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Set Star-Menger and Set Strongly Star-Menger Spaces

  • Ljubiša D. R. Kočinac EMAIL logo , Şukran Konca EMAIL logo and Sumit Singh EMAIL logo
Published/Copyright: February 16, 2022
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Abstract

Motivated by the Arhangel’skii “s-Lindelöf cardinal function” definition, Kočinac and Konca defined and studied set covering properties and set star covering properties. In this paper, we present results on the star covering properties called set star-Menger and set strongly star-Menger. We investigate the relationship among set star-Menger, set strongly star-Menger and other related properties and study the topological properties of set star-Menger and set strongly star-Menger properties.

2020 Mathematics Subject Classification: Primary 54D20; Secondary 54E35

1. Introduction and preliminaries

In [1], Arhangel’skii defined a cardinal function sL, and spaces X such that sL(X) = ω we call s-Lindelöf: a space X is s-Lindelöf if for each subset A of X and each open cover U of A¯ by open sets in X there is a countable set VU such that AV¯. Motivated by this definition, Kočinac and Konca [14,15] (see also [6] for a similar study) considered new types of selective covering properties called set covering properties. In [14], the authors investigated the set-Menger, set-Hurewicz, set-Rothberger and other related (weaker) properties. Later on, Singh [19] and Kočinac [13] noticed that the properties set-Menger, set-Hurewicz and set-Rothberger are actually equvalent to Menger, Hurewicz and Rothberger properties, respectively.

In this paper, by using the star operator, we investigate the star versions of the set-Menger property called set star-Menger and set strongly star-Menger properties. Let us mention that set star-Menger spaces have been defined and considered the first time in [15]. We discuss the relationships among the set star-Menger, set strongly star-Menger and other related properties. Further, we study topological properties of the set star-Menger and set strongly star-Menger properties.

If A is a subset of a set X and F is a collection of subsets of X, then the star of A with respect to F, denoted by St(A,F), is the set St(A,F)={FF:FA0}. We write St(x,F) instead of St(x,F).

Throughout the paper the following assumptions are considered:

  1. By “a space” we mean “a topological space”.

  2. ℕ denotes the set of natural numbers.

  3. An open cover U of a subset AX means elements of U are open in X and AU={U:UU}.

We first recall the classical notions of spaces which are used in this paper. The Menger covering property is a well-known covering property in topological spaces.

A space X is said to have the Menger property [16] if for each sequence Un:n of open covers of X, there is a sequence Vn:n such that for each n,Vn is a finite subset of Un and X=nVn.

Kočinac [10,11], introduced the star versions of the Menger covering property using star operator in the following way (for some articles related to the star versions of the classical selective covering properties see, for instance, [4, 5, 20, 21]).

A space X is said to have the star-Menger property (SM) [10,11] if for each sequence Un:n of open covers of X, there is a sequence Vn:n such that for each n,Vn is a finite subset of Un and X=nStVn,Un.

A space X is said to be strongly star-Menger (SSM) [10,11] if for each sequence Un:n of open covers of X, there is a sequence (Fn : n ∈ ℕ) of finite subsets of X such that X=nStFn,Un.

Recently, Kočinac and Konca [14] defined set-Menger spaces and their weaker versions.

Definition 1 ([14]).

A space X is said to have the set-Menger property (set-M) if for each nonempty set AX and each sequence Un:n of collections of open sets in X such that A¯Un, there is a sequence Vn:n such that for each n,Vn is a finite subset of Un and AnVn.

Remark 1.

In [19] and [13], the authors noticed that set-Menger spaces are nothing but another way to define Menger spaces.

Definition 2 ([2, 7, 17]).

A space X is said to be:

  1. starcompact (SC) if for each open cover U of X there is a finite subset V of U such that X=St(V,U).

  2. strongly starcompact (SSC) if for each open cover U of X, there is a finite subset F of X such that X=St(F,U).

In a similar way, we define the following.

Definition 3.

A space X is said to be:

  1. set-starcompact (set-SC) if for each nonempty subset A of X and each open cover U of A¯, there is a finite subset V of U such that A=St(V,U)A.

  2. set strongly starcompact (set-SSC) if for each nonempty subset A of X and each open cover U of A¯, there is a finite subset F of A¯ such that A=St(F,U)A.

    It is clear by the definition that every set strongly starcompact space is set-starcompact.

Theorem 1.1.

Every countably compact space is set strongly starcompact.

Proof. Let X be a countably compact space, A a nonempty subset of X and U a cover of A¯ by open sets in X. As closed subsets of a countably compact space are also countably compact, A¯ is countably compact. But any countably compact space is strongly starcompact [7]. Therefore, there is a finite set FA¯ such that AA¯St(F,U), i.e. X is set strongly starcompact. □

Corollary 1.1.1.

Every countably compact space is set-starcompact.

In [7: Theorem 2.1.5] (see also [9]), it is proved that a strongly starcompact Hausorff space is countably compact. Since set strong starcompactness implies strong starcompactness, we have the following theorem.

Theorem 1.2.

If X is a set strongly starcompact Hausdorff space, then X is countably compact.

Recall that a collection AP(ω) is said to be almost disjoint if each set AA is infinite and the sets AB are finite for all distinct elements A,BA. For an almost disjoint family A, put ψ(A)=Aω and topologize ψ(A) as follows: for each element AA and each finite set Fω, {A} ∪ (A \ F) is a basic open neighborhood of A and the natural numbers are isolated. The spaces of this type are called Isbell-Mrówka ψ-spaces [3,18] or ψ(A) space.

Throughout the paper, notation and terminology mainly follow [8]. The cardinality of a set is denoted by |A|. Let ω denote the first infinite cardinal, ω1 the first uncountable cardinal, c the cardinality of the set of real numbers. For a cardinal κ, κ+ denotes the smallest cardinal greater than κ. For each pair of ordinals α, β with α < β, we write

[α,β)={γ:αγ<β},(α,β]={γ:α<γβ},(α,β)={γ:α<γ<β},[α,β]={γ:αγβ}.

As usual, a cardinal is an initial ordinal and an ordinal is the set of smaller ordinals. A cardinal is often viewed as a space with the usual order topology.

A subset A of X is said to be regular open if A=Int(A¯). A subset B of X is said to be regular closed if its complement is regular open or, equivalently, if B=Int(B)¯.

2. Set star-Menger and set strongly star-Menger spaces

In this section, we introduce set star-Menger and set strongly star-Menger spaces and give some examples showing the relationships between set star-Menger spaces and other related spaces. Some of these examples are known in the star selection principles theory and we discover some their additional properties.

Definition 4.

A space X is said to have:

  1. the set star-Menger property (shortly, set-SM property) if for each nonempty subset A of X and each sequence Un:n of collections of open sets in X such that A¯Un, n ∈ ℕ, there is a sequence Vn:n such that for each n ∈ ℕ, Vn is a finite subset of Un and AnStVn,Un;

  2. the set strongly star-Menger property (shortly, set-SSM property) if for each nonempty set AX and each sequence Un:n of collections of open sets in X such that A¯Un, there is a sequence (Fn: n ∈ ℕ) of finite subsets of A¯ such that AnStFn,Un

    Theorem 1.1 and the following lemma shows that the class of set strongly star-Menger spaces is big enough.

Lemma 2.1.

Every Menger space is set strongly star-Menger.

Proof. Let X be a Menger space. Let A be any nonempty subset of X and Un:n be a sequence of collections of open sets in X such that A¯Un. Since closed subsets of Menger spaces are Menger, then A¯ is Menger. Therefore, there exists a sequence Vn:n such that for each n ∈ ℕ, Vn is a finite subset of Un and A¯nVn. Choose xVA¯V for each VVn. For each n ∈ ℕ, let Fn=xV:VVn. Then each Fn is a finite subset of A¯ and AA¯nStFn,Un. □

The following example shows that converse of Lemma 2.1 is not true.

Example 1.

There exists a Tychonoff set strongly star-Menger space which is not Menger.

Proof. Let X = [0, ω1). Then X is a countably compact space, but not Lindelöf. Hence, X is a set strongly star-Menger space which is not Menger. □

We have the following diagram from the definitions and by Lemma 2.1. However, the converse of the implications may not be true as shown by examples below.

DIAGRAM 1
DIAGRAM 1

We now show that vertical arrows between first and second lines of properties in Diagram 1 are not reversible.

Example 2.

There exists a Tychonoff set star-Menger (resp., set strongly star-Menger) space which is not set-starcompact (resp., set strongly starcompact).

Proof. Let

X=([0,ω]×[0,ω]){ω,ω}

be the subspace of the product space [0, ω] ×[0, ω]. Then X is a Tychonoff space.

Since X is countable, it is a Menger space. Since every Menger space is set strongly star-Menger and set star-Menger, we have that X is set strongly star-Menger and set star-Menger.

Next, we show that X is not set-starcompact. Let A={⟨n, ω⟩ : nω} and for each nω, let

Un={n}×[n,ω].

Let us consider the open cover

U=Un:nω

of A=A¯. To prove that X is not set-starcompact, it is enough to show that there exists a point aA such that aSt(V,U) for any finite subset V of U. So, let V be a finite subset of U. Then, there exists n1ω such that UnV for each n > n1. Let a = 〈m, ω〉 with m > n1. But Um is the only element of U containing ⟨m, ω⟩. Thus a=m,ωSt(V,U)=V, which shows that X is not set-starcompact. It also follows that X cannot be set strongly starcompact. This completes the proof. □

We are going now to prove in the following two examples that vertical arrows between properties in the second and third lines of Diagram 1 are not reversible.

Example 3.

There exists a Tychonoff star-Menger space which is not set star-Menger.

Proof. Let D(c)=dα:α<c be the discrete space of cardinality c, and let

X=βD(c)×c++1(βD(c)D(c))×c+

be the subspace of the product space βD(c)×c++1, where βD(c) is the Stone-Čech compactification of D(c).

In [22: Example 2.2], Song shows that X is a star-Menger space. Now we prove that X is not set star-Menger.

Let A=D(c)×c+. Then A is a closed subset of X. For each α<c, let

Uα=dα×c++1.

Then Uα is open in X by the construction of the topology of X and UαUα=0 for αα′. For each n ∈ ℕ, let Un=Uα:α<c. Then Un:n is a sequence of open covers of A¯. It is enough to show that there exists a point dβ,c+A such that

dβ,c+StVn,Unforalln,

for any sequence Vn:n such that Vn is a finite subset of Un,n. Let Vn:n be any sequence such that for each n ∈ ℕ, Vn is a finite subset of Un. For each n ∈ ℕ, Vn is finite, then there exists αn<c such that UαVn for each α > αn. Let

α=supαn:n.

If we pick β > α′, then UβVn for each n ∈ ℕ. Since Uβ is the only element of Un containing the point dβ,c+ for each n ∈ ℕ, then dβ,c+StVn,Un for all n ∈ ℕ, which shows that X is not set star-Menger. □

Example 4.

Assuming ω1<d=c, there exists a Tychonoff pseudocompact strongly star-Menger space which is not set strongly star-Menger.

Proof. Let X=ψ(A) be the Isbell-Mrówka space with A is maximal and |A|=ω1. Then X is strongly star-Menger Tychonoff pseudocompact space (see [3]). Now we prove that X is not set strongly star-Menger. Let A=A=aα:α<ω1. Then A is closed subset of X. For each α < ω1, let Uα = {aα} ∪ (aα). For each n ∈ ℕ, let Un=Uα:α<ω1. Then Un:n is a sequence of open covers of A¯. It is enough to show that there exists a point αβA such that

aβStFn,Unforalln,

for any sequence (Fn : n ∈ ℕ) of finite subsets of A¯. Let (Fn : n ∈ ℕ) be any sequence of finite subsets of A¯. Then there exists α′ < ω1 such that Uα(nFn)=0, for each α > α′. Pick β > α′, then UβFn=0 for each n ∈ ℕ. Since Uβ is the only element of Un containing the point αβ for each n ∈ ℕ, then aβStFn,Un for all n ∈ ℕ. It shows that X is not set strongly star-Menger. □

We now show that horizontal arrows between first and second lines of properties in Diagram 1 are not reversible.

Example 5.

There exists a T1 set star-Menger space which is not set strongly star-Menger.

Proof. Let X = AB, where A=aα:α<c is any set with |A|=c and B is any countable set such that any element of B is not in A. Topologize X as follows: for each ααA and each finite subset FB, {αα} ∪ (B \ F) is a basic open neighborhood of aα, and each element of B is isolated. Then X is a T1-space.

First we show that X is set star-Menger space. Let C be any nonempty subset of X and Un:n be any sequence of open covers of C¯. We have three possible cases.

  1. CA.

    Then for each n ∈ ℕ and for each aαC, there exists Uα,nUn such that aαUα,n, i.e. we can find a finite set Fα,nB such that {aα} ∪ (B \ Fα,n) ⊂ Uα,n. Then, it is clear that for each n ∈ ℕ and each β<c with βα, Uα,nUβ,n0. For each n ∈ ℕ, let Vn=Uα,n. Then each Vn is a finite subset of Un and CnSt(Vn,Un).

  2. CB.

    Since B is countable, B is set star Menger. Therefore, for each n ∈ ℕ there is a finite subset Wn of Un such that CnStWn,Un.

  3. CAB.

    Let C = C1C2, where C1A and C2B. Choose VnUn and WnUn such that C1nStVn,Un and C2nStWn,Un. Let Hn=VnWn. Then Vn is a finite subset of Hn and CnStHn,Un.

So, we conclude that X is a set star-Menger space.

Taking A=A¯X and working quite similarly to the proof of Example 4, we easily prove that X is not a set strongly star-Menger space. □

It would be interesting to answer the following question.

Problem 1.

Does there exist a Tychonoff set star-Menger space which is not set strongly star-Menger?

Remark 2.

  1. The space X in Example 5 is a set-starcompact space but not set strongly starcompact. So, we have proved that the horizontal arrow in the first line of properties in Diagram 1 is not reversible.

  2. It is known that there are star-Menger spaces which are not strongly star-Menger (see, for example, [5, 12]) so that the horizontal arrow in the last line of Diagram 1 is not reversible.

In some classes of spaces certain properties from Diagram 1 coincide. Kočinac proved the following theorem in [10].

Theorem 2.1.

([10: Theorem 2.8]). In the class of paracompact Hausdorff spaces, Mengerness, star-Mengerness and strongly star-Mengerness coincide.

From Theorem 2.1 and Diagram 1 we get the following result.

Theorem 2.2.

If X is a paracompact Hausdorff space, then the following statements are equivalent:

  1. X is Menger;

  2. X is set star-Menger;

  3. X is set strongly star-Menger;

  4. X is strongly star-Menger;

  5. X is star-Menger.

Remark 3.

A space X is said to be para-Lindelöf if every open cover U of X has a locally-countable open refinement V. In [5: Theorem 2.10] it was proved that in the class of regular para-Lindelöf spaces Mengerness, star-Mengerness and strongly star-Mengerness are equivalent. So, Theorem 2.2 can be extended to the class of regular para-Lindelöf spaces.

A space is said to be meta-Lindelöf if every open cover of it has a point-countable open refinement. Kočinac [10] obtained the following corollary.

Corollary 2.2.1.

([10: Corollary 2.10]). A regular meta-Lindelöf strongly star-Menger space is Menger.

Corollary 2.2.1 and Diagram 1 give the following corollary.

Corollary 2.2.2.

If X is a regular meta-Lindelöf space, then the following statements are equivalent:

  1. X is Menger;

  2. X is set strongly star-Menger;

  3. X is strongly star-Menger.

A space X is metacompact if each open cover of X has a point-finite open refinement. From [10: Theorem 2.4], we have the following corollary.

Corollary 2.2.3.

Every set strongly star-Menger hereditarily metacompact spaceXis a Menger space.

3. Properties of set star-Menger and set strongly star-Menger spaces

In this section, we study some topological properties of set star-Menger and set strongly star-Menger spaces.

Observe that set star-Mengerness and set strong star-Mengerness are not hereditary properties. The ordinal space [0, ω1) is a Hausdorff countably compact space, therefore it is set strongly star-Menger. But its subspace Y = {α + 1 : α is a limit ordinal} is uncountable and discrete, so it cannot be set strongly star-Menger.

Example 5 shows that a closed subset of a set star-Menger space need not be set star-Menger. The space X in that example is set star-Menger, but the set A=aα:α<cX is not, since it is a discrete closed subset with cardinality c.

We have the following results about preservation of set star-Mengerness and set strong star-Mengerness by subspaces.

Theorem 3.1.

A clopen subspace of a set star-Menger space is also set star-Menger.

Proof. Let X be a set star-Menger space and YX be a clopen subspace. Let A be any subset of Y and Un:n be any sequence of collections of open sets in (Y, τY) such that for each n ∈ ℕ, ClY(A)Un. Since Y is open, then Un:n is a sequence of collections of open sets in X, and since Y is closed, ClY(A) = ClX(A). Applying the set star-Mengerness of X, there exists a sequence Vn:n such that for each n ∈ ℕ, Vn is a finite subset of Un and AnStVn,Un. Hence Y is set star-Menger. □

On the lines of Theorem 3.1, we can similarly prove the following theorem.

Theorem 3.2.

A clopen subspace of a set strongly star-Menger space is also set strongly star-Menger.

We now consider (non)preservation of set star-Mengerness and set strong star-Mengerness under some sorts of mappings.

Theorem 3.3.

A continuous image of a set star-Menger space is set star-Menger.

Proof. Let X be a set star-Menger space and f: XY a continuous mapping from X onto Y. Let B be any subset of Y and Vn:n be a sequence of open covers of B¯. Set A = f(B). Since ƒ is continuous, for each n ∈ ℕ, Un=f(V):VVn is a collection of open sets in X with

A¯=f(B)¯f(B¯)f(Vn)=Un.

As X is set star-Menger, there exists a sequence Un:n such that for each n ∈ ℕ, Un is a finite subset of Un and,

AnStUn,Un.

Let Vn=V:f(V)Un. Then for each n ∈ ℕ, Vn is a finite subset of Vn and

B=f(A)fnStUn,UnnStff(V):VVn,Vn=nStVn,Vn.

Thus Y is a set star-Menger space. □

We can prove the following theorem similarly to the proof of Theorem 3.3.

Theorem 3.4.

A continuous image of a set strongly star-Menger space is set strongly star-Menger.

Now we give a positive result on preimages of set strongly star-Menger spaces. For this we need a new concept defined as follows. We call a space Xnearly set stongly star-Menger if for each AX and each sequence Un:n of open covers of X there is a sequence (Fn : n ∈ ℕ) of finite subsets of X such that AnStFn,Un.

Theorem 3.5.

Letf : XYbe an open and closed, finite-to-one continuous mapping from a spaceXonto a set strongly star-Menger spaceY. ThenXis nearly set strongly star-Menger.

Proof. Let AX be any nonempty set and Un:n be a sequence of open covers of X. Then B = ƒ(A) is a subset of Y. Let yB¯. Then f(y) is a finite subset of X, and thus for each n ∈ ℕ, there is a finite subset Un,y of Un such that f(y)Un,y and Uf(y)0 for each UUn,y. Since ƒ is closed, there exists an open neighborhood Vn,y of y in Y such that fVn,yU:UUn,y. Since ƒ is open, we can assume that

Vn,yf(U):UUn,y.

Now, for each n ∈ ℕ, Vn=Vn,y:yB¯ is an open cover of B¯. Since Y is set strongly star-Menger, there exist a sequence (Fn : n ∈ ℕ) of finite subsets of B¯ such that

BnStFn,Vn.

Since ƒ is finite-to-one, the sequence (f(Fn) : n ∈ ℕ) is a sequence of finite subsets of X. We prove

AnSt(f(Fn),Un),

Let XA. Then, there exists n ∈ ℕ and yB¯ such that f(x) ∈ Vn,y and Vn,yFn0. Since

xfVn,yU:UUn,y

we can choose UUn,y with xU. Then Vn,yf(U). Thus Uf(Fn)0. Hence xStfFn,Un. It follows that

AnStfFn,Un.

Thus X is nearly set strongly star-Menger. □

Following the above definition of nearly set strongly star-Menger spaces, we will call a space Xnearly set star-Menger if for each AX and each sequence Un:n of open covers of X there is a sequence Vn:n such that for each n, Vn is a finite subset of Un and AnStVn,Un.

Similarly to the proof of Theorem 3.5, with necessary small modifications, we can prove the following.

Theorem 3.6.

If f : X → Y is an open perfect mapping and Y is a set star-Menger space, then X is nearly set star-Menger.

The product of two set star-Menger spaces need not be set star-Menger. In fact, the following well-known example (see [8, 24]) shows that the product of two countably compact (hence set strongly star-Menger) spaces need not be set star-Menger (hence not set strongly star-Menger). Song [23: Example 2.12] proved that the product X × Y is not star-Menger. Thus X × Y is not set star-Menger. Here we give a rough proof for the sake of completeness.

Example 6.

There exist two countably compact spaces X and Y such that X × Y is not set star-Menger.

Proof. Let Dc be the discrete space of cardinality c. We can define X=α<ω1Eα, Y=α<ω1Fα, where Eα and Fα are subsets of βDc defined inductively so that the following three conditions are satisfied:

  1. EαFβ=D(c) if αβ;

  2. Eαc and Fαc;

  3. every infinite subset of Eα (resp., Fα) has an accumulation point in Eα+1(resp., Fα + 1).

Those sets Eα and Fα are well-defined since every infinite closed set in βDc has cardinality 2c (see [24]). The diagonal {d,d:dD(c)} is a discrete open and closed subset of X × Y of cardinality c so that it is not set star-Menger. Thus X × Y is not set star-Menger, since, by Theorem 3.1, open and closed subsets of set star-Menger spaces are set star-Menger. □

In the following example, initially considered in [7: Example 3.3.3], we show that the product of a countably compact (hence, set star-Menger) space and a Lindelöf space need not be set star-Menger.

Example 7.

There exist a countably compact (hence, set star-Menger) space X and a Lindelöf space Y such that X × Y is not set star-Menger.

Proof. Let X = [0, ω1) be equipped with the order topology, and let Y = [0, ω1] with the following topology. Each point α < ω1 is isolated, and a set U containing ω1 is open if and only if Y \ U is countable. Then, X is countably compact and Y is Lindelöf. By [23: Example 2.13], X × Y is not star-Menger. Thus it cannot be set star-Menger. □

Above results suggest the following problem.

Problem 2.

Is the product of a set strongly star-Menger (set star-Menger) space with a compact space set strongly star-Menger (set star-Menger)?

4. Concluding remarks

This paper deals with two set star properties. Some further investigations on this kind of star covering properties (which we began to study) may include similar properties of Hurewicz-type and Rothberger-type star selection principles, as well as some weaker forms of set-SM, set-SSM spaces and their Hurewicz-type and Rothberger-type versions. We give here definitions of these properties.

Definition 5.

A space X is said to be:

  1. set star-Hurewicz (resp., set strongly star-Hurewicz) if for each AX and each sequence Un:n of open covers of A¯ there is a sequence Vn:n (resp., a sequence (Fn : n ∈ ℕ)) such that Vn is a finite subset of Un (resp., Fn is a finite subset of A¯) for each n ∈ ℕ, and each XA belongs to all but finitely many sets StVn,Un (resp., to all but finitely many sets StFn,Un);

  2. set star-Rothberger (resp., set strongly star-Rothberger) if for each AX and each sequence Un:n of collections of open sets in X such that A¯Un, there is a sequence (Un : n ∈ ℕ) (resp., a sequence (xn : n ∈ ℕ)) such that UnUn (resp., xnA¯) for each n ∈ ℕ and AnStUn,Un (resp., AnSt(xn,Un)).

Definition 6.

A space X is said to be:

  1. weakly set star-Menger (almost set star-Menger, faintly set star-Menger) if for each AX and each sequence Un:n of open covers of A¯ by open sets in X, there is a sequence Vn:n such that Vn is a finite subset of Un for each n ∈ ℕ, and AnStVn,Un¯, AnSt(Vn,Un)¯(AnSt(Vn¯,Un));

  2. weakly set strongly star-Menger (almost set strongly star-Menger) if for each AX and each sequence Un:n of open covers of A¯ there is a sequence (Fn : n ∈ ℕ) of finite subsets of A¯ such that AnSt(Fn,Un)¯(AnSt(Fn,Un)¯)..

In a similar way we define weaker forms of Hurewicz-type and Rothberger-type properties.


(Communicated by David Buhagiar)


Acknowledgement

The authors are grateful to the referees for their careful reading of the paper and for a number of comments and remarks which improved the exposition of the paper.

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Received: 2020-09-28
Accepted: 2021-01-31
Published Online: 2022-02-16
Published in Print: 2022-02-16

© 2022 Mathematical Institute Slovak Academy of Sciences

This work is licensed under the Creative Commons Attribution 4.0 International License.

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