sthuragt.dvi @ Applied General Topology c© Universidad Politécnica de Valencia Volume 5, No. 1, 2004 pp. 79- 89 Star-Hurewicz and related properties M. Bonanzinga, F. Cammaroto and Lj.D.R. Kočinac ∗ Abstract. We continue the investigation of star selection principles first considered in [9]. We are concentrated onto star versions of the Hurewicz covering property and star selection principles related to the classes of open covers which have been recently introduced. 2000 AMS Classification: 54D20. Keywords: Selection principles, (strongly) star-Menger, (strongly) star- Rothberger, (strongly) star-Hurewicz, groupability, weak groupability, ω-cover, γ-cover. 1. Introduction A number of the results in the literature show that many topological proper- ties can be described and characterized in terms of star covering properties (see [3], [13], [2], [12]). The method of stars has been used to study the problem of metrization of topological spaces, and for definitions of several important classical topological notions. We use here such a method in investigation of selection principles for topological spaces. Let A and B be collections of open covers of a topological space X. The symbol S1(A, B) denotes the selection hypothesis that for each sequence (Un : n ∈ N) of elements of A there exists a sequence (Un : n ∈ N) such that for each n, Un ∈ Un and {Un : n ∈ N} ∈ B [18]. The symbol Sfin(A, B) denotes the selection hypothesis that for each se- quence (Un : n ∈ N) of elements of A there is a sequence (Vn : n ∈ N) such that for each n ∈ N, Vn is a finite subset of Un and ⋃ n∈N Vn is an element of B [18]. In [9], Kočinac introduced star selection principles in the following way. ∗The first and the second authors were supported by MURST - PRA 2000. The third author (corresponding author) was supported by MSRS, grant N0 1233. 80 M. Bonanzinga, F. Cammaroto, Lj.D.R. Kočinac Definition 1.1. Let A and B be collections of open covers of a space X. Then: (a) The symbol S∗1(A, B) denotes the selection hypothesis: for each sequence (Un : n ∈ N) of elements of A there exists a sequence (Un : n ∈ N) such that for each n, Un ∈ Un and {St(Un, Un) : n ∈ N} is an element of B; (b) The symbol S∗fin(A, B) denotes the selection hypothesis: for each se- quence (Un : n ∈ N) of elements of A there is a sequence (Vn : n ∈ N) such that for each n ∈ N, Vn is a finite subset of Un, and ⋃ n∈N{St(V, Un) : V ∈ Vn} ∈ B; (c) By U∗fin(A, B) we denote the selection hypothesis: for every sequence (Un : n ∈ N) of members of A there exists a sequence (Vn : n ∈ N) such that for every n, Vn is a finite subset of Un and {St(∪Vn, Un) : n ∈ N} ∈ B or there is some n ∈ N such that St(∪Vn, Un) = X. Definition 1.2. Let A and B be collections of open covers of a space X and let K be a family of subsets of X. Then we say that X belongs to the class SS ∗ K(A, B) if X satisfies the following selection hypothesis: for every sequence (Un : n ∈ N) of elements of A there exists a sequence (Kn : n ∈ N) of elements of K such that {St(Kn, Un) : n ∈ N} ∈ B. When K is the collection of all one-point [resp., finite, compact] subspaces of X we write SS∗1(A, B) [resp., SS ∗ fin(A, B), SS ∗ comp(A, B)] instead of SS ∗ K(A, B). Here, as usual, for a subset A of a space X and a collection P of subsets of X, St(A, P) denotes the star of A with respect to P, that is the set ∪{P ∈ P : A ∩ P 6= ∅}; for A = {x}, x ∈ X, we write St(x, P) instead of St({x}, P). In [10] it was explained that selection principles in uniform spaces are actu- ally a kind of star selection principles. Let X be a space. If U and V are families of subsets of X we denote by U ∧V the set {U ∩ V : U ∈ U, V ∈ V}. The symbols [X]<ω and [X]≤n denote the collection of all finite subsets of X and all subsets of X having ≤ n elements, respectively. In this paper all spaces will be Hausdorff. A and B will be collections of the following open covers of a space X: O: the collection of all open covers of X; Ω: the collection of ω-covers of X. An open cover U of X is an ω-cover [5] if X does not belong to U and every finite subset of X is contained in an element of U; Γ: the collection of γ-covers of X. An open cover U of X is a γ-cover [5] if it is infinite and each x ∈ X belongs to all but finitely many elements of U. Ogp: the collection of groupable open covers. An open cover U of X is groupable [11] if it can be expressed as a countable union of finite, pairwise disjoint subfamilies Un, n ∈ N, such that each x ∈ X belongs to ∪Un for all but finitely many n; Owgp: the collection of weakly groupable open covers. A cover U of X is a weakly groupable [1] if it is a countable union of finite, pairwise disjoint sets Un, n ∈ N, such that for each finite set F ⊂ X we have F ⊂ ∪Un for some n. Star-Hurewicz and related properties 81 We consider only spaces X whose each ω-cover contains a countable ω- subcover (or equivalently, for each n ∈ N, every open cover of Xn has a count- able subcover). Thus all considered covers are assumed to be countable. Recall that a space X is said to have the Menger property [15], [6], [16], [8] (resp. the Rothberger property [17], [16], [18] if the selection hypothesis Sfin(O, O) (resp. S1(O, O)) is true for X. The following terminology was introduced in [9]. A space X is said to have: 1. the star-Rothberger property SR, 2. the star-Menger property SM, 3. the strongly star-Rothberger property SSR, 4. the strongly star-Menger property SSM, if it satisfies the selection hypothesis: 1. S∗1(O, O), 2. S∗fin(O, O) (or, equivalently, U ∗ fin(O, O)), 3. SS∗1(O, O), 4. SS∗fin(O, O), respectively. In 1925 in [6] (see also [7]), W. Hurewicz introduced the Hurewicz covering property for a space X in the following way: H: For each sequence (Un : n ∈ N) of open covers of X there is a sequence (Vn : n ∈ N) of finite sets such that for each n Vn ⊂ Un, and for each x ∈ X, for all but finitely many n, x ∈ ∪Vn. Two star versions of this property are: SH: A space X satisfies the star-Hurewicz property if for each sequence (Un : n ∈ N) of open covers of X there is a sequence (Vn : n ∈ N) such that for each n ∈ N Vn is a finite subset of Un and each x ∈ X belongs to St(∪Vn, Un) for all but finitely many n. SSH: A space X satisfies the strongly star-Hurewicz property if for each se- quence (Un : n ∈ N) of open covers of X there is a sequence (An : n ∈ N) of finite subsets of X such that each x ∈ X belongs to St(An, Un) for all but finitely many n (i.e. if X satisfies SS∗fin(O, Γ)). In this paper we study some properties of these spaces. We also consider SM and SSM spaces, in particular in connection with new classes of covers that appeared recently in the literature - groupable and weakly groupable covers. 2. Spaces related to SM spaces Theorem 2.1. If each finite power of a space X is SM, then X satisfies U∗fin(O, Ω). Proof. Let (Un : n ∈ N) be a sequence of open covers of X and let N = N1 ∪ N2 ∪ · · · be a partition of N into infinitely many infinite subsets. For each k and each m ∈ Nk let Wm = {U1 × · · · × Uk : U1, · · · , Uk ∈ Um}. Then 82 M. Bonanzinga, F. Cammaroto, Lj.D.R. Kočinac (Wm : m ∈ Nk) is a sequence of open covers of X k, and since Xk is a star- Menger space, one can choose a sequence (Hm : m ∈ Nk) such that for each m, Hm ∈ [Wm] <ω and ⋃ m∈Nk {St(H, Wm) : H ∈ Hm} is an open cover of X k. For every m ∈ Nk and every H ∈ Hm we have H = U1(H) × · · · × Uk(H), where Ui(H) ∈ Um for every i ≤ k. Put Vm = {Ui(H) : i ≤ k, H ∈ Hm}. Then for each m ∈ Nk Vm is a finite subset of Um. We claim that {St(∪Vn, Un) : n ∈ N} is an ω-cover of X. Let F = {x1, · · · , xs} be a finite subset of X. Then x = (x1, · · · , xs) ∈ X s so that there is an n ∈ Ns such that x ∈St(H, Wn) for some H ∈ Hn. But H = U1(H) × · · · × Us(H), where U1(H), · · · , Us(H) ∈ Vn. The point x belongs to some W ∈ Wn of the form V1 × · · · × Vs, Vi ∈ Un for each i ≤ s, which meets Ui(H)×· · ·×Us(H). This means that for each i ≤ s we have xi ∈ St(Ui(H), Un) ⊂ St(∪Vn, Un), i.e. F ⊂ St(∪Vn, Un). So, X satisfies U∗fin(O, Ω). � Now we shall see that the previous theorem can be given in another form. Theorem 2.2. For a space X the following are equivalent: (1) X satisfies U∗fin(O, Ω); (2) X satisfies U∗fin(O, O wgp). Proof. Because each countable ω-cover is weakly groupable, (1) implies (2) is trivial, so that we have to prove only (2) ⇒ (1). Let (Un : n ∈ N) be a sequence of open covers of X. Let for each n, Hn := ∧ i≤n Ui. Apply (2) to the sequence (Hn; n ∈ N). There is a sequence (Wn : n ∈ N) such that for each n Wn ∈ [Hn] <ω and {St(∪Wn, Hn) : n ∈ N} is a weakly groupable cover of X. There is, therefore, a sequence n1 < n2 < · · · in N such that for each finite set F in X one has F ⊂ ∪{St(∪Wi, Hi) : nk ≤ i < nk+1} for some k. Consider the sequence (Vn : n ∈ N) defined in the following way: Vn = ⋃ i k0. Since St(Ti, Vi) ⊂ St(Si, Ui) for all i with nk ≤ i < nk+1, we have that for each k > k0, x ∈ St(Sk, Uk), i.e. {St(Sn, Un) : n ∈ N} is a γ-cover of X. � The previous theorem suggests to consider also the selection principle SS∗1(O, O gp) that is naturally related to the SSH property. We have the following result. Theorem 5.3. Let a space X satisfies the following condition: for each se- quence (Un : n ∈ N) of open covers of X there is a sequence (An : n ∈ N) of subsets of X such that for each n |An| ≤ n and {St(An, Un) : n ∈ N} is a γ-cover of X. Then X satisfies SS∗1(O, O gp). Proof. Let (Un : n ∈ N) be a sequence of open covers of X. For each n let Vn = ∧ (n−1)n/2 n0. For each n write An as An = {xi : (n − 1)n/2 < i ≤ n(n + 1)/2}. Then {St(xi, Ui) : i ∈ N} is an open groupable cover of X. Indeed, consider the sequence n1 < n2 < · · · < nk < · · · of natural numbers defined by nk = k(k − 1)/2. Then for each point x ∈ X we have x ∈ ⋃ nk fa(n) for every n ≥ na. Further, consider for each n ∈ N the finite set An := {1, 2, · · · , f(n)} subset of N. We claim that the sequence (An : n ∈ N) witnesses for (Un : n ∈ N) that A is relatively SSH in Ψ(A). Indeed, for each a ∈ A the intersection 88 M. Bonanzinga, F. Cammaroto, Lj.D.R. Kočinac Un(a) ∩ An 6= ∅ (because fa(n) ∈ An ∩ Un(a)) for each n ≥ na, i.e. each point a ∈ A belongs to all but finitely many sets St(An, Un). On the other hand, the subspace A of Ψ(A) is the discrete space of cardi- nality b and thus it can not be SSH. Let us remark that according to a result from [14] this space Ψ(A) is SSM. Acknowledgements. The third author thanks INDAM for the support and the Dipartimento di Matematica of the Università di Messina and F. Cam- maroto for the hospitality he enjoyed during his visit in November/December 2002. References [1] L. Babinkostova, Lj.D.R. Kočinac and M. Scheepers, Combinatorics of open covers (VIII), Topology Appl. (to appear). [2] M. Bonanzinga, Star-Lindelöf and absolutely star-Lindelöf spaces, Q & A in Gen. Topology 16 (1998), 79–104. [3] E.K. van Douwen, G.M. Reed, A.W. Roscoe and I.J. Tree, Star covering properties, Topology Appl. 39 (1991), 71–103. [4] R. Engelking, General Topology (PWN, Warszawa, 1977). [5] J. Gerlits and Zs. Nagy, Some properties of C(X), I, Topology Appl. 14 (1982), 151–161. [6] W. Hurewicz, Über eine Verallgemeinerung des Borelschen Theorems, Math. Z. 24 (1925), 401–421. [7] W. Hurewicz, Über Folgen stetiger Funktionen, Fund. Math. 9 (1927), 193–204. [8] W. Just, A.W. Miller, M. Scheepers and P.J. 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Math. 129 (1988), 17–33. [17] F. Rothberger, Eine Verschärfung der Eigenschaft C, Fund. Math. 30 (1938), 50–55. [18] M. Scheepers, Combinatorics of open covers I: Ramsey theory, Topology Appl. 69 (1996), 31–62. Received December 2002 Accepted February 2004 Star-Hurewicz and related properties 89 M. Bonanzinga, F. Cammaroto (milena@dipmat.unime.it, camfil@unime.it) Dipartimento di Matematica, Università di Messina, 98166, Messina, Italia Lj.D.R. Kočinac (lkocinac@ptt.yu) Faculty of Sciences and Mathematics, University of Nǐs, 18000, Nǐs, Serbia