Abstract
It is known that there is a constant c > 0 such that for every sequence x1, x2, . . . in [0, 1) we have for the star discrepancy
It is known that there is a constant c > 0 such that for every sequence x1, x2, . . . in [0, 1) we have for the star discrepancy
© 2017 Gerhard Larcher, Florian Puchhammer, published by Slovak Academy of Sciences, Mathematical Institute
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