Topology Proceedings 38

Total Page:16

File Type:pdf, Size:1020Kb

Topology Proceedings 38 Volume 38, 2011 Pages 149{164 http://topology.auburn.edu/tp/ C(휏)-Cosmic Spaces by D. N. Georgiou, S. D. Iliadis, and A. C. Megaritis Electronically published on August 26, 2010 Topology Proceedings Web: http://topology.auburn.edu/tp/ Mail: Topology Proceedings Department of Mathematics & Statistics Auburn University, Alabama 36849, USA E-mail: [email protected] ISSN: 0146-4124 COPYRIGHT ⃝c by Topology Proceedings. All rights reserved. http://topology.auburn.edu/tp/ TOPOLOGY PROCEEDINGS Volume 38 (2011) Pages 149-164 E-Published on August 26, 2010 C(휏)-COSMIC SPACES D. N. GEORGIOU, S. D. ILIADIS, AND A. C. MEGARITIS Abstract. In this paper we introduce and study the notion of C(휏)-cosmic space, where 휏 is an infinite cardinal. Partic- ularly, we prove that in the class of all C(휏)-cosmic spaces of weight ≤ 휏, there exists a universal element. 1. Preliminaries In what follows, by ! and c, we denote the first infinite cardinal and the cardinality of the continuum, respectively. Also, by jXj, we denote the cardinality of a set X and by w(X), the weight of a space X. A space T is said to be universal (see [3]) in a class IP of spaces if (1) T 2 IP and (2) for every X 2 IP there exists an embedding e of X into T . A regular space X is called cosmic (see [5]) if there exists a collection P of subsets of X with the properties (1) for every open subset U of X and every x 2 U, there exists P 2 P such that x 2 P ⊆ U, (2) jPj ≤ !. Recall that a family P of subsets of a space X is called a network of X (see [3]) if, for every point x 2 X and every open neighborhood 2000 Mathematics Subject Classification. Primary 54B99, 54C25, 54A05. Key words and phrases. cosmic space, C(휏)-cosmic space, saturated class, universal space. Work supported by the Caratheodory Programme of the University of Patras. ⃝c 2010 Topology Proceedings. 149 150 D. N. GEORGIOU, S. D. ILIADIS, AND A. C. MEGARITIS Ux of x, there exists P 2 P such that x 2 P ⊆ Ux. The network weight of a space X, denoted by nw(X), is defined as the least cardinal number 휏 such that X has a network of cardinality ≤ 휏. We note that a space X is cosmic if and only if it is regular and nw(X) ≤ !. Let 휏 be an infinite cardinal. A space X is called 휏-monolithic (see [1] and [2]) if, for every subset A of X with jAj ≤ 휏, we have nw(Cl(A)) ≤ 휏. In section 2, we give the notion of C(휏)-cosmic space and basic properties for this notion. In section 3, we prove that in the class of all C(휏)-cosmic spaces of weight ≤ 휏 there exists universal element. Finally, in section 4, we give some open problems. 2. Basic properties Definition 2.1. Let 휏 be an infinite cardinal. A space X is called Closed(휏)-cosmic (C(휏)-cosmic) if there exists a collection K of closed subsets of X with the properties (1) for every open subset U of X and every x 2 U, there exists K 2 K such that x 2 K ⊆ U, and (2) jKj ≤ 휏. Remark 2.2. (1) It is clear that for every C(휏)-cosmic space X we have nw(X) ≤ 휏. Particularly, if X is Hausdorff and compact, then we have w(X) = nw(X) ≤ 휏 (see [3, Theorem 3.1.19]). (2) Every C(휏)-cosmic space is C(휏1)-cosmic space for every 휏1 ≥ 휏. (3) Every regular space of weight less than or equal to 휏 is C(휏)- cosmic. (4) Every regular C(!)-cosmic space is cosmic. (5) Every C(휏)-cosmic is 휏-monolithic. (6) Every T1-space X with jXj ≤ 휏 is C(휏)-cosmic. 휏 (7) Every T1-space X with w(X) ≤ 휏 is C(2 )-cosmic. Indeed, for 휏 every T1-space X with w(X) ≤ 휏, we have that jXj ≤ 2 . Thus, by (6) the space X is C(2휏 )-cosmic. (8) Let X be the set of real numbers with the topology t = f(훼; +1): 훼 2 Xg [ f;g. For the space (X; t), we have that nw(X) ≤ !, X is not regular, and X is not C(휏)-cosmic for every infinite cardinal 휏. (9) Let X = [−1; 1] and t = fU ⊆ X : 0 2= U or (−1; 1) ⊆ Ug. Obviously, t is a topology on X. The space X is T0 and T4, but C(휏)-COSMIC SPACES 151 neither T1 nor T2. The space (X; t) is not C(휏)-cosmic for every infinite cardinal 휏. (10) Let X be a discrete space with jXj = 휏, where 휏 is an infinite cardinal. The space X is C(휏)-cosmic. However, X is not C(휈)- cosmic for every infinite cardinal 휈 < 휏. (11) Consider a dense subspace D of cardinality 휏 of the Cantor cube 2휏 . Then D is a C(휏)-cosmic regular space. Also, it has character 2휏 , and hence w(D) > 휏. (12) Consider the space X = (! × !) [ f1g in which a subset U is open if and only if U is empty or 1 2 U and U n (fng × !) is finite for all n 2 !. Then X is T0, cosmic (being countable), has uncountable weight (the neighborhoods of 1 are the same as in the countable Fr´echet fan), and has no closed network (because the singleton f1g is dense in X). (13) If, in Definition 2.1, the elements K of the family K are regular closed sets (that is, Cl(Int(K)) = K), then the class of all C(휏)- cosmic spaces is exactly the class of all regular spaces of weight less than or equal to 휏. (14) Let X be a non-compact locally compact space of weight less than or equal to 휏. Then the Alexandroff compactification !X of X is a C(휏)-cosmic space. In what follows we give special examples of C(휏)-cosmic spaces. In particular, we give Hausdorff C(휏)-cosmic spaces which are not regular. Example 2.3. (1) Let X be the set of real numbers with the topology t = fU ⊆ X : jX n Uj ≤ !g [ f;g: The space (X; t) is T1-space of weight c and it is not regular. Also, setting K = ffxg : x 2 Xg, we take a family of closed subsets of X such that jKj = c and for every open subset U of X and every x 2 U, we have x 2 fxg ⊆ U. This means that the space (X; t) is C(c)-cosmic. (2) Let P = f(훼; 훽) 2 R2 : 훽 > 0g be the open upper half-plane with the Euclidean topology T and L = f(훼; 훽) 2 R2 : 훽 = 0g. We consider the set X = P [ L with the topology t = T [ ffxg [ (P \ Ux): x 2 L; Ux 2 T; and x 2 Uxg. The space (X; t) is Hausdorff and it is not regular. Moreover, since 152 D. N. GEORGIOU, S. D. ILIADIS, AND A. C. MEGARITIS the subspace L of X is discrete, the weight of X is c. Setting K = ffxg : x 2 Xg, we take a family of closed subsets of X such that jKj = c and for every open subset U of X and every x 2 U, we have x 2 fxg ⊆ U. Therefore, the space (X; t) is C(c)-cosmic. (3) Let X be the set of real numbers with open neighborhoods of every nonzero point being as in the usual topology, while open 1 neighborhoods of 0 will have the form U n f n : n = 1; 2;:::g, where U is an open neighborhood of 0 in the usual topology. The space X is Hausdorff of weight !, is C(!)-cosmic, and is not regular. Proposition 2.4. Every subspace of a C(휏)-cosmic space is a C(휏)- cosmic space. Proof: Let X be a C(휏)-cosmic space and A ⊆ X. Then there exists a collection K of closed subsets of X with the properties (1) for every open subset U of X and every x 2 U, there exists K 2 K such that x 2 K ⊆ U, and (2) jKj ≤ 휏. We consider the collection KA ≡ fA \ K : K 2 Kg of closed subsets of A. The family KA satisfies the properties (3) for every open subset U A of A and every x 2 U A, there A A A exists K 2 KA such that x 2 K ⊆ U , and (4) jKAj ≤ 휏. The fourth property is clear. For the third, we consider an open subset U A of A and an element x of U A. Then there exists an open neighborhood U of x in X such that U A = A \ U. By the first property, there exists an element K of K such that x 2 K ⊆ U. A A A A Setting K = A \ K, we have K 2 KA and x 2 K ⊆ U . □ Q Proposition 2.5. The product 휆2Λ X휆 of a family fX휆 : 휆 2 Λg of C(휏)-cosmic spaces, where jΛj ≤ 휏, is a C(휏)-cosmic space. Proof: For every family of C(휏)-cosmic spaces X휆, 휆 2 Λ, there exists a collection K휆 of closed subsets of X휆 with the properties (1) for every open subset U휆 of X휆 and every x 2 U휆, there exists K휆 2 K휆 such that x 2 K휆 ⊆ U휆, and (2) jK j ≤ 휏.
Recommended publications
  • Arxiv:1901.10987V3 [Math.GN] 5 Apr 2020 Set C Products
    THE COMETRIZABILITY OF GENERALIZED METRIC SPACES TARAS BANAKH AND YARYNA STELMAKH Abstract. A topological space X is cometrizable if it admits a weaker metrizable topology such that each point x ∈ X has a (not necessarily open) neighborhood base consisting of metrically closed sets. We study the relation of cometrizable spaces to other generalized metric spaces and prove that all as-cosmic spaces are cometrizable. Also, we present an example of a regular countable space of weight ω1, which is not cometrizable. Under ω1 = c this space contains no infinite compact subsets and hence is cs-cosmic. Under ω1 < p this countable space is Fr´echet-Urysohn and is not cs-cosmic. 1. Introduction In this paper we study the interplay between the class of cometrizable spaces and other classes of generalized metric spaces. A topological space X is called cometrizable if it admits a metrizable topology such that each point x ∈ X has a (not necessarily open) neighborhood base consisting of metrically closed sets. Equivalently, cometrizable spaces can be defined as spaces X for which there exists a bijective continuous map f : X → M to a metrizable space M such that for any open set U ⊆ X and point x ∈ U there exists a neighborhood V ⊆ X of x such that f −1(f(V )) ⊆ U. It is clear that each cometrizable space X is regular and submetrizable, i.e. admits a continuous bijective map onto a metrizable space. Cometrizable spaces were introduced by Gruenhage [21] who proved the following interest- ing implication of PFA, the Proper Forcing Axiom [6].
    [Show full text]
  • A Selection of Recent Results and Problems in Cp-Theory V
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector Topology and its Applications 154 (2007) 2465–2493 www.elsevier.com/locate/topol ✩ A selection of recent results and problems in Cp-theory V. V. T k ach u k Departamento de Matematicas, Universidad Autónoma Metropolitana, Av. San Rafael Atlixco, 186, Iztapalapa, A.P. 55-532, C.P. 09340, México, D.F., Mexico Received 19 December 2006; accepted 18 March 2007 Abstract The author presents five popular topics in Cp-theory giving their general description together with some unsolved problems. The main idea is to show the areas of major activities displaying what is being done nowadays and trying to outline the trends of their future development. A big percentage of the cited results and problems are new, i.e., published/obtained in the 21-st century. However, some classical old theorems and questions are also cited the author being convinced that they are worth to be repeated with a new emphasis due to what is achieved at the present time. © 2007 Elsevier B.V. All rights reserved. MSC: primary 54H11, 54C10, 22A05, 54D06; secondary 54D25, 54C25 Keywords: Compact space; Eberlein compact; Corson compact; Gul’ko space; Lindelöf Σ-property; Neighborhood assignments; Lindelöf property; D-space; Pseudocompact spaces; Countably compact spaces; t-equivalency; l-equivalency; d-separable space; Sokolov space 0. Introduction The first critical mass of results accumulated in Cp-theory dates back to the sixties and seventies of the last cen- tury. They mostly belong to specialists in Functional Analysis and serve specific purposes in their areas; however, it was soon noticed by topologists that quite a few theorems of Functional Analysis contained very interesting and nontrivial topological facts.
    [Show full text]
  • A NOTE on SPACES C P( X) K-ANALYTIC-FRAMED in X
    Bull. Austral. Math. Soc. 78 (2008), 141–146 doi:10.1017/S0004972708000567 X A NOTE ON SPACES C p(X) K-ANALYTIC-FRAMED IN R J. C. FERRANDO ˛ and J. K ˛AKOL (Received 1 October 2007) Abstract X This paper characterizes the K -analyticity-framedness in R for C p(X) (the space of real-valued continuous functions on X with pointwise topology) in terms of C p(X). This is used to extend 0 Tkachuk’s result about the K -analyticity of spaces C p(X) and to supplement the Arkhangel ski˘ı–Calbrix characterization of σ -compact cosmic spaces. A partial answer to an Arkhangel0ski˘ı–Calbrix problem is also provided. 2000 Mathematics subject classification: 54C35, 54H05. Keywords and phrases: P-framed space, cosmic space, K -analytic space, Lindelof¨ 6-space, angelic space. 1. Preliminaries Christensen [12] proved that a metric and separable space X is σ-compact if and only N if C p(X) is analytic, that is, a continuous image of the Polish space N . Calbrix [11] showed that a completely regular Hausdorff space X is σ-compact if C p(X) is analytic. The converse does not hold in general; for if ξ ∈ βN \ N and X = N ∪ {ξ}, where the set of natural numbers N is considered with the discrete topology, then C p(X) is a metrizable Baire space [17] but not even K -analytic by [22, p. 64]. A closely related result is given in [4]: A regular cosmic space X is σ-compact if and only if X C p(X) is K -analytic-framed in R , that is, there exists a K -analytic space Y such that X C p(X) ⊆ Y ⊆ R , although it was already known [18] that if X is σ -bounded (that is, X a countable union of functionally bounded sets), then C p(X) is Kσ δ-framed in R .
    [Show full text]
  • Arxiv:1910.05293V1 [Math.GN] 11 Oct 2019 Where Otne N[9,[0,[1,[2,[3,[4,[25]
    LUSIN AND SUSLIN PROPERTIES OF FUNCTION SPACES TARAS BANAKH AND LEIJIE WANG Abstract. A topological space is Suslin (Lusin) if it is a continuous (and bijective) image of a Polish space. For a Tychonoff space X let Cp(X), Ck(X) and C↓F(X) be the spaces of continuous real-valued functions on X, endowed with the topology of pointwise convergence, the compact-open topology, and the Fell hypograph topology, respectively. For a metrizable space X we prove the equivalence of the following statements: (1) X is σ-compact, (2) Cp(X) is Suslin, (3) Ck(X) is Suslin, (4) C↓F(X) is Suslin, (5) Cp(X) is Lusin, (6) Ck(X) is Lusin, (7) C↓F(X) is Lusin, (8) Cp(X) is Fσ-Lusin, (9) Ck(X) is Fσ-Lusin, (10) C↓F(X) is Cδσ- Lusin. Also we construct an example of a sequential ℵ0-space X with a unique non-isolated point such that the function spaces Cp(X), Ck(X) and C↓F(X) are not Suslin. 1. Introduction In this paper we study the descriptive properties of the spaces Cp(X), Ck(X) and C↓F(X) of continuous real-valued functions on a Tychonoff space X. The function space Cp(X) is the space C(X) of continuous real-valued functions on X, endowed with the topology of pointwise convergence. This topology is generated by the subbase consisting of the sets ⌊x; r⌋ := {f ∈ C(X) : f(x) > r} and ⌈x; r⌉ := {f ∈ C(X) : f(x) < r} where x ∈ X and r is a real number.
    [Show full text]
  • $\Mathfrak G $-Bases in Free (Locally Convex) Topological Vector Spaces
    G-BASES IN FREE (LOCALLY CONVEX) TOPOLOGICAL VECTOR SPACES TARAS BANAKH AND ARKADY LEIDERMAN Abstract. A topological space X is defined to have a local G-base if every point x ∈ X has a neighborhood base (Uα)α∈ωω such that Uβ ⊂ Uα for all α ≤ β in ωω . We prove that for every Tychonoff space X the following conditions are equivalent: (1) the free locally convex space L(X) of X has a local G-base; (2) the free topological vector space V(X) of X has a local G-base; (3) the finest uniformity U(X) of X admits a G-base and the function space C(X) is ωω-dominated. The conditions (1)–(3) imply that every metrizable continuous image of X is σ-compact and all finite powers of X are countably tight. If the space X is separable, then the conditions (1)–(3) imply that X is a countable union of compact metrizable spaces and (1)–(3) are equivalent to: (4) the finest uniformity U(X) of X has a G-base. If the space X is first-countable and perfectly normal, then the conditions (1)–(3) are equivalent to: (5) X is metrizable and σ-compact. If the space X is countable, then the conditions (1)–(4) are equivalent to: (6) the space X has a local G-base. If X is a k-space, then the conditions (1)–(3) are equivalent to: (7) the double function space Ck(Ck(X)) has a local G-base. Under ω1 < b the conditions (1)–(3) are equivalent to (8) the finest uniformity U(X) of X is ω-narrow and has a G-base.
    [Show full text]
  • Cosmic Convergence†
    COSMIC CONVERGENCE† R.T. Rockafellar Departments of Mathematics and Applied Mathematics University of Washington, Seattle Roger J-B Wets Department of Mathematics and Institute of Theoretical Dynamics University of California, Davis Abstract. We introduce a new notion of convergence for sets that plays a crucial role in the study of the preservation of set convergence under various operations. Keywords: set convergence, Painlev´e-Kuratowski convergence, cosmic convergence paracosmic convergence. Date: April 1, 1991 Version: February 18, 2007 † Research supported in part by grants from the National Science Foundation 1 A comprehensive approximation theory for optimization problems, variational inequal- ities, linear or nonlinear systems of equations (including differential equations) is ultimately rooted in the convergence theory for sets. This has been vividly demonstrated by the results obtained via epi-convergence (equivalently, Γ-convergence) for constrained opti- mization problems and the calculus of variations, via graphical convergence (equivalently, G-convergence) for differential equations, in particular for problems involving nonsmooth coefficients (e.g., for conductivity problems involving composite materials). Although set convergence, introduced by Painlev´e(between 1902 and 1905), has a long mathematical history, it is only during the last two decades that it has started to be viewed as a major tool for dealing with approximations in optimization, systems of equations and related objects. One of the major shortcomings of the theory, as developed mostly by point-set topologists (between 1930 and 1970), was the (somewhat arbitrary) restriction of many results to hyperspaces (spaces of sets) consisting of the subsets of compacta. Because epigraphs of functions and graphs of operators are typically unbounded sets, there was a need for a theory that was not specifically aimed at the convergence of bounded sets, and where the continuity of set-valued mappings was not defined to suit only the case when these mappings are bounded.
    [Show full text]
  • K-Analytic-Framed in X
    Bull. Austral. Math. Soc. 78 (2008), 141–146 doi:10.1017/S0004972708000567 X A NOTE ON SPACES C p(X) K-ANALYTIC-FRAMED IN R J. C. FERRANDO ˛ and J. K ˛AKOL (Received 1 October 2007) Abstract X This paper characterizes the K -analyticity-framedness in R for C p(X) (the space of real-valued continuous functions on X with pointwise topology) in terms of C p(X). This is used to extend 0 Tkachuk’s result about the K -analyticity of spaces C p(X) and to supplement the Arkhangel ski˘ı–Calbrix characterization of σ -compact cosmic spaces. A partial answer to an Arkhangel0ski˘ı–Calbrix problem is also provided. 2000 Mathematics subject classification: 54C35, 54H05. Keywords and phrases: P-framed space, cosmic space, K -analytic space, Lindelof¨ 6-space, angelic space. 1. Preliminaries Christensen [12] proved that a metric and separable space X is σ-compact if and only N if C p(X) is analytic, that is, a continuous image of the Polish space N . Calbrix [11] showed that a completely regular Hausdorff space X is σ-compact if C p(X) is analytic. The converse does not hold in general; for if ξ ∈ βN \ N and X = N ∪ {ξ}, where the set of natural numbers N is considered with the discrete topology, then C p(X) is a metrizable Baire space [17] but not even K -analytic by [22, p. 64]. A closely related result is given in [4]: A regular cosmic space X is σ-compact if and only if X C p(X) is K -analytic-framed in R , that is, there exists a K -analytic space Y such that X C p(X) ⊆ Y ⊆ R , although it was already known [18] that if X is σ -bounded (that is, X a countable union of functionally bounded sets), then C p(X) is Kσ δ-framed in R .
    [Show full text]
  • ON K-SPACES, Kr-SPACES and K(X)
    Pacific Journal of Mathematics ON k-SPACES, kR-SPACES AND k.X/ ERNEST A. MICHAEL Vol. 47, No. 2 February 1973 PACIFIC JOURNAL OF MATHEMATICS Vol. 47, No. 2, 1973 ON β-SPACES, ^-SPACES AND k(X) E. MICHAEL Two examples of Avspaces which are not A -spaces are constructed; one of them is a σ-compact cosmic space, and the other is an ^0-space. On the positive side, a theorem is proved which implies that every σ-compact ^0-space which is a &#-space must be a &-space. 1* Introduction* In this paper, we prove and extend some results which were announced in [8]. Recall that a topological space X is called a k-space if every subset of X, whose intersection with every compact K c X is relatively open in K, is open in X. (For example, locally compact spaces and first-countable spaces are Λ-spaces.) Analogously, a space X is a kB- space if it is completely regular and if every /: X—+R, whose re- striction to every compact KdX is continuous, is continuous on X. Clearly every completely regular &-space is a Z^-space. The converse is false, as was first shown by an example of M. Katetov which appeared in a paper by V. Ptak [15, p. 357]. That example, however, was not normal1^ and our first purpose in this note is to construct two examples which are normal,—in fact, regular Lindelof and thus paracompact. Both our examples are modifications of Katetov's example, which had, in turn, been previously introduced (for a different purpose) by J.
    [Show full text]
  • Topology Proceedings
    Topology Proceedings Web: http://topology.auburn.edu/tp/ Mail: Topology Proceedings Department of Mathematics & Statistics Auburn University, Alabama 36849, USA E-mail: [email protected] ISSN: 0146-4124 COPYRIGHT °c by Topology Proceedings. All rights reserved. TOPOLOGY PROCEEDINGS Volume 27, No. 2, 2003 Pages 411{427 IDEAL REFLECTIONS PAUL GARTSIDE, SINA GREENWOOD∗, AND DAVID MCINTYRE Abstract. A reflection theorem is a result of the form \if all small subsets of a space have property then the space itself has ". Typical \small" sets would beP those of cardinality P 1, the meager sets, or closed nowhere dense sets. We ab- stract≤ @ the properties of \small" necessary to ensure reflection of the countable chain condition, separability and the Lindel¨of property. We investigate when first and second countability reflect in meager sets. 1. Introduction A reflection theorem is a result of the form \if all small subsets of a space (in some class of spaces) have property then the space itself has ". If a reflectionC theorem holds for a propertyP , then one says \P reflects in small subsets (for the class )". Classically,P P C \small" has meant \of size !1". For example Hajnal and Juhasz ≤ [10] showed that second countability reflects in size !1 subsets; ≤ and Dow [7] proved that metrizability reflects in size !1 subsets for compact spaces. Reflection results are also important≤ in set theory, hence the emphasis on cardinality. 2000 Mathematics Subject Classification. Primary 54A35; Secondary 54D65, 54D30. Key words and phrases. Reflection, meager, closed nowhere dense, separable, countable chain condition, Lindel¨of,first countable, second countable, nowhere densely generated.
    [Show full text]