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The Fact of Modern Mathematics: Geometry, Logic, and Concept Formation in Kant and Cassirer
THE FACT OF MODERN MATHEMATICS: GEOMETRY, LOGIC, AND CONCEPT FORMATION IN KANT AND CASSIRER by Jeremy Heis B.A., Michigan State University, 1999 Submitted to the Graduate Faculty of Arts and Sciences in partial fulfillment of the requirements for the degree of Doctor of Philosophy University of Pittsburgh 2007 UNIVERSITY OF PITTSBURGH COLLEGE OF ARTS AND SCIENCES This dissertation was presented by Jeremy Heis It was defended on September 5, 2007 and approved by Jeremy Avigad, Associate Professor, Philosophy, Carnegie Mellon University Stephen Engstrom, Associate Professor, Philosophy, University of Pittsburgh Anil Gupta, Distinguished Professor, Philosophy, University of Pittsburgh Kenneth Manders, Associate Professor, Philosophy, University of Pittsburgh Thomas Ricketts, Professor, Philosophy, University of Pittsburgh Dissertation Advisor: Mark Wilson, Professor, Philosophy, University of Pittsburgh ii Copyright © by Jeremy Heis 2007 iii THE FACT OF MODERN MATHEMATICS: GEOMETRY, LOGIC, AND CONCEPT FORMATION IN KANT AND CASSIRER Jeremy Heis, PhD University of Pittsburgh, 2007 It is now commonly accepted that any adequate history of late nineteenth and early twentieth century philosophy—and thus of the origins of analytic philosophy—must take seriously the role of Neo-Kantianism and Kant interpretation in the period. This dissertation is a contribution to our understanding of this interesting but poorly understood stage in the history of philosophy. Kant’s theory of the concepts, postulates, and proofs of geometry was informed by philosophical reflection on diagram-based geometry in the Greek synthetic tradition. However, even before the widespread acceptance of non-Euclidean geometry, the projective revolution in nineteenth century geometry eliminated diagrams from proofs and introduced “ideal” elements that could not be given a straightforward interpretation in empirical space. -
Geometry of the Mathieu Groups and Golay Codes
Proc. Indian Acad. Sci. (Math. Sci.), Vol. 98, Nos 2 and 3, December 1988, pp. 153-177. 9 Printed in India. Geometry of the Mathieu groups and Golay codes ERIC A LORD Centre for Theoretical Studies and Department of Applied Mathematics, Indian Institute of Science, Bangalore 560012, India MS received 11 January 1988 Abstraet. A brief review is given of the linear fractional subgroups of the Mathieu groups. The main part of the paper then deals with the proj~x-~tiveinterpretation of the Golay codes; these codes are shown to describe Coxeter's configuration in PG(5, 3) and Todd's configuration in PG(11, 2) when interpreted projectively. We obtain two twelve-dimensional representations of M24. One is obtained as the coUineation group that permutes the twelve special points in PC,(11, 2); the other arises by interpreting geometrically the automorphism group of the binary Golay code. Both representations are reducible to eleven-dimensional representations of M24. Keywords. Geometry; Mathieu groups; Golay codes; Coxeter's configuration; hemi- icosahedron; octastigms; dodecastigms. 1. Introduction We shall first review some of the known properties of the Mathieu groups and their linear fractional subgroups. This is mainly a brief resum6 of the first two of Conway's 'Three Lectures on Exceptional Groups' [3] and will serve to establish the notation and underlying concepts of the subsequent sections. The six points of the projective line PL(5) can be labelled by the marks of GF(5) together with a sixth symbol oo defined to be the inverse of 0. The symbol set is f~ = {0 1 2 3 4 oo}. -
LINEAR GROUPS AS RIGHT MULTIPLICATION GROUPS of QUASIFIELDS 3 Group T (Π) of Translations
LINEAR GROUPS AS RIGHT MULTIPLICATION GROUPS OF QUASIFIELDS GABOR´ P. NAGY Abstract. For quasifields, the concept of parastrophy is slightly weaker than isotopy. Parastrophic quasifields yield isomorphic translation planes but not conversely. We investigate the right multiplication groups of fi- nite quasifields. We classify all quasifields having an exceptional finite transitive linear group as right multiplication group. The classification is up to parastrophy, which turns out to be the same as up to the iso- morphism of the corresponding translation planes. 1. Introduction A translation plane is often represented by an algebraic structure called a quasifield. Many properties of the translation plane can be most easily understood by looking at the appropriate quasifield. However, isomorphic translation planes can be represented by nonisomorphic quasifields. Further- more, the collineations do not always have a nice representation in terms of operations in the quasifields. Let p be a prime number and (Q, +, ·) be a quasifield of finite order pn. Fn We identify (Q, +) with the vector group ( p , +). With respect to the multiplication, the set Q∗ of nonzero elements of Q form a loop. The right multiplication maps of Q are the maps Ra : Q → Q, xRa = x · a, where Fn a, x ∈ Q. By the right distributive law, Ra is a linear map of Q = p . Clearly, R0 is the zero map. If a 6= 0 then Ra ∈ GL(n,p). In geometric context, the set of right translations are also called the slope set or the spread set of the quasifield Q, cf. [6, Chapter 5]. The right multiplication group RMlt(Q) of the quasifield Q is the linear group generated by the nonzero right multiplication maps. -
Spanning Sets and Scattering Sets in Steiner Triple Systems
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector JOURNAL OF COMBINATORIAL THEORY, %XieS A 57, 4659 (1991) Spanning Sets and Scattering Sets in Steiner Triple Systems CHARLESJ. COLBOURN Department of Combinatorics and Optimization, University of Waterloo, Waterloo. Ontario, N2L 3G1, Canada JEFFREYH. DMTZ Department of Mathematics, University of Vermont, Burlington, Vermont 05405 AND DOUGLASR. STINSON Department of Computer Science, University of Manitoba, Winnipeg, Manitoba, R3T 2N2, Canada Communicated by the Managing Editors Received August 15, 1988 A spanning set in a Steiner triple system is a set of elements for which each element not in the spanning set appears in at least one triple with a pair of elements from the spanning set. A scattering set is a set of elements that is independent, and for which each element not in the scattering set is in at most one triple with a pair of elements from the scattering set. For each v = 1,3 (mod 6), we exhibit a Steiner triple system with a spanning set of minimum cardinality, and a Steiner triple system with a scattering set of maximum cardinality. In the process, we establish the existence of Steiner triple systems with complete arcs of the minimum possible cardinality. 0 1991 Academic Press, Inc. 1. BACKGROUND A Steiner triple system of order u, or STS(u), is a v-element set V, and a set g of 3-element subsets of V called triples, for which each pair of elements from V appears in precisely one triple of 9% For XG V, the spannedsetV(X)istheset {~EV\X:{~,~,~)E~,~,~EX}.A~~~XEV 46 0097-3165/91 $3.00 Copyright 0 1991 by Academic Press, Inc. -
Probabilistic Combinatorics and the Recent Work of Peter Keevash
BULLETIN (New Series) OF THE AMERICAN MATHEMATICAL SOCIETY Volume 54, Number 1, January 2017, Pages 107–116 http://dx.doi.org/10.1090/bull/1553 Article electronically published on September 14, 2016 PROBABILISTIC COMBINATORICS AND THE RECENT WORK OF PETER KEEVASH W. T. GOWERS 1. The probabilistic method A graph is a collection of points, or vertices, some of which are joined together by edges. Graphs can be used to model a wide range of phenomena: whenever you have a set of objects such that any two may or may not be related in a certain way, then you have a graph. For example, the vertices could represent towns and the edges could represent roads from one town to another, or the vertices could represent people, with an edge joining two people if they know each other, or the vertices could represent countries, with an edge joining two countries if they border each other, or the vertices could represent websites, with edges representing links from one site to another (in this last case the edges have directions—a link is from one website to another—so the resulting mathematical structure is called a directed graph). Mathematically, a graph is a very simple object. It can be defined formally as simply a set V of vertices and a set E of unordered pairs of vertices from V .For example, if we take V = {1, 2, 3, 4} and E = {12, 23, 34, 14} (using ab as shorthand for {a, b}), then we obtain a graph known as the 4-cycle. Despite the simplicity and apparent lack of structure of a general graph, there turn out to be all sorts of interesting questions one can ask about them. -
A Conjecture of Berge About Linear Hypergraphs and Steiner Systems S(2; 4;V)
CORE Metadata, citation and similar papers at core.ac.uk Provided by Elsevier - Publisher Connector Discrete Mathematics 255 (2002) 125–133 www.elsevier.com/locate/disc A conjecture of Berge about linear hypergraphs and Steiner systems S(2; 4;v) Lucia Gionfriddo∗ Department of Mathematics, University of Catania, Viale A. Doria 6, 95125 Catania, Italy Received 5 April 1999; received in revised form 23 February 2000; accepted 26 June 2000 Abstract A famous conjecture of Berge about linear hypergraphs is studied. It is proved that all nearly resolvable Steiner systems S(2; 4;v) and all almost nearly resolvable S(2; 4;v) verify this conjecture. c 2002 Elsevier Science B.V. All rights reserved. Keywords: Combinatorics; Hypergraphs; Designs 1. Introduction A hypergraph is a pair H =(X; E), where X is a ÿnite non-empty set and E is a collection of subsets E ⊆ X , such that E = ∅, for every E ∈E, and E∈E E = X . The elements of X are called the points (or vertices)ofH, the elements of E are called the edges of H. A hypergraph H is called k-uniform if all its edges have exactly k distinct elements. For k = 2, hypergraphs are called graphs. The degree of a point x ∈ X is the number of edges containing x. A hypergraph is called linear if any two of its edges share at most one vertex. The heredity Hˆof H is the hypergraph having the same point-set of H and its edge-set is the family of all non- empty subsets of the edges of H. -
Steiner Systems S(2,4,V)
Steiner systems S(2, 4,v) - a survey Colin Reid, [email protected] Alex Rosa, [email protected] Department of Mathematics and Statistics, McMaster University, Hamilton, Ontario, Canada Submitted: Jan 21, 2009; Accepted: Jan 25, 2010; Published: Feb 1, 2010 Mathematics Subject Classification: 05B05 Abstract We survey the basic properties and results on Steiner systems S(2, 4, v), as well as open problems. 1 Introduction A Steiner system S(t, k, v) is a pair (V, ) where V is a v-element set and is a family of k-element subsets of V called blocks suchB that each t-element subset of V Bis contained in exactly one block. For basic properties and results on Steiner systems, see [51]. By far the most popular and most studied Steiner systems are those with t = 2 and k = 3, called Steiner triple systems (STS). There exists a very extensive literature on STSs (see, eg., [54] and the bibliography therein). Steiner systems with t = 3 and k =4 are known as Steiner quadruple systems and are commonly abbreviated as SQS; there exist (at least) two extensive surveys on SQSs (see [122], [95]); see also [51]). When t = 2, one often speaks of a Steiner 2-design. Quite a deal of attention has also been paid to the case of Steiner systems S(2, 4, v), but to the best of our knowledge, no survey of known results and problems on these Steiner 2-designs with block size 4 has been published. It is the purpose of this article to fill this gap by bringing together known results and problems on this quite interesting class of Steiner systems. -
Finite Semifields and Nonsingular Tensors
FINITE SEMIFIELDS AND NONSINGULAR TENSORS MICHEL LAVRAUW Abstract. In this article, we give an overview of the classification results in the theory of finite semifields1and elaborate on the approach using nonsingular tensors based on Liebler [52]. 1. Introduction and classification results of finite semifields 1.1. Definition, examples and first classification results. Finite semifields are a generalisation of finite fields (where associativity of multiplication is not assumed) and the study of finite semifields originated as a classical part of algebra in the work of L. E. Dickson and A. A. Albert at the start of the 20th century. Remark 1.1. The name semifield was introduced by Knuth in his dissertation ([41]). In the literature before that, the algebraic structure, satisfying (S1)-(S4), was called a distributive quasifield, a division ring or a division algebra. Since the 1970's the use of the name semifields has become the standard. Due to the Dickson-Wedderburn Theorem which says that each finite skew field is a field (see [36, Section 2] for some historical remarks), finite semifields are in some sense the algebraic structures closest to finite fields. It is therefore not surprising that Dickson took up the study of finite semifields shortly after the classification of finite fields at the end of the 19th century (announced by E. H. Moore on the International Congress for Mathematicians in Chicago in 1893). Remark 1.2. In the remainder of this paper we only consider finite semifields (unless stated otherwise) and finiteness will often be assumed implicitly. In the infinite case, the octonions (see e.g. -
Strongly Minimal Steiner Systems Ii: Coordinatization and Quasigroups
STRONGLY MINIMAL STEINER SYSTEMS II: COORDINATIZATION AND QUASIGROUPS JOHN T. BALDWIN UNIVERSITY OF ILLINOIS AT CHICAGO Abstract. We note that a strongly minimal Steiner k-Steiner system (M; R) from [BP20] can be `coordinatized' in the sense of [GW75] by a quasigroup if k is a prime-power. But for the basic construction this coordinatization is never definable in (M; R). Nevertheless, by refining the construction, if k is a prime power there is a (2; k)-variety of quasigroups which is strongly minimal and definably coordinatizes a Steiner k-system. A linear space is collection of points and lines that satisfy a minimal condition to call a structure a geometry: two points determine a line. A linear space is a Steiner k-system if every line (block) has cardinality k. Such mathematicians as Steiner, Bose, Skolem, Bruck have established deep connections between the existence of a Steiner system with v points and blocks of size k and divisibility relations among k and v. A strongly minimal theory is a complete first order theory such that every defin- able set is finite or cofinite. They are the building blocks of @1-categorical theories. Alternatively, in a strongly minimal theory T the model theoretic notion of alge- braic closure1 determines a combinatorial geometry (matroid). Zilber conjectured S that these geometries were all discrete (acl(A) = a2A φ(x; a)), locally modular (group-like) or field-like. The examples here are based on Hrushovki's construction refuting this conjecture [Hru93]. These counterexamples, with ‘flat2 geometries' [Hru93, Section 4.2], have generally been regarded as an incohate class of exotic structures. -
Locally Symmetric Designs
PETER J. CAMERON LOCALLY SYMMETRIC DESIGNS A design (or balanced incomplete block design) D is locally symmetric if, for any point p, the lines and blocks through p form a symmetric design D*(p). Equivalently, D is locally symmetric if the number of blocks con- taining three non-eollinear points and the number of points in two non- disjoint blocks are both nonzero constants. The main result of this paper is: THEOREM 1. If D is a locally symmetric design with parameters v, k, 2, in which a line has s+ 1 points and three non-collinear points are contained in t blocks, then exactly one of the following occurs: O) D is the design of points and hyperplanes in a projective geometry of dimension at least 3 over GF(s) ; (ii) D is the design of points and hyperplanes in an affine geometry of dimension at least 3 over GF(s + 1), s> 1 ; (iii) D is a Hadamard 3-design (s= 1, v= 4( t + 1), k = 2( t + 1), 2=2t+ 1 ; (iv) v=(1 +st) (2s2+2s+l +(3s+2)s2t+s't2), k=(1 +st) (1 +s+s2t), 2=l +(2s+l)t+s2t 2, and/fs>l and t>l then t>s+2 and s+l divides t(t--1); (v) t= 1, v =(s+ 1)" (s3+ 2s2+ 3s+ l), k = (s+ my s + 1), 2=s3+ +3s2+4s+3; (vi) s=l, t=3, v=496, k=40, 2=39. Some special cases of this result have already been proved. It is known, for example, when D is symmetric (Dembowski and Wagner [10]), affme (Dernbowski [7], [8]), an extension of a symmetric design (the case s = 1 : Cameron [4]), locally a projective plane (the case t = 1 : Doyen and Hubaut [11 ]), or locally a projective geometry of dimension at least 3 (essentially [11 ]; this also follows from results of Kantor [16]). -
Finite Semifields
i “LavrauwPolverino” — 2010/2/12 — 11:49 — page 125 — #1 i i i In: Current research topics in Galois geometry ISBN 0000000000 Editors: J. De Beule, L. Storme, pp. 125-152 c 2010 Nova Science Publishers, Inc. 1 Chapter 6 2 FINITE SEMIFIELDS ∗† ‡ 3 Michel Lavrauw and Olga Polverino 4 1 Introduction and preliminaries 5 In this chapter, we concentrate on the links between Galois geometry and a particular kind 6 of non-associative algebras of finite dimension over a finite field F, called finite semifields. 7 Although in the earlier literature (predating 1965) the term semifields was not used, the 8 study of these algebras was initiated about a century ago by Dickson [32], shortly after 9 the classification of finite fields, taking a purely algebraic point of view. Nowadays it is 10 common to use the term semifields introduced by Knuth [59] in 1965 with the following 11 motivation: 12 “We are concerned with a certain type of algebraic system, called a semifield. Such a 13 system has several names in the literature, where it is called, for example, a "nonassocia- 14 tive division ring" or a "distributive quasifield". Since these terms are rather lengthy, and 15 since we make frequent reference to such systems in this paper, the more convenient name 16 semifield will be used." 17 By now, the theory of semifields has become of considerable interest in many different 18 areas of mathematics. Besides the numerous links with finite geometry, most of which con- 19 sidered here, semifields arise in the context of difference sets, coding theory, cryptography, 20 and group theory. -
Embedding Steiner Triple Systems Into Steiner Systems S(2;4;V)
Discrete Mathematics 274 (2004) 199–212 www.elsevier.com/locate/disc Embedding Steiner triple systems into Steiner systems S(2; 4;v) Mariusz Meszkaa , Alexander Rosab aDepartment of Applied Mathematics, AGH Krakow, Krakow, Poland bDepartment of Mathematics and Statistics, McMaster University, Hamilton, Ontario, Canada L8S 4K1 Received 26 March 2002; received in revised form 13 November 2002; accepted 3 December 2002 Abstract We initiate a systematic study of embeddings of Steiner triple systems into Steiner systems S(2; 4;v). We settle the existence of an embedding of the unique STS(7) and, with one possible exception, of the unique STS(9) into S(2; 4;v). We also obtain bounds for embedding sizes of Steiner triple systems of larger orders. c 2003 Elsevier B.V. All rights reserved. Keywords: Steiner triple systems; Steiner systems S(2; 4;v); Embedding 1. Introduction A Steiner system S(t; k; v) is a pair (V; B) where V is a v-set, v¿0, and B is a collection of k-subsets of V called blocks such that each t-subset of V is contained in exactly one block. A Steiner system S(2; 3;v) is called a Steiner triple system of order v, brie5y STS(v). If we replace in the above deÿnition the words “exactly one” with “at most one”, we obtain the deÿnition of a partial Steiner system S(t; k; v). It is well known that an STS(v) exists if and only if v ≡ 1; 3 (mod 6) [3], and that an S(2; 4;w) exists if and only if w ≡ 1; 4 (mod 12).