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research article

Computing Bounds for the Star Discrepancy

Thiémard, Eric
2000
Computing

We observe that the time required to compute the star discrepancy of a sequence of points in a multidimensional unit cube is prohibitive and that the best known upper bounds for the star discrepancy of (t,s)-sequences and (t,m,s)-nets are useful only for sample sizes that grow exponentially with the dimension s. Then, an algorithm to compute upper bounds for the star discrepancy of an arbitrary set of n points in the s-dimensional unit cube is proposed. For an integer k≥1, this algorithm computes in O(nslogk+2^s*k^s) time and O(k^s) space a bound that is no better than a function depending on s and k. As an application, we give improved upper bounds for the star discrepancy of some Faure (0,m,s)-nets for s∈{7,…,20}.

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Type
research article
DOI
10.1007/s006070070018
Web of Science ID

WOS:000165880600005

Author(s)
Thiémard, Eric
Date Issued

2000

Published in
Computing
Volume

65

Issue

2

Start page

169

End page

186

Subjects

Star discrepancy

•

mathematical programming

•

algorithm

•

complexity

Note

PRO 2000.09

Editorial or Peer reviewed

REVIEWED

Written at

EPFL

EPFL units
ROSO  
Available on Infoscience
February 13, 2006
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/222946
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