Probabilistic Star Discrepancy Bounds for Double Infinite Random Matrices

2Citations
Citations of this article
1Readers
Mendeley users who have this article in their library.
Get full text

Abstract

In 2001 Heinrich, Novak, Wasilkowski and Wózniakowski proved that the inverse of the discrepancy depends linearly on the dimension, by showing that a Monte Carlo point set P of N points in the s-dimensional unit cube satisfies the discrepancy bound D*sN (P) ≥ cabss1/2N-1/2 with positive probability. Later their results were generalized by Dick to the case of double infinite random matrices. In the present paper we give asymptotically optimal bounds for the discrepancy of such random matrices, and give estimates for the corresponding probabilities. In particular we prove that the N ×s-dimensional projections PN,s of a double infinite random matrix satisfy the discrepancy estimate D*sN (PN,s) ≤ (2130 + 308 1n 1n N/s)1/2 s1/2N-1/2 for all N and s with positive probability. This improves the bound D*sN (PN,s) ≤ (cabs ln N)1/2 s1/2N-1/2 given by Dick. Additionally, we show how our approach can be used to show the existence of completely uniformly distributed sequences of small discrepancy which find applications in Markov Chain Monte Carlo. © Springer-Verlag Berlin Heidelberg 2013.

Cite

CITATION STYLE

APA

Aistleitner, C., & Weimar, M. (2013). Probabilistic Star Discrepancy Bounds for Double Infinite Random Matrices. In Springer Proceedings in Mathematics and Statistics (Vol. 65, pp. 271–287). https://doi.org/10.1007/978-3-642-41095-6_10

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free