AbstractFor numerical integration in higher dimensions, bounds for the star-discrepancy with polynomial dependence on the dimension d are desirable. Furthermore, it is still a great challenge to give construction methods for low-discrepancy point sets.In this paper, we give upper bounds for the star-discrepancy and its inverse for subsets of the d-dimensional unit cube. They improve known results. In particular, we determine the usually only implicitly given constants. The bounds are based on the construction of nearly optimal δ-covers of anchored boxes in the d-dimensional unit cube.We give an explicit construction of low-discrepancy points with a derandomized algorithm. The running time of the algorithm, which is exponentially in d, is di...
AbstractWe propose an algorithm to compute upper and lower bounds for the star discrepancy of an arb...
AbstractIn the first part of this paper we derive lower bounds and constructive upper bounds for the...
AbstractIt was shown by Heinrich et al. [The inverse of the star-discrepancy depends linearly on the...
For numerical integration in higher dimensions, bounds for the star-discrepancy with polynomial depe...
AbstractFor numerical integration in higher dimensions, bounds for the star-discrepancy with polynom...
For numerical integration in higher dimensions, bounds for the star-discre-pancy with polynomial dep...
AbstractWe show new lower bounds for the star-discrepancy and its inverse for subsets of the unit cu...
For numerical integration in higher dimensions, bounds for the star-dis\-cre\-pan\-cy with polynomia...
For numerical integration in higher dimensions, bounds for the star-dis\-cre\-pan\-cy with polynomia...
For numerical integration in higher dimensions, bounds for the star-dis\-cre\-pan\-cy with polynomia...
AbstractWe provide a deterministic algorithm that constructs small point sets exhibiting a low star ...
AbstractThe well-known star discrepancy is a common measure for the uniformity of point distribution...
A mixed sequence is a sequence in the $s$-dimensional unit cube which one obtains by concatenating a...
A mixed sequence is a sequence in the $s$-dimensional unit cube which one obtains by concatenating a...
AbstractWe discuss open problems on the minimal star-discrepancy of an n-point set in the d-dimensio...
AbstractWe propose an algorithm to compute upper and lower bounds for the star discrepancy of an arb...
AbstractIn the first part of this paper we derive lower bounds and constructive upper bounds for the...
AbstractIt was shown by Heinrich et al. [The inverse of the star-discrepancy depends linearly on the...
For numerical integration in higher dimensions, bounds for the star-discrepancy with polynomial depe...
AbstractFor numerical integration in higher dimensions, bounds for the star-discrepancy with polynom...
For numerical integration in higher dimensions, bounds for the star-discre-pancy with polynomial dep...
AbstractWe show new lower bounds for the star-discrepancy and its inverse for subsets of the unit cu...
For numerical integration in higher dimensions, bounds for the star-dis\-cre\-pan\-cy with polynomia...
For numerical integration in higher dimensions, bounds for the star-dis\-cre\-pan\-cy with polynomia...
For numerical integration in higher dimensions, bounds for the star-dis\-cre\-pan\-cy with polynomia...
AbstractWe provide a deterministic algorithm that constructs small point sets exhibiting a low star ...
AbstractThe well-known star discrepancy is a common measure for the uniformity of point distribution...
A mixed sequence is a sequence in the $s$-dimensional unit cube which one obtains by concatenating a...
A mixed sequence is a sequence in the $s$-dimensional unit cube which one obtains by concatenating a...
AbstractWe discuss open problems on the minimal star-discrepancy of an n-point set in the d-dimensio...
AbstractWe propose an algorithm to compute upper and lower bounds for the star discrepancy of an arb...
AbstractIn the first part of this paper we derive lower bounds and constructive upper bounds for the...
AbstractIt was shown by Heinrich et al. [The inverse of the star-discrepancy depends linearly on the...