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Let Mn, n ≥ 3, be a complete oriented minimal hypersurface in Euclidean space Rn+1. It is shown that, if the total scalar curvature on M is less than the n/2 power of 1/2Cs, where Cs is the Sobolev constant for M, and the square norm of the second fundamental form is a L2 function, then M is a hyperplane.
Let Ω be a convex planar domain, with no curvature or regularity assumption on the boundary. Let Nθ(R) = card{RΩθ∩ℤ2}, where Ωθ denotes the rotation of Ω by θ. It is proved that, up to a small logarithmic transgression, Nθ(R) = |Ω|R2 + O(R2/3), for almost every rotation. A refined result based on the fractal structure of the image of the boundary of Ω under the Gauss map is also obtained.
where φ denotes Euler's function. In this memoir we study the set w of sigmaphi numbers, that is, those composite natural numbers n which satisfy
The smallest such number is 65, and they appear to be moderately frequent. There are 290 sigma-phi numbers not exceeding 105 and 1,231 not exceeding 106. By comparison, we observe that the number of primes in these ranges is 9,592 and 78,498, respectively. Since the primes also satisfy the relationship (1.2) a sigma-phi number can be thought of as a kind of pseudo-prime. The motivation for studying sigma-phi numbers is that they should have similar properties to Carmichael numbers but be easier to study. A Carmichael number is a number n such that the least common multiple of the φ(pk) with pk||n divides n-1, i.e., by Korseldt's criterion, a number for which p-1||n-1 whenever p|n. The number of Carmichael numbers not exceeding 105 and 106 is 16 and 43, respectively. It seems that the counting functions for Carmichael and sigma-phi numbers have somewhat similar growth rates. The counts above are skewed by the fact that there are many sigma-phi numbers with exactly two prime factors but there are no Carmichael numbers of this kind.
In this paper we continue the investigation begun in [11]. Let λ1…., λs and μ1, …, μs be real numbers, and define the forms
Further, let τ be a positive real number. Our goal is to determine conditions under which the system of inequalities
has a non-trivial integral solution. As has frequently been the case in work on systems of diophantine inequalities (see, for example, Brüdern and Cook [6] and Cook [7]), we were forced in [11] to impose a condition requiring certain coefficient ratios to be algebraic. A recent paper of Bentkus and Gotze [4] introduced a method for avoiding such a restriction in the study of positivede finite quadratic forms, and these ideas are in fact flexible enough to be applied to other problems. In particular, Freeman [10] was able to adapt the method to obtain an asymptotic lower bound for the number of solutions of a single diophantine inequality, thus finally providing the expected strengthening of a classical theorem of Davenport and Heilbronn [9]. The purpose of the present note is to apply these new ideas to the system of inequalities (1.1).
This paper presents existence criteria for continuous and discrete boundary value problems on the infinite interval, using the notion of upper and lower solution.
A well-known result of Ehrenfeucht states that a difference polynomial f(X)-g(Y) in two variables X, Y with complex coefficients is irreducible if the degrees of f and g are coprime. Panaitopol and Stefǎnescu generalized this result, by giving an irreducibility condition for a larger class of polynomials called “generalized difference polynomials”. This paper gives an irreducibility criterion for more general polynomials, of which the criterion of Panaitopol and Stefǎnescu is a special case.
For k ≥ 2, a graph G is said to be k-vertex connected, or simply k-connected, when |V(G)| ≥ k + 1 and the removal of any k − 1 vertices (and any incident edges) from G does not result in a disconnected graph. We use 1-connected as a synonym for connected.
If a graph G with at least k + 1 vertices is not k-connected and the deletion of a set S of k − 1 vertices disconnects it, there is a partition of V(G) \ S into nonempty sets X, Y with no edges crossing (one end in X, one in Y). Let H and K be the subgraphs induced by X ∪ S and Y ∪ S, except that edges with both ends in S are to be put in one and only one of H or K. Then we obtain edge-disjoint subgraphs H and K whose union is G and such that |V(H)∩V(K)| = k − 1. Conversely, if such subgraphs H and K exist and each contains at least one more vertex than their intersection, then G is not k-connected.
A graph is said to be nonseparable when it is 2-connected and has no loops, or when it is a bond-graph (with two vertices and any positive number of edges joining them, including the link-graph with one such edge), a loop-graph (one edge joining a single vertex to itself), or a vertex-graph. All polygons, for example, are nonseparable; path-graphs or other trees with at least two edges are not.
The favorable reception of our book and its use for a variety of courses on combinatorial mathematics at numerous colleges and universities has encouraged us to prepare this second edition. We have added new material and have updated references for this version. A number of typographical and other errors have been corrected. We had to change “this century” to “the last century” in several places.
The new material has, for the most part, been inserted into the chapters with the same titles as in the first edition. An exception is that the material of the later chapters on graph theory has been reorganized into four chapters rather than two. The added material includes, for example, discussion of the Lovàsz sieve, associative block designs, and list colorings of graphs.
Many new problems have been added, and we hope that this last change, in particular, will increase the value of the book as a text. We have decided not to attempt to indicate in the book the level of difficulty of the various problems, but remark again that this can vary greatly. The difficulty will often depend on the experience and background of the reader, and an instructor will need to decide which exercises are appropriate for his or her students. We like the idea of stating problems at the point in the text where they are most relevant, but have also added some problems at the end of the chapters. It is not true that the problems appearing later are necessarily more difficult than those at the beginning of a chapter.
We shall first look at a few so-called coloring problems for graphs.
A proper coloring of a graph G is a function from the vertices to a set C of ‘colors’ (e.g. C = {1, 2, 3, 4}) such that the ends of every edge have distinct colors. (So a graph with a loop will admit no proper colorings.) If |C| = k, we say that G is k-colored.
The chromatic number χ(G) of a graph G is the minimal number of colors for which a proper coloring exists.
If χ(G) = 2 (or χ(G) = 1, which is the case when and only when G has no edges), then G is called bipartite. A graph with no odd polygons (equivalently, no closed paths of odd length) is bipartite as the reader should verify.
The famous ‘Four Color Theorem’ (K. Appel and W. Haken, 1977) states that if G is planar, then χ(G) ≤ 4.
Clearly χ(Kn) = n. If k is odd then χ(Pk) = 3. In the following theorem, we show that, with the exception of these examples, the chromatic number is at most equal to the maximum degree (R. L. Brooks, 1941).
Theorem 3.1.Let d ≥ 3 and let G be a graph in which all vertices have degree ≤ d and such that Kd+1 is not a subgraph of G. Then χ(G) ≤ d.
Proof 1: As is the case in many theorems in combinatorial analysis, one can prove the theorem by assuming that it is not true, then considering a minimal counterexample (in this case a graph with the minimal number of vertices) and arriving at a contradiction.
The following problem originated in communication theory. For a telephone network, a connection between terminals A and B is established before messages flow in either direction. For a network of computers it is desirable to be able to send a message from A to B without B knowing that a message is on its way. The idea is to let the message be preceded by some ‘address’ of B such that at each node of the network a decision can be made concerning the direction in which the message should proceed.
A natural thing to try is to give each vertex of a graph G a binary address, say in {0, 1}k, in such a way that the distance of two vertices in the graph is equal to the so-called Hamming distance of the addresses, i.e. the number of places where the addresses differ. This is equivalent to regarding G as an induced subgraph of the hypercube Hk, which has V(Hk) ≔ {0, 1}k and where k-tuples are adjacent when they differ in exactly one coordinate. The example G = K3 already shows that this is impossible. We now introduce a new alphabet {0,1, ⋆} and form addresses by taking n-tuples from this alphabet. The distance between two addresses is defined to be the number of places where one has a 0 and the other a 1 (so stars do not contribute to the distance).
In this chapter we give an introduction to a large and important area of combinatorial theory which is known as design theory. The most general object that is studied in this theory is a so-called incidence structure. This is a triple S = (P, B, I), where:
P is a set, the elements of which are called points;
B is a set, the elements of which are called blocks;
I is an incidence relation between P and B (i.e. I ⊆ P × B). The elements of I are called flags.
If (p, B) ∈ I, then we say that point p and block B are incident. We allow two different blocks B1 and B2 to be incident with the same subset of points of P. In this case one speaks of ‘repeated blocks’. If this does not happen, then the design is called a simple design and we can then consider blocks as subsets of P. In fact, from now on we shall always do that, taking care to realize that different blocks are possibly the same subset of P. This allows us to replace the notation (p, B) ∈ I by p ∈ B, and we shall often say that point p is ‘in block B’ instead of incident with B.
It has become customary to denote the cardinality of P by v and the cardinality of B by b.