Abstract

Summary The ‘goodness’ of a set of quadrature points in [0, 1]d may be measured by the weighted star discrepancy. If the weights for the weighted star discrepancy are summable, then we show that for n prime there exist n-point rank-1 lattice rules whose weighted star discrepancy is O(n−1+δ) for any δ>0, where the implied constant depends on δ and the weights, but is independent of d and n. Further, we show that the generating vector z for such lattice rules may be obtained using a component-by-component construction. The results given here for the weighted star discrepancy are used to derive corresponding results for a weighted Lp discrepancy.

Suggested Citation

  • Stephen Joe, 2006. "Construction of Good Rank-1 Lattice Rules Based on the Weighted Star Discrepancy," Springer Books, in: Harald Niederreiter & Denis Talay (ed.), Monte Carlo and Quasi-Monte Carlo Methods 2004, pages 181-196, Springer.
  • Handle: RePEc:spr:sprchp:978-3-540-31186-7_12
    DOI: 10.1007/3-540-31186-6_12
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