On the inverse of the star-discrepancy
Numerical Analysis
2013-03-18 v2
Abstract
The inverse of the star-discrepancy denotes the smallest possible cardinality of a set of points in achieving a star-discrepancy of at most . By a result of Heinrich, Novak, Wasilkowski and Wo{\'z}niakowski, Here the dependence on the dimension is optimal, while the precise dependence on is an open problem. In the present paper we prove that This is a surprising result, which disproves a conjecture of Novak and Wo{\'z}niakowski.
Keywords
Cite
@article{arxiv.1211.2511,
title = {On the inverse of the star-discrepancy},
author = {Christoph Aistleitner},
journal= {arXiv preprint arXiv:1211.2511},
year = {2013}
}
Comments
This paper has been withdrawn by the author due to a crucial error in the proof of the main theorem