• Keine Ergebnisse gefunden

s-dimensional Sierpi´nski carpet

N/A
N/A
Protected

Academic year: 2022

Aktie "s-dimensional Sierpi´nski carpet"

Copied!
22
0
0

Wird geladen.... (Jetzt Volltext ansehen)

Volltext

(1)

www.ricam.oeaw.ac.at

Discrepancy estimates for point sets on the

s-dimensional Sierpinski carpet

L.L. Cristea, F. Pillichshammer, G. Pirsic, K. Scheicher

RICAM-Report 2004-13

(2)

s-dimensional Sierpi´nski carpet

L.L. Cristea

, F. Pillichshammer

, G. Pirsic and K. Scheicher

Abstract

In a recent paper Cristea and Tichy introduced several types of discrepancies of point sets on thes-dimensional Sierpi´nski carpet and proved various relations between these discrepancies. In the present paper we prove a general lower bound for those discrepancies in terms ofN, the cardinality of the point set, and we give a probabilistic proof for the existence of point sets with “small” discrepancy. Furthermore we consider a van der Corput type construction of point sets on Cs and determine the exact order of convergence of various notions of discrepancy. Finally, Carpet-Walsh functions are defined to prove an Erd˝os-Tur´an-Koksma inequality which we apply to digital point sets on the carpet.

Keywords: Discrepancy, uniform distribution, fractal sets, Sierpi´nski carpet.

MSC 2000: 11K06, 11K38, 28A80.

1 Introduction

The s-dimensional Sierpi´nski carpet Cs, s 2, is a fractal set embedded in Rs and can be obtained as follows.

LetA0 = [0,1]sbe the closed unit-cube inRs. DivideA0 into 3scongruent cubes with side length 1/3 and delete the open “central” cube. We denote

The first author is supported by the Austrian Research Foundation (FWF), Project S 8308-N05.

The second author is supported by the Austrian Research Foundation (FWF), Project S 8305 and Project P17022-N12.

1

(3)

the resulting set by A1, i.e.,

A1 =A0 \ µ1

3,2 3

s .

The set A1 is the union of 3s 1 cubes with side length 1/3. Repeat this operation for each of these 3s 1 cubes successively to obtain A2, A3, . . ..

For n N0, An is the union of (3s1)n cubes with side length 3−n, called elementary cubes of level n. We will often call such cubes simply n-cubes.

We have

An=An−1\

à 3n−1−1 [

k1,...,ks=0

Ys

i=1

µ ki 3n−1 + 1

3n, ki 3n−1 + 2

3n

¶!

.

Now the s-dimensional Sierpi´nski carpet Cs is defined as the intersection of the sets An, n N0, i.e.,

Cs:=

\

n=0

An. (See Figure 1 for an illustration of T4

n=0An.)

It is well known that Cs is a fractal set which verifies the open set con- dition and has Hausdorff dimension αs = log(3log 3s−1). Furthermore it can be shown that 0 < Hαs(Cs) < ∞, where Hαs is the αs-dimensional Hausdorff measure on Cs. Hence we may define the normalized Hausdorff measure µ on Cs by µ(A) = Hαs(A)/Hαs(Cs) for any Borel set A Cs. For a survey on properties of fractal sets we refer to [2, 7, 8, 9].

The notion of discrepancy is intimately related to that of uniform distri- bution: let X be a compact metric space with a Borel probability measure ν. A sequence ω = (xn)n≥0 is said to be ν-uniformly distributed if for any Borel set B ⊆X with ν(∂B) = 0

N−→∞lim

AN(ω, B)

N =ν(B),

where AN(ω, B) denotes the number of indices n, 0≤n ≤N 1, such that xn is contained in B. For more details we refer to [15], see also [6, 13] .

Let D be a system of Borel sets B X such that ν(∂B) = 0 for each B ∈ D. Then the discrepancy of a point set PN = {x0, . . . ,xN−1} with respect to D is defined by

DND(PN) := sup

B∈D

¯¯

¯¯AN(PN, B)

N −ν(B)

¯¯

¯¯.

(4)

Figure 1: Dimensions= 2, T4

n=0An.

For an infinite sequence ω the discrepancy DND(ω) is defined as the discrep- ancy of the first N points of the sequence. The discrepancy of a given se- quence in X is a quantitative measure for the irregularity of distribution of the sequence in X.

Discrepancies of sequences on fractal sets have already been studied for example for the planar Sierpi´nski gasket [10] (see also [6]), and also for the Sierpi´nski gasket in higher dimension, see [14]. In [1] an L2 discrepancy of point sets on self-similar fractals that fulfill the open set condition was studied.

As in [5] we consider the caseX =Cs,s≥2, endowed with the Euclidean metric. The existence of µ-uniformly distributed sequences of points on the fractal Cs follows from [15, Chapter 3, Theorem 2.2]. In [4] and [5] the authors introduce different discrepancies onCsby choosing different systems D of Borel sets in Cs.

(5)

The first discrepancy introduced onCsis the so-calledelementary discrep- ancy DNE which is defined by the system E of all elementary cubes of level n, for all n N0 (intersected with Cs). Each n-cube (n 1) is considered together with “half” of its boundary, namely with all of its lower-dimensional faces that are closer to the origin (in the Euclidean metric) than any of the parallel faces of the same dimension in then-cube. There are situations when then-cubes are considered together with more than “half” of their boundary:

if a face of the n-cube is contained in a face of a “deleted” m-cube (m≤n), then the n-cube is taken together with this face.

Furthermore, D is considered to be the system S of all sets which are intersections of Cs with intervals of the form

J = Ys

i=1

[ai, bi)

such that all vertices of J belong toCs. (If bi = 1 for some i, 1≤i≤s, then [ai, bi] occurs instead of [ai, bi) in the above product.) The related discrepancy is called carpet discrepancy and will be denoted by DNS.

In the present paper we also define a carpet star discrepancy DSN where the system S consists of all sets of S with (a1, . . . , as) = (0, . . . ,0). Note that the carpet star discrepancy is similar to the corner discrepancy defined in [5] except that for the corner discrepancy a slightly larger class of intervals is considered.

We have the following relations between the kinds of discrepancy intro- duced above:

Proposition 1 Let s≥2 and letPN ={x0, . . . ,xN−1}be a point set in Cs. 1. We have

DNE(PN)≤DSN(PN)≤c(s)¡

DNE(PN1−s−1

αs ,

where c(s) > 0 only depends on the dimension s and where αs =

log(3s−1)

log 3 denotes the Hausdorff dimension of Cs. 2. We have

DSN(PN)≤DSN(PN)2sDSN(PN).

(6)

Proof. The proof of the first statement was given in [5]. The left-hand in- equality in the second statement follows from the definitions of the discrep- ancies, and the right-hand inequality can pe proven by using the inclusion- exclusion principle. We refer to [5, Proposition 3] for the detailed proof of

an analogous result. 2

For more types of discrepancies on Cs and relations between those dis- crepancies we refer to [4, 5].

We end this Introduction with a brief outline of the paper. In Section 2 we prove a lower bound for the carpet star discrepancy of sequences in Cs and for any s 2 we prove the existence of a point set with carpet star discrepancy of order (logN/N)1/2. In Section 3 we give a van der Corput type construction of a sequence on Cs and we determine the exact order of convergence of the elementary and the carpet (star) discrepancy. In order to do this we make use of the fact that Cs can be defined as the attractor (or invariant set) of an IFS (Iterated Functions System). Finally, in the last section, Walsh functions on the carpet are defined and applied in the proof of an Erd˝os-Tur´an-Koksma inequality. Also, IFS-digital sequences are introduced and a carpet star discrepancy bound is given for IFS-digital point sets.

2 General discrepancy bounds

In this section we prove bounds for the carpet star discrepancy DNS of se- quences on Cs. Bounds for other types of discrepancy can be obtained by applying the estimates from Proposition 1.

In [10] Grabner and Tichy use W. Schmidt’s theorem on irregularities of distribution to prove a lower bound for a certain discrepancy of sequences on the planar Sierpi´nski gasket. Here we use their technique to prove a lower bound for the carpet star discrepancy of sequences in Cs.

Theorem 1 Letω = (xn)n≥0 be a sequence inCs,s 2. Then the inequality DNS(ω)≥clogN

N

holds for infinitely many N, where c >0 denotes an absolute constant.

(7)

Proof. We consider intervals of the form

I(x) := ([0, x)×[0,1)s−1)∩Cs.

Let F(x) := µ(I(x)), where µ denotes the normalized Hausdorff measure on Cs. Then for any x we have

DNS(ω)

¯¯

¯¯AN(ω, I(x))

N −F(x)

¯¯

¯¯. (1)

For any x= (x1, . . . , xs)∈Cs letk1(x) := x1. Then it is clear that AN(ω, I(x)) =AN((k1(xn))n≥0,[0, x)).

Since F is strictly increasing and continuous we find that k1(xn) [0, x) if and only if F(k1(xn))[0, F(x)). Hence from (1) we obtain

DSN(ω)

¯¯

¯¯AN((F(k1(xn)))n≥0,[0, F(x)))

N −F(x)

¯¯

¯¯. (2) It follows by a result of Schmidt [20] (see also [6, 15]) that there exists a constant c >0 such that

DSN(ω) sup

0≤y≤1

¯¯

¯¯AN((F(k1(xn)))n≥0,[0, y))

N −y

¯¯

¯¯≥clogN N

for infinitely many N. (Kuipers and Niederreiter [15] showed that one may

choose c= 1/(66 log 4).) 2

In the following theorem we give a probabilistic proof for the existence of point sets on Cs with “small” carpet star discrepancy. The idea of the proof of this result was first given by Beck in the early 1980s, see [3]. A similar approach was later used by Grabner and Tichy [10] to prove the existence of point sets on the planar Sierpi´nski gasket with small discrepancy, and by Heinrich et al. [11] to prove the existence of point sets in [0,1)s with small star discrepancy. Here we mainly follow [11].

Theorem 2 For every integer s > 1 there exists a constant c(s) > 0 such that for every positive integer N > 1 there exists a point set PN in Cs con- sisting of N points such that

DNS(PN)≤c(s)

rlogN N .

(8)

For the proof of Theorem 2 we need the following lemma.

Lemma 1 Let Γ3k be the equidistant grid on [0,1]s with mesh-size 1/3k. Then for any point set P consisting of N points in Cs we have

DSN(P) max

x∈Γ3k

¯¯

¯¯AN(P,[0,x))

N −µ([0,x))

¯¯

¯¯+δ(s, k),

where δ(s, k) := s

³3s−1 3s−1

´k

and [0,x) := Cs Qs

i=1[0, xi) for any x = (x1, . . . , xs)[0,1]s.

Remark 1 1. Note that some points of Γ3k are not contained in Cs, e.g.

(4/9,4/9)Γ9\C2.

2. The cardinality of Γ3k is (3k+ 1)s. Hence Lemma 1 shows that the supremum in the definition of the carpet star discrepancy can be re- placed by a maximum extended over the finite set Γ3k with a maximal

“error” of at most δ(s, k).

Proof. From the definition of DSN we find that for anyη >0 there exists an x ∈Cs such that the inequality

DSN

¯¯

¯¯AN(P,[0,x))

N −µ([0,x))

¯¯

¯¯+η (3)

holds. Let now x,y∈Γ3k, x= (x1, . . . , xs) and y= (y1, . . . , ys) such that xi ≤xi < xi+ 1

3k =:yi, (or

xi < xi ≤xi+ 1

3k =:yi,

should xi = 1 hold for some i) for 1≤i≤s. Then we have µ([0,y))−µ([0,x))≤£

(3k)s(3k1)s¤ 1

(3s1)k ≤s(3k)s−1 1

(3s1)k =δ(s, k).

On the other hand,

−δ(s, k) +µ([0,y))≤µ([0,x))≤µ([0,x))≤µ([0,y))≤µ([0,x)) +δ(s, k)

(9)

and therefore

µ([0,y))− AN(P,[0,y))

N −δ(s, k) µ([0,x))−AN(P,[0,x)) N

µ([0,x))− AN(P,[0,x))

N +δ(s, k).

From here and from (3) the result follows (since η > 0 can be arbitrarily

small). 2

Now we can give the proof of Theorem 2.

Proof. Let z0, . . . ,zN−1 be independent, µ-uniformly distributed random variables on Cs. For x∈Cs let

ξ(i)x =1[0,x)(zi)−µ([0,x)),

0≤i≤N−1. Then we haveE[ξx(i)] = 0 and(i)x | ≤1 for every 0 ≤i≤N−1.

From Hoeffding’s inequality (see for example [18]) it follows that for each x∈Cs we have

P

"¯¯

¯¯

¯ 1 N

NX−1

i=0

ξ(i)x

¯¯

¯¯

¯≥δ(s, k)

#

2 eδ(s,k)2N2 .

Hence with Lemma 1 and Remark 1 we obtain P[DSN 2δ(s, k)] P

·

x∈Γmax3k

¯¯

¯¯AN(P,[0,x))

N −µ([0,x))

¯¯

¯¯≤δ(s, k)

¸

1(3k+ 1)s2 eδ(s,k)2N2 . Inserting the value of δ(s, k) we get

P

"

DSN 2s

µ 3s−1 3s1

k#

1(3k+ 1)s2 es

2N 2

ş3s−1 3s−1

ť2k

.

The right hand side of the above inequality is strictly positive iff 0>log 2 +slog(3k+ 1) s2N

2

µ 3s−1 3s1

2k .

(10)

This is true for k < x0 =x0(s, N), where x0 satisfies 0 = log 2 +slog(3x0 + 1) s2N

2

µ 3s−1 3s1

2x0 . This is equivalent to

µ 3s−1 3s1

2x0

= 2

s2N (s log(3x0 + 1) + log 2). (4) It follows that

µ3s1 3s−1

2x0

= s2N

2 (s log(3x0 + 1) + log 2) < s2N 4 log 2 and hence

x0 <log3s−1

3s−1

s s2N 4 log 2. Now we insert this back into (4) and obtain

µ 3s−1 3s1

2x0

< 2 s2N

³

s log(3log33ss−1−1

q s2N 4 log 2

+ 1) + log 2

´

=:R(s, N) and further (note that 33ss−1−1 <1)

x0 >log3s−1 3s−1

pR(s, N).

We have shown that if k log3s−1 3s−1

pR(s, N), then there exists a point set PN inCs consisting of N points such that

DSN(PN)2s

µ 3s−1 3s1

k . Choosing for k =

j

log3s−1 3s−1

pR(s, N) k

, we obtain that there exists a point set PN inCs consisting of N points such that

DSN(PN)2s

µ 3s−1 3s1

¶j

log3s−1 3s−1

R(s,N)

k

2s3s1 3s−1

pR(s, N)6sp

R(s, N).

(11)

Since (note that log(3)/log(33ss−1−1) = 1/(αs−s+ 1)) R(s, N) = 2

s2N

³

s log(3log33ss−1−1

q s2N 4 log 2

+ 1) + log 2

´

= 2

s2N

³ s log

³Ãs s2N 4 log 2

!αs−s+11 + 1

´

+ log 2

´

2 s2N

³

(s+ 1) log 2 + 1

2(αs−s+ 1)log

µ s2N 4 log 2

¶ ´ ,

the result follows. 2

3 A van der Corput type construction

Constructions of analogs of the van der Corput sequence on fractals have already been done for the (planar) Sierpi´nski gasket [10] and for the s- dimensional Sierpi´nski carpet Cs, for s 2 [4]. In both cases the authors state (without explicit proofs) that the elementary discrepancy of the cor- responding sequence is of order O(1/N). In the present section we give the detailed proof for the Sierpi´nski carpet Cs and we give the exact order of convergence for the carpet (star) discrepancy of the van der Corput sequence on Cs.

Let us define the van der Corput sequence on Cs starting from the ap- proach of this fractal by means of IFS. An Iterated Functions System, in short IFS, is a (finite) family of contractions. In particular, the families of similarities of the same ratio r < 1 are IFS’s. This often occurs when one constructs so-called self-similar fractals. It is known that, if {f1, f2, . . . , fm} is a family of contractions on a closed set D⊂Rs, then there exists a unique non-empty compact setF that is invariant for thefi,i= 1, . . . , m, i.e., which satisfies F = mi=1fi(F). This unique set F is called the invariant set or the attractor of the IFS {f1, f2, . . . , fm}. For more details about IFS’s we refer e.g. to [2] and [8].

In fact,Cs can be obtained as the attractor of an IFS consisting of 3s1 affine contractions on [0,1]s,

fm(y1, . . . , ys) =

³1

3y1+α1 3 ,1

3y2+ α2

3 , . . . ,1

3ys+αs 3

´ ,

(12)

where

m ∈ {0, . . . ,3s1}\n3s1 2

o

, m= Xs

i=1

αi·3s−i, αi ∈ {0,1,2}.

We have chosen the indices of the functions fm such that the following condition is satisfied: if p Cs is a point lying in the interior of a 1-cube R and p has Cartesian coordinates yi, 1 i s, with the ternary digit expansions

yi = ²i1 3 + ²i2

32 + ²i3

33 +· · · ,

where ²il ∈ {0,1,2} for 1 i s and l = 1,2, . . ., then, for m = Ps

i=1²i1· 3s−i ∈ {0, . . . ,3s1}\ ©3s−1

2

ª we have fm([0,1]s) = R. This IFS provides addresses for all points of the fractal set Cs. For details regarding IFS- addresses we refer e.g. to [2]. The special case of the Sierpi´nski carpet has already been approached in [4]. In the following we will use the addresses provided by the IFS mentioned above in order to define a particular sequence ω = (xn)n≥0 onCs.

For this purpose we expand every integern 0 in the base 3s1:

n = XL

l=0

αl+1(n)·(3s1)l, αL+1(n)6= 0 and define

δl(n) =

½ αl(n) if αl(n)6= 3s2−1, 3s1 if αl(n) = 3s2−1, for any l 1.

We define xn as the point encoded (in the sense of IFS-addresses) by (δ1(n), δ2(n), . . . , δL+1(n),0).

The sequence ω of points on Cs which is defined in this way is a Cs- analogue of the van der Corput sequence in the unit interval in R (see e.g.

[13]) and we call it van der Corput sequence on Cs.

Theorem 3 Let ω be the van der Corput sequence on Cs. Then for any N 1

(13)

1. for the elementary discrepancy we have 1

N ≤DNE(ω)≤c1(s) 1 N,

2. for the carpet (star) discrepancy we have c2(s) 1

N1−s−1αs ≤DSN(ω)≤DSN(ω)≤c3(s) 1 N1−s−1αs . Here ci(s)>0, 1≤i≤3, depend only on s.

Proof. 1. The left-hand inequality is trivial. For the right-hand inequality let us denote, for k∈N0, by Ek the set of elementary intervals of level k and let

DN(k)(ω) := sup

E∈Ek

¯¯

¯1 N

NX−1

n=0

1E(xn)−µ(E)

¯¯

¯,

where ω = (xn)n≥0. For simplicity we write bs := 3s 1, the number of (l+ 1)-cubes contained in anl-cube for every l≥0.

In order to find an upper bound forD(k)N (ω) let us consider the following cases:

(a) Assume that k is such that N bks. Then every k-cube contains at most one point of the set {x0, . . . ,xN−1}, and we obtain

D(k)N (ω) = max n¯¯

¯1 N 1

bks

¯¯

¯,

¯¯

¯0 1 bks

¯¯

¯ o

bs1

bks bs1 N .

Thus, for any k with N ≤bks, we have DN(k)(ω) bs1

N .

(b) Assume that k is such that N > bks. As every k-cube corresponds (e.g. by its IFS-address) to a residual classa modulo bks, 0≤a <

bks, for a given elementary cube E ∈ Ek we have

N−1X

n=0

1E(xn) = #{n < N : n≡a(modbks)}=

¹N −a bks

º + 1.

(14)

Therefore we obtain

¯¯

¯1 N

NX−1

n=0

1E(xn)−µ(E)

¯¯

¯ =

¯¯

¯1 N

¹N −a bks

º + 1

N 1 bks

¯¯

¯

max n a

N ·bks,

¯¯

¯1

N a

N ·bks

¯¯

¯ o

1 N.

Thus we have shown that the inequality DN(k)(ω) bs1

N = 3s2 N

holds for every k N0. The result follows (with c1(s) = 3s2).

2. The upper bound follows from 1. and Proposition 1.

To prove the lower bound let N 1 and let k be the unique integer with (3s1)k−1 ≤N <(3s1)k. Then the pointsx0, . . . ,xN−1 of the van der Corput sequence are the vertices of elementary cubes of level k that are closest to the origin. Hence the interval

Ek+1 :=

h

0,3k+11 3k+1

´s

∩Cs

contains all the points x0, . . . ,xN−1, i.e., AN(ω, Ek+1)/N = 1. We ob- tain

DNS 1−µ(Ek+1) = µ(Cs\Ek+1).

The setCs\Ek+1 is a disjoint union of (3k+1)s(3k+11)s elementary cubes of level k + 1 each of which has normalized Hausdorff measure 1/(3s1)k+1. Thus

µ(Cs\Ek+1) = 1

(3s1)k+1((3k+1)s(3k+11)s)

1

(3s1)k+1s(3k+11)s−1 ≥c(s) (3k)s−1 (3s1)k−1

c(s)(3log3s−1N)s−1

N =c(s) 1

N1−s−1αs , which is the desired result.

2

(15)

4 Walsh functions on the carpet and applica- tions

In this section we aim to give a version on the Sierpi´nski carpet of the well- known Erd˝os-Tur´an-Koksma (ETK) inequality (see e.g. [12]) for the carpet star discrepancy. The crucial point in the proof of such inequalities is the Fourier expansion of indicator functions, with respect to some orthonormal L2-basis. Here, we choose a kind of Walsh function system as such a basis.

Also, we define a way to employ “digital” methods and apply the ETK- inequality to give a discrepancy bound for digital point sets on the carpet.

As in the previous section, we will make use of the IFS-address of a point.

We want to make sure that each point gets a unique address. For a given point p0 we proceed as follows: first assign digits to the elementary cubes of level 1.

Then determine in which of them the point lies to obtain the first digit; note that the elementary cubes partition the carpet so that there is only one such cube. Then repeat the process with the points pn+1 = 3pn mod [0,1)s, n≥0 to get the next digits. (We assume the same assignment of digits to n-cubes in each level, but actually the introduction of permutations at any point of the process seems to be a merely technical but otherwise not too difficult generalization.)

If, say, thel-th IFS-digit is nonzero but all subsequent digits are zero, we call l the IFS-length. The IFS-address of an elementary cube shall be the common initial IFS-digit vector of all points inside that cube.

First we define the Walsh function system on the Sierpi´nski carpet.

Definition 1 Let bs := 3s1. If k = Pn

i=1kibi−1s is the bs-adic expansion of k N0, then the k-th Walsh function on the Sierpi´nski carpet is constant on all n-cubes and for all x∈Cs in ann-cube with IFS-address (x1, . . . , xn) it attains the value

Cswalk(x) := exp (2πi·(k1x1+· · ·+knxn)/bs). (In particular, Cswal0 is constant 1 on the whole carpet.)

Earlier definitions of Walsh functions have been defined on the unit cube [0,1)s, using the b-adic expansion for an arbitrary b > 1, also Cantor digit expansions have been considered. (See, e.g. [16, 19] for an introduction and further references.)

We state some properties of the Walsh function system.

(16)

Proposition 2 1. WCs := {Cswalk}k≥0 is a complete orthonormal basis on the space of square-integrable functions on the Sierpi´nski carpet with respect to the normalized Hausdorff measure, L2(Cs, µ).

2. If we define an abelian group on Cs by introducing as group operation

⊕, the digit-wise addition modulobsof the IFS-addresses of points, then WCs is the dual or character group of Cs. In particular

Cswalk(x)Cswalk(y) = Cswalk(x⊕y)

Cswalk(x)Cswall(x) = Cswalk⊕l(x)

Cswalk(ªx) = Cswalk(x)

= Cswalªk(x),

for all k, l∈N0,x,y∈Cs. The operation on the indices is the digit- wise addition of the bs-adic expansions; ªx is the inverse of x in the group.

3. Let m be the length of the bs-adic expansion of k N (i.e., m = blogbs(k)c+ 1), let En be any n-cube of Cs and x an arbitrary point of the carpet inside that n-cube, then

Z

En

Cswalkdµ =

½ 0 if n < m,

b−ns ·Cswalk(x) if n ≥m.

4. The sumPbns−1

k=0 Cswalkevaluates to the indicator function ofCs∩[0, b−ns )s. Proof. Defining a homeomorphism of the s-dimensional carpet to [0,1) by the bijective map using the IFS-address of a point and the induced topology on the carpet, the properties follow immediately from those of the generalized (univariate) Walsh function system in base bs. For example, 3 follows from the fact that b-adic intervals of [0,1) get mapped to elementary cubes of the

Sierpi´nski carpet. 2

As the next step we will need the Walsh-Fourier expansion of the indica- tor (sometimes called characteristic) functions of half-open intervals with a corner point in the origin. (These are the sets in S in the definition of the carpet star discrepancy DNS.)

(17)

Lemma 2 For a [0,1)s, let

Ia =I(a1,...,as) :=Cs Ys

i=1

[0, ai),

and 1Ia the corresponding indicator function. For 0 < k N, let l be the length of the bs-adic expansion of k.

Thena(0) =µ(Ia) and for k >0 the modulus of the k-th carpet Walsh- Fourier coefficient is bounded by

¯¯ˆ1a(k)¯

¯ :=

¯¯

¯ Z

Cs

1Ia·Cswalk

¯¯

¯≤µ(Ia)−µ(I(a1(l−1),...,as(l−1)))≤δ(s, l), where, as in Lemma 1, δ(s, l) = s(3l(s−1))/(3s−1)l and byx(m)forx∈[0,1), m N we denote the truncation of x to m ternary digits, i.e., x(m) :=

b3mxc/3m.

Furthermore, if a lies on the 3-adic grid Γ3L = [0,1]s3−LNs0 for some L N0 thena(k) vanishes for k > bLs. In this case the Walsh-Fourier expansion is finite.

Proof. By Proposition 2(3), we can disregard the integral overI(a1(l−1),...,as(l−1))

since this interval is a union of level (l1) elementary cubes, where the in- tegral vanishes. So

Z

Cs

1Ia ·Cswalkdµ= Z

Cs

1Ia\I(a

1(l−1),...,as(l−1)) ·Cswalkdµ.

The bound follows immediately from application of the triangle inequality on the above equation. For the upper bound δ(s, l) cf. the proof of Lemma 1.

An immediate consequence of the above is that for a 3−LNs0 for some L∈N0 clearly the bound becomes zero for l > L and so the coefficient does

as well. 2

We are now ready to prove

Theorem 4 (ETK-inequality on the Sierpi´nski carpet)

(18)

Let P be a point set of cardinality N on Cs. For any L, s∈N,

DSN(P) δ(s, L) +

bXLs−1

k=1

δ(s,blogbs(bsk)c)¯

¯SN(k)¯

¯

sb(s−1)/αs s

³ 1

N1−(s−1)αs +

bsXL−1

k=1

s k1−(s−1)αs

¯¯SN(k)¯

¯´ where SN(k) := P

p∈P Cswalk(p) and δ(s, L) as in Lemma 2.

Furthermore, for s log3(L),

DNS(P)9s

³ 1

N1/αs + 9s

bXLs−1

k=1

1 k1/αs

¯¯SN(k)¯

¯´ .

Proof. First we perform a discretization using Lemma 1 of Section 2, i.e., DSN ≤δ(s, L)+ max

x∈Γ3L

¯¯

¯AN(P,[0,x))

N −µ([0,x))

¯¯

¯=:δ(s, L)+ max

x∈Γ3L

|∆N(P,x)|. We now consider the second summand more closely.

Let Ix be the interval spanned between the origin and x Γ3L. Let 1x be its indicator function (i.e., assuming 1 on Ix and 0 otherwise). We can use the Carpet-Walsh series expansion of 1x (which exists and converges by Proposition 2(1)) to calculate the local star discrepancy of the points pof a point set P as follows.

|∆N(P,x)| =

¯¯

¯1 N

X

p∈P

(1x(p)−µ(Ix))

¯¯

¯=

¯¯

¯1 N

X

p∈P bXLs−1

k=1

x(k)Cswalk(p)

¯¯

¯

=

¯¯

¯

bXLs−1

k=1

ˆ1x(k)¡ 1 N

X

p∈P

Cswalk(p)¢¯¯

¯

bXLs−1

k=1

¯¯ˆ1x(k)¯

¯· |SN(k)|.

Now the first part of the result follows from the bound on|x(k)| of Lemma 2 and, for bl−1s ≤k < bls,

δ(s, l) =s µ3s−1

3αs

l

=sbl(s−1)/αs s

bls < sb(s−1)/αs s

k1−(s−1)αs .

(19)

For the second part note that δ(s, l) =s

µ3s−1 3αs

l

3s3L(s−αs) k1/αs

and the fact that fors >log3(L) we haves(1−1/L)< αs, thusL(s−αs)<1.

2

Another way to obtain a sequence in the Sierpi´nski carpet is the so-called digital method. In the context of the current setting this would mean to proceed as follows.

Definition 2 Let an infinite matrixC Z∞×∞bs be given such that the upper left m×m sub-matrices are regular for all m∈N. To obtain the n-th point of an IFS-digital sequence, consider the infinite bs-adic digit vector d~n of n as a vector in Zbs. Then the IFS-digits of the n-th point shall be given by the coordinates of C ~dn. (For safety, C should be chosen such that in each column almost all entries are 0 to avoid ambiguous IFS-addresses.)

The above procedure corresponds to abs-adic digital (0,1)-sequence (see e.g.

[17, Ch.4], [6, Sec. 3.1.2], for more information about digital sequences on the unit cube).

We can now give the carpet star discrepancy of finite point sets of such sequences.

Corollary 1 For L, s∈N let PN be the set of the first N =bLs points of an IFS-digital sequence (xn)n≥0 on the Sierpi´nski carpet. Then

DNS(PN) s N1−s−1αs .

Proof. This follows immediately from Theorem 4 if we show SN(k) = 0 for k > 0. (This is a simple consequence of the character properties of the Walsh function system.) For m∈N, let d~m denote the infinite vector of the bs-adic digits m1, m2, . . . of m. Then, withxn=C ~dn and 0≤k < bls,

SN(k) =

NX−1

n=0

Cswalk(xn) =

NX−1

n=0

exp(2πi(d~k|C ~dn)/bs)

=

bXs−1

n1,...,nL=0

YL

j=1

exp³

2πi(d~k|~cj)nj bs

´

= YL

j=1 bXs−1

n=0

exp³

2πi(d~k|~cj) bs

´n ,

(20)

where~cj is thej-th column vector ofC and (~x|~y) denotes the scalar product.

The product can be nonzero only if (d~k|~cj) = 0 for allj. But by the definition of C, the vectors~cj(L) (i.e., truncated to lengthL) are linearly independent in ZLbs, so this can only happen for d~k =0, i.e., k = 0.

2 Remark 2 By choosing C to be the identity matrix we obtain the van der Corput sequence of Section 3 and get the same upper bound order of DSN for N =bLs points.

References

[1] Albrecher H, Matouˇsek J, and Tichy R F (2000) Discrepancy of point sequences on fractal sets. Publicationes Mathematicae Debrecen, 56/3- 4: 233–249

[2] Barnsley M F (1993) Fractals Everywhere, Boston: Academic Press [3] Beck J (1984) Some upper bounds in the theory of irregularities of dis-

tribution. Acta Arithmetica, 44 No. 2: 115–130

[4] Cristea L L (2002) Geometric Properties of Fractals, TU Graz: PhD thesis

[5] Cristea L L, Tichy R F (2003) Discrepancies of point sequences on the Sierpi´nski carpet. Math Slovaca 53 No. 4: 351–367

[6] Drmota M, Tichy R F (1997) Sequences, Discrepancies and Applications volume 1651 of Lecture Notes in Mathematics, Berlin: Springer

[7] Falconer K J (1985) The Geometry of Fractal Sets, Cambridge: Cam- bridge University Press

[8] Falconer K J (1990) Fractal Geometry, Chichester: John Wiley & Sons [9] Falconer K J (1997) Techniques in Fractal Geometry, Chichester: John

Wiley & Sons

[10] Grabner P J, Tichy R F (1998) Equidistribution and Brownian Motion on the Sierpi´nski Gasket. Monatsh Math , 125: 147–164

(21)

[11] Heinrich S, Novak E, Wasilkowski G, Wo´zniakowski H (2001) The inverse of the star-discrepancy depends linearly on the dimension. Acta Arith, 96: 279–302

[12] Hellekalek P (1994) General Discrepancy estimates: the Walsh function system. Acta Arithmetica, 67, no.3: 209–218

[13] Hlawka E (1984) The Theory of Uniform Distribution, (Translated from the German by Henry Orde with a foreword by S K Zaremba), Topics and Texts in Math, Vol 1, Reading: A B Academic Publishers (Eastern Press)

[14] Klinger B (1998) Discrepancy of Point Sequences and Numerical Inte- gration, TU Graz: PhD thesis

[15] Kuipers L , Niederreiter H (1974) Uniform Distribution of Sequences, New York: John Wiley

[16] Larcher G , Pirsic G (1999) Base change problems for generalized Walsh series and multivariate numerical integration. Pacific J Math 189, no 1:

75–105

[17] Niederreiter H (1992) Random number generation and quasi-Monte Carlo methods, CBMS-NSF Regional Conference Series in Applied Mathematics, 63, Philadelphia: SIAM

[18] Pollard D (1984) Convergence of Stochastic Processes, New York:

Springer

[19] Schipp F, Wade W R, Simon P (1990) Walsh series An introduction to dyadic harmonic analysis, Bristol: Adam Hilger, Ltd

[20] Schmidt W M (1972) Irregularities of distribution, VII. Acta Arith, 21:

45–50

Authors’ Addresses:

Ligia L Cristea, Institut f¨ur Mathematik C, TU Graz, Steyrergasse 30 / III, A - 8010 Graz, Austria (Department of Mathematics, Politehnica University

(22)

of Timisoara, Romania). Email: [email protected]

Friedrich Pillichshammer, Institut f¨ur Analysis, Universit¨at Linz, Altenbergstraße 69, A-4040 Linz, Austria. Email: friedrich. [email protected]

Gottlieb Pirsic, Johann Radon Institute for Computational and Applied Mathematics (RICAM), Austrian Academy of Sciences, Altenbergerstraße 69, A-4040 Linz, Austria. Email: [email protected]

Klaus Scheicher, Johann Radon Institute for Computational and Applied Mathematics (RICAM), Austrian Academy of Sciences, Altenbergerstraße 69, A-4040 Linz, Austria. Email: [email protected]

Referenzen

ÄHNLICHE DOKUMENTE

The analysis is presented within the proof of forthcoming Proposition 1, whose key conclusion is that under the scenario in consideration, sets A λ must have small

Periodic representations in algebraic basis Rewriting trails - Intermediate alphabets - Proof of Main Theorem.. Denote by (h 0 q,j ) j=0,1,...,s−1 the s-tuple of integers produced

Combining computational results with the theory of constructing new rigid graphs by gluing, we give a new lower bound on the maximal possible number of realizations for graphs with

This allows one to prove, for arbitrarily small cross diffusion, the global existence of weak solutions to the parabolic-parabolic model as well as the global existence of bounded

Furthermore, a standard way of computing integrals of the form (1) is to apply quasi- Monte Carlo integration by mapping the point set of a given QMC rule from the s- dimensional

Following this technique, we first prove a global L p estimate for the curl of the solutions of the Maxwell equations, for p near 2 and p ≤ 2, in the spirit of Meyers’s result, and

An essential ingredient in the proof of Theorem 1.1 is a new sum-product type result which shows that a certain expander involving products and shifts gives superquadratic growth..

In the second step, for improving the result of the first step, we use this result as an initial guess to estimate the depth of burial, the height and mean values of the