The star-discrepancy lower-bound conjecture
The star-discrepancy lower-bound conjecture
Let points be chosen in , and let denote the infimum of their discrepancy. Star-discrepancy lower-bound conjecture. For ,
This is the classical great open problem in discrepancy theory, formulated as an excruciatingly difficult problem; the optimal logarithmic exponent is known in several weaker settings but remains open for the discrepancy in dimensions at least three.
Sources & referencesView supporting material
Primary source
Vladimir Temlyakov, “Connections between numerical integration, discrepancy, dispersion, and universal discretization”, arXiv:1812.04489 (2018).
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