A best possible upper bound on the star discrepancy of (t, m, 2)-nets
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Publication:3412508
DOI10.1515/156939606776886643zbMath1103.11022OpenAlexW2038921847MaRDI QIDQ3412508
Publication date: 6 December 2006
Published in: Monte Carlo Methods and Applications (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1515/156939606776886643
Irregularities of distribution, discrepancy (11K38) Pseudo-random numbers; Monte Carlo methods (11K45)
Related Items (5)
Van der Corput sequences towards general \((0,1)\)-sequences in base \(b\) ⋮ New star discrepancy bounds for \((t,m,s)\)-nets and \((t,s)\)-sequences ⋮ Quasi-Monte Carlo rules for numerical integration over the unit sphere \({\mathbb{S}^2}\) ⋮ Improved upper bounds on the star discrepancy of \((t,m,s)\)-nets and \((t,s)\)-sequences ⋮ A thorough analysis of the discrepancy of shifted Hammersley and van der Corput point sets
Cites Work
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- Point sets and sequences with small discrepancy
- A method for exact calculation of the stardiscrepancy of plane sets applied to the sequences of Hammersley
- Star discrepancy estimates for digital \((t,m,2)\)-nets and digital \((t,2)\)-sequences over \(\mathbb Z_2\)
- On some remarkable properties of the two-dimensional Hammersley point set in base 2
- The extreme and \(L^2\) discrepancies of some plane sets
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