1996
DOI: 10.1006/ffta.1996.0016
|View full text |Cite
|
Sign up to set email alerts
|

Low-Discrepancy Sequences and Global Function Fields with Many Rational Places

Abstract: We construct digital (t, s)-sequences in a prime-power base q for which the quality parameter t has the least possible order of magnitude. The construction uses algebraic function fields over the finite field of order q which contain many places of degree 1 relative to the genus.

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
121
0
4

Year Published

1997
1997
2012
2012

Publication Types

Select...
6
2
1

Relationship

2
7

Authors

Journals

citations
Cited by 163 publications
(125 citation statements)
references
References 21 publications
(43 reference statements)
0
121
0
4
Order By: Relevance
“…sequences [55], Faure sequences [8], Niederreiter sequences [35,36] and NiederreiterXing sequences [37]. Although a bound of the form (1.14) indicates an ultimate order of convergence theoretically higher than the classical Monte Carlo rate of 1/ √ N, that bound is unsatisfactory when the dimensionality is high because, for fixed s, (ln N) s /N keeps growing with increasing N until N is exponentially large in s. In contrast to that somewhat negative observation is a remarkable result proved by Heinrich et al [12], which states that there exists a sequence of QMC point sets for which the star discrepancy is of order √ s/N with an unknown constant, or alternatively √ s ln s ln N/N with an explicit constant.…”
Section: The Classical Setting and What Goes Wrongmentioning
confidence: 99%
“…sequences [55], Faure sequences [8], Niederreiter sequences [35,36] and NiederreiterXing sequences [37]. Although a bound of the form (1.14) indicates an ultimate order of convergence theoretically higher than the classical Monte Carlo rate of 1/ √ N, that bound is unsatisfactory when the dimensionality is high because, for fixed s, (ln N) s /N keeps growing with increasing N until N is exponentially large in s. In contrast to that somewhat negative observation is a remarkable result proved by Heinrich et al [12], which states that there exists a sequence of QMC point sets for which the star discrepancy is of order √ s/N with an unknown constant, or alternatively √ s ln s ln N/N with an explicit constant.…”
Section: The Classical Setting and What Goes Wrongmentioning
confidence: 99%
“…Of course |J F [2]| is dealt with asymptotically with the torsion limit J 2 (q, A) which we have introduced in this paper. Stirling's Formula gives an asymptotical bound for the binomial coefficients n t when t is some fixed fraction of n. Finally the quotients A r /h can be bounded by means of algebraic geometric techniques which have been used before in the code theoretic literature, for instance [25], [28], [39], [40]. We state now an upper bound of this type.…”
Section: If the N-code C * I Is T-disconnected And If C * J Has (N − mentioning
confidence: 99%
“…The construction of global function fields with many rational places, or equivalently of algebraic curves over F, with many F g -rational points, is of great theoretical interest. Moreover, it is also important for applications in the theory of algebraic-geometry codes (see [15], [16]) and in the recent constructions of low-discrepancy sequences introduced by the authors (see [5], [7], [10], [17]). …”
Section: N Q (G) = Maxn(k)mentioning
confidence: 99%
“…For the construction of sdimensional low-discrepancy sequences in a given base q by means of rational places (see e.g. [5]) we need a global function field K/W q with N(K) > s + 1. In order to cover the standard range 1 < s < 50 of applications of low-discrepancy sequences in an efficient manner, we need to find, for each dimension s in this range, a global function field K/F 9 of relatively small genus with N(K) > s + 1.…”
Section: N Q (G) = Maxn(k)mentioning
confidence: 99%