Improving a constant in high-dimensional discrepancy estimates
For all s ? 1 and N ? 1 there exist sequences (z1,..., zN) in [0, 1]s such that the star-discrepancy of these points can be bounded by D* N(z1,..., zN) ? c ?s/?N . In practice it is desirable to obtain low values of c. The best known value for the constant is c = 10 as has been calculated by Aistleitner. In this paper we improve the bound to c = 9.
Keyword(s):
1994 ◽
Vol 14
(3)
◽
pp. 241-251
◽
2015 ◽
Vol E98.A
(12)
◽
pp. 2439-2445
1997 ◽
Vol 29
(6)
◽
pp. 83-94
Keyword(s):
2019 ◽
Vol 8
(5)
◽
pp. 2414-2417