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Optimal star-discrepancy order in dimension at least three
1 · Prerequisites
- Binary Operations, Monoids, Groups and Subgroups
- Compactness in Metric Spaces
- Completeness, Completion, and Uniform Continuity
- Congruences, the Integers Modulo n and the Chinese Remainder Theorem
- Construction of the Natural Numbers
- Construction of the Real Numbers via Cauchy Sequences
- Construction of the Real Numbers via Dedekind Cuts
- Countability and Uncountability
- Deterministic quasi-Monte Carlo and discrepancy
- Divisibility, Greatest Common Divisors and Bézout's Identity
- Filters and Ultrafilters
- Finite Counting, Factorials and Binomial Coefficients
- Foundations of the Real Numbers for Analysis
- Linear Independence, Bases and Dimension
- Linear Transformations, Rank-Nullity and Quotient Spaces
- Metric Spaces
- Monotone Sequences, Bolzano-Weierstrass, and Cauchy Completeness
- Order, Zorn's Lemma, and the Axiom of Choice
- Primes, Euclid's Lemma and the Fundamental Theorem of Arithmetic
- Relations, Functions, and Quotients
- Rings, Subrings, Integral Domains and Fields
- Rⁿ as a Normed Space; Vector-Valued Functions
- Roots, Rational Powers, and Classical Inequalities
- Sequences and Limits
- Series: Convergence and the Nonnegative Tests
- Suprema and Infima
- The Riemann Integral in Rᵐ and Jordan Content
- The Riemann Integral: Definition and Integrability
- The ZFC Axioms and the Basic Set Constructions
- Vector Spaces, Linear Subspaces, Span and Direct Sums
2 · Summary
Summary
Using the published half-open, equal-weight point-multiset definition of star discrepancy, this page asks for the exact minimum order when the integer dimension is fixed before . The candidate remains conjectural in this scope. Configurations are ordered -point lists, and repeated points count with multiplicity. The companion page is contextual and does not supply a proof.
3 · Logical flowchart
4 · Definitions, theorems and proofs
Optimal star-discrepancy order at fixed dimension at least three
Open problem
Fix an integer . For each integer , let range over the ordered configurations in , with repeated points counted with multiplicity, and set where is the normalized half-open anchored-box star discrepancy of Star discrepancy, digital nets, and digital sequences. Determine the exact asymptotic order of as with fixed. In particular, prove or disprove the conjectured order and determine the correct order if this conjecture fails. Here is the natural logarithm, and means that positive constants and an integer exist such that for all .
The configuration set is nonempty because it contains the list with every point equal to . Each empirical fraction and box volume lies in , so for every configuration. Thus is a well-defined finite real infimum; attainment is not asserted.
Status
Status reviewed on 2026-10-17: the inspected sources support retaining the fixed- question as open. Owen's Practical Quasi-Monte Carlo, printed pp. 18–19, says the best possible rate is not known, records the classical Roth lower baseline and the conjectural rate, and distinguishes the settled planar order . The Roth bound is stated here only as a classical baseline, not as the strongest known lower bound. Owen's Theorem 15.7, printed p. 27, supplies an upper-order construction.
Dick's version 3 paper, dated 2026-10-15, states a result on uniform polynomial tractability exponents for inverse star discrepancy. Its Remark 1.4 explicitly separates that growing-dimension result from each fixed-dimension ray and gives a fixed-d construction upper bound; it does not state a matching fixed-d lower bound. The refreshed bounded current-results review recorded in the batch coverage and the ROOT cycle-1 report found no inspected source resolving this exact question. That review is not exhaustive and does not prove that no resolution exists. Publication requires a fresh source/version/status check. No proof of the conjectured lower bound is claimed, and this open problem is never a logical supplier.
5 · Examples, counterexamples and false statements
None yet.