On the Generalization of the Lambert W Function
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Labeled Factorization of Integers
Labeled Factorization of Integers Augustine O. Munagi John Knopfmacher Centre for Applicable Analysis and Number Theory School of Mathematics, University of the Witwatersrand Wits 2050, Johannesburg, South Africa [email protected] Submitted: Jan 5, 2009; Accepted: Apr 16, 2009; Published: Apr 22, 2009 Mathematics Subject Classification: 11Y05, 05A05, 11B73, 11B13 Abstract The labeled factorizations of a positive integer n are obtained as a completion of the set of ordered factorizations of n. This follows a new technique for generating ordered factorizations found by extending a method for unordered factorizations that relies on partitioning the multiset of prime factors of n. Our results include explicit enumeration formulas and some combinatorial identities. It is proved that labeled factorizations of n are equinumerous with the systems of complementing subsets of {0, 1,...,n − 1}. We also give a new combinatorial interpretation of a class of generalized Stirling numbers. 1 Ordered and labeled factorization An ordered factorization of a positive integer n is a representation of n as an ordered product of integers, each factor greater than 1. The set of ordered factorizations of n will be denoted by F (n), and |F (n)| = f(n). For example, F (6) = {6, 2.3, 3.2}. So f(6) = 3. Every integer n> 1 has a canonical factorization into prime numbers p1,p2,..., namely m1 m2 mr n = p1 p2 ...pr , p1 <p2 < ··· <pr, mi > 0, 1 ≤ i ≤ r. (1) The enumeration function f(n) does not depend on the size of n but on the exponents mi. In particular we define Ω(n)= m1 + m2 + ··· + mr, Ω(1) = 0. -
A Subspace Theorem for Manifolds
A subspace theorem for manifolds Emmanuel Breuillard and Nicolas de Saxcé February 5, 2021 Abstract We prove a theorem that generalizes Schmidt’s Subspace Theorem in the context of metric diophantine approximation. To do so we reformulate the Subspace theorem in the framework of homogeneous dynamics by introducing and studying a slope formalism and the corresponding notion of semistability for diagonal flows. Introduction In 1972, Wolfgang Schmidt formulated his celebrated subspace theorem [32, Lemma 7], a far reaching generalization of results of Thue [37], Siegel [35], and Roth [28] on rational approximations to algebraic numbers. Around the same time, in his work on arithmeticity of lattices in Lie groups, Gregory Margulis [26] used the geometry of numbers to establish the recurrence of unipotent flows on the space of lattices GLd(R)=GLd(Z). More than two decades later, a quantita- tive refinement of this fact, the so-called quantitative non-divergence estimate, was used by Kleinbock and Margulis [18] in their solution to the Sprindzuk conjecture regarding the extremality of non-degenerate manifolds in metric dio- phantine approximation. As it turns out, these two remarkable results – the subspace theorem and the Sprindzuk conjecture – are closely related and can be understood together as statements about diagonal orbits in the space of lat- tices. In this paper we prove a theorem that generalizes both results at the same time. We also provide several applications. This marriage is possible thanks to a better understanding of the geometry lying behind the subspace theorem, in particular the notion of Harder-Narasimhan filtration for one-parameter di- agonal actions, which leads both to a dynamical reformulation of the original subspace theorem and to a further geometric understanding of the family of exceptional subspaces arising in Schmidt’s theorem. -
Black Holes with Lambert W Function Horizons
Black holes with Lambert W function horizons Moises Bravo Gaete,∗ Sebastian Gomezy and Mokhtar Hassainez ∗Facultad de Ciencias B´asicas,Universidad Cat´olicadel Maule, Casilla 617, Talca, Chile. y Facultad de Ingenier´ıa,Universidad Aut´onomade Chile, 5 poniente 1670, Talca, Chile. zInstituto de Matem´aticay F´ısica,Universidad de Talca, Casilla 747, Talca, Chile. September 17, 2021 Abstract We consider Einstein gravity with a negative cosmological constant endowed with distinct matter sources. The different models analyzed here share the following two properties: (i) they admit static symmetric solutions with planar base manifold characterized by their mass and some additional Noetherian charges, and (ii) the contribution of these latter in the metric has a slower falloff to zero than the mass term, and this slowness is of logarithmic order. Under these hypothesis, it is shown that, for suitable bounds between the mass and the additional Noetherian charges, the solutions can represent black holes with two horizons whose locations are given in term of the real branches of the Lambert W functions. We present various examples of such black hole solutions with electric, dyonic or axionic charges with AdS and Lifshitz asymptotics. As an illustrative example, we construct a purely AdS magnetic black hole in five dimensions with a matter source given by three different Maxwell invariants. 1 Introduction The AdS/CFT correspondence has been proved to be extremely useful for getting a better understanding of strongly coupled systems by studying classical gravity, and more specifically arXiv:1901.09612v1 [hep-th] 28 Jan 2019 black holes. In particular, the gauge/gravity duality can be a powerful tool for analyzing fi- nite temperature systems in presence of a background magnetic field. -
Universit`A Degli Studi Di Perugia the Lambert W Function on Matrices
Universita` degli Studi di Perugia Facolta` di Scienze Matematiche, Fisiche e Naturali Corso di Laurea Triennale in Informatica The Lambert W function on matrices Candidato Relatore MassimilianoFasi BrunoIannazzo Contents Preface iii 1 The Lambert W function 1 1.1 Definitions............................. 1 1.2 Branches.............................. 2 1.3 Seriesexpansions ......................... 10 1.3.1 Taylor series and the Lagrange Inversion Theorem. 10 1.3.2 Asymptoticexpansions. 13 2 Lambert W function for scalar values 15 2.1 Iterativeroot-findingmethods. 16 2.1.1 Newton’smethod. 17 2.1.2 Halley’smethod . 18 2.1.3 K¨onig’s family of iterative methods . 20 2.2 Computing W ........................... 22 2.2.1 Choiceoftheinitialvalue . 23 2.2.2 Iteration.......................... 26 3 Lambert W function for matrices 29 3.1 Iterativeroot-findingmethods. 29 3.1.1 Newton’smethod. 31 3.2 Computing W ........................... 34 3.2.1 Computing W (A)trougheigenvectors . 34 3.2.2 Computing W (A) trough an iterative method . 36 A Complex numbers 45 A.1 Definitionandrepresentations. 45 B Functions of matrices 47 B.1 Definitions............................. 47 i ii CONTENTS C Source code 51 C.1 mixW(<branch>, <argument>) ................. 51 C.2 blockW(<branch>, <argument>, <guess>) .......... 52 C.3 matW(<branch>, <argument>) ................. 53 Preface Main aim of the present work was learning something about a not- so-widely known special function, that we will formally call Lambert W function. This function has many useful applications, although its presence goes sometimes unrecognised, in mathematics and in physics as well, and we found some of them very curious and amusing. One of the strangest situation in which it comes out is in writing in a simpler form the function . -
Enciclopedia Matematica a Claselor De Numere Întregi
THE MATH ENCYCLOPEDIA OF SMARANDACHE TYPE NOTIONS vol. I. NUMBER THEORY Marius Coman INTRODUCTION About the works of Florentin Smarandache have been written a lot of books (he himself wrote dozens of books and articles regarding math, physics, literature, philosophy). Being a globally recognized personality in both mathematics (there are countless functions and concepts that bear his name), it is natural that the volume of writings about his research is huge. What we try to do with this encyclopedia is to gather together as much as we can both from Smarandache’s mathematical work and the works of many mathematicians around the world inspired by the Smarandache notions. Because this is too vast to be covered in one book, we divide encyclopedia in more volumes. In this first volume of encyclopedia we try to synthesize his work in the field of number theory, one of the great Smarandache’s passions, a surfer on the ocean of numbers, to paraphrase the title of the book Surfing on the ocean of numbers – a few Smarandache notions and similar topics, by Henry Ibstedt. We quote from the introduction to the Smarandache’work “On new functions in number theory”, Moldova State University, Kishinev, 1999: “The performances in current mathematics, as the future discoveries, have, of course, their beginning in the oldest and the closest of philosophy branch of nathematics, the number theory. Mathematicians of all times have been, they still are, and they will be drawn to the beaty and variety of specific problems of this branch of mathematics. Queen of mathematics, which is the queen of sciences, as Gauss said, the number theory is shining with its light and attractions, fascinating and facilitating for us the knowledge of the laws that govern the macrocosm and the microcosm”. -
Tropical Moduli Space of Rational Graphically Stable Curves 3
TROPICAL MODULI SPACE OF RATIONAL GRAPHICALLY STABLE CURVES ANDY FRY Abstract. We study moduli spaces of rational graphically stable tropical curves and a refinement given by radial alignment. Given a complete multipartite graph Γ, the moduli space of radially aligned Γ-stable tropical curves can be given the structure of a balanced fan. This fan structure coincides with the Bergman fan of the cycle matroid of Γ. 1. Introduction trop The moduli space M0,n is a cone complex which parameterizes leaf-labelled metric trees. Its structure is obtained by gluing positive orthants of Rn−3 corresponding to trivalent trees. Speyer and Sturmfels [14] give an embedding of this cone complex (in the context of phy- logenetic trees) into a real vector space as a balanced fan where each top-dimensional cone is assigned weight 1. In [1], Ardila and Klivans study phylogenetic trees and show that the trop fan structure of M0,n has a refinement which coincides with the Bergman fan of the cycle matroid of Kn−1, the complete graph on n − 1 vertices. As a generalization of Ardila and Klivans, it is shown by Cavalieri, Hampe, Markwig, and Ranganathan in [3] that the fan trop associated to the moduli space of rational heavy/light weighted stable tropical curves, M0,w , and the Bergman fan of a graphic matroid have the same support. The main result of this paper further generalizes their result by starting with stability conditions defined by a graph (reduced weight graph) rather than a weight vector. We trop introduce tropical rational graphically stable curves (Definition 3.12) and write M0,Γ as the moduli space of these curves. -
Partial Metrics, Quasi-Metrics and Oriented Hypercubes
General Weightable l1 Cones Hypercube Hamiltonian Sink References Partial Metrics, Quasi-metrics and Oriented Hypercubes Michel Deza Ecole Normale Superieure, Paris, and JAIST, Ishikawa General Weightable l1 Cones Hypercube Hamiltonian Sink References Overview 1 General quasi-semi-metrics 2 Weightable q-s-metrics and equivalent notions 3 l1 Quasi-metrics 4 The cones under consideration 5 Path quasi-metrics of oriented hypercubes 6 Hamiltonian orientations of hypercubes 7 Unique-sink orientations of hypercubes 8 References A weak quasi-metric is a quasi-semi-metric q with weak symmetry: q(x, y) = q(y, x) whenever q(y, x) = 0. An Albert quasi-metric is a quasi-semi-metric q with weak definiteness: x = y whenever q(x, y) = q(y, x) = 0. General Weightable l1 Cones Hypercube Hamiltonian Sink References Quasi-semi-metrics Given a set X , a function q : X × X → R≥0 with q(x, x)=0 is a quasi-distance (or, in Topology, prametric) on X . A quasi-distance q is a quasi-semi-metric if for x, y, z ∈ X it holds (oriented triangle inequality) q(x, y) ≤ q(x, z) + q(z, y) . q0 given by q0(x, y)=q(y, x) is dual quasi-semi-metric to q. (X , q) can be partially ordered by the specialization order: x y if and only if q(x, y)=0. Discrete quasi-metric on poset (X , ≤) is q≤(x, y)=0 if x y and =1 else; for (X , q≤), order coincides with ≤. General Weightable l1 Cones Hypercube Hamiltonian Sink References Quasi-semi-metrics Given a set X , a function q : X × X → R≥0 with q(x, x)=0 is a quasi-distance (or, in Topology, prametric) on X . -
The Strange Properties of the Infinite Power Tower Arxiv:1908.05559V1
The strange properties of the infinite power tower An \investigative math" approach for young students Luca Moroni∗ (August 2019) Nevertheless, the fact is that there is nothing as dreamy and poetic, nothing as radical, subversive, and psychedelic, as mathematics. Paul Lockhart { \A Mathematician's Lament" Abstract In this article we investigate some "unexpected" properties of the \Infinite Power Tower 1" function (or \Tetration with infinite height"): . .. xx y = f(x) = xx where the \tower" of exponentiations has an infinite height. Apart from following an initial personal curiosity, the material collected here is also intended as a potential guide for teachers of high-school/undergraduate students interested in planning an activity of \investigative mathematics in the classroom", where the knowledge is gained through the active, creative and cooperative use of diversified mathematical tools (and some ingenuity). The activity should possibly be carried on with a laboratorial style, with no preclusions on the paths chosen and undertaken by the students and with little or no information imparted from the teacher's desk. The teacher should then act just as a guide and a facilitator. The infinite power tower proves to be particularly well suited to this kind of learning activity, as the student will have to face a challenging function defined through a rather uncommon infinite recursive process. They'll then have to find the right strategies to get around the trickiness of this function and achieve some concrete results, without the help of pre-defined procedures. The mathematical requisites to follow this path are: functions, properties of exponentials and logarithms, sequences, limits and derivatives. -
Note on De Sitter Vacua from Perturbative and Non-Perturbative Dynamics in Type IIB/F-Theory Compactifications ∗ Vasileios Basiouris, George K
Physics Letters B 810 (2020) 135809 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Note on de Sitter vacua from perturbative and non-perturbative dynamics in type IIB/F-theory compactifications ∗ Vasileios Basiouris, George K. Leontaris Physics Department, University of Ioannina, 45110, Ioannina, Greece a r t i c l e i n f o a b s t r a c t Article history: The properties of the effective scalar potential are studied in the framework of type IIB string theory, Received 1 August 2020 taking into account perturbative and non-perturbative corrections. The former modify the Kähler Received in revised form 21 September potential and include α and logarithmic corrections generated when intersecting D7branes are part of 2020 the internal geometric configuration. The latter add exponentially suppressed Kähler moduli dependent Accepted 23 September 2020 terms to the fluxed superpotential. The possibility of partial elimination of such terms which may Available online 1 October 2020 happen for particular choices of world volume fluxes is also taken into account. That being the case, Editor: A. Volovichis a simple set up of three Kähler moduli is considered in the large volume regime, where only one of them is assumed to induce non-perturbative corrections. It is found that the shape of the F-term potential crucially depends on the parametric space associated with the perturbative sector and the volume modulus. De Sitter vacua can be obtained by implementing one of the standard mechanisms, i.e., either relying on D-terms related to U (1) symmetries associated with the D7branes, or introducing D3 branes. -
On the Lambert W Function and Its Utility in Biochemical Kinetics
Biochemical Engineering Journal 63 (2012) 116–123 Contents lists available at SciVerse ScienceDirect Biochemical Engineering Journal j ournal homepage: www.elsevier.com/locate/bej Review On the Lambert W function and its utility in biochemical kinetics ∗ Marko Golicnikˇ Institute of Biochemistry, Faculty of Medicine, University of Ljubljana, Vrazov trg 2, 1000 Ljubljana, Slovenia a r t i c l e i n f o a b s t r a c t Article history: This article presents closed-form analytic solutions to three illustrative problems in biochemical kinetics Received 6 October 2011 that have usually been considered solvable only by various numerical methods. The problems solved Received in revised form concern two enzyme-catalyzed reaction systems that obey diversely modified Michaelis–Menten rate 20 December 2011 equations, and biomolecule surface binding that is limited by mass transport. These problems involve Accepted 21 January 2012 the solutions of transcendental equations that include products of variables and their logarithms. Such Available online 3 February 2012 equations are solvable by the use of the Lambert W(x) function. Thus, these standard kinetics examples are solved in terms of W(x) to show the applicability of this commonly unknown function to the biochemical Keywords: Biokinetics community. Hence, this review first of all describes the mathematical definition and properties of the W(x) Biosensors function and its numerical evaluations, together with analytical approximations, and then it describes the Enzymes use of the W(x) function in biochemical kinetics. Other applications of the function in various engineering Integrated rate equation sciences are also cited, although not described. -
The Deranged Bell Numbers 2
THE DERANGED BELL NUMBERS BELBACHIR HACENE,` DJEMMADA YAHIA, AND NEMETH´ LASZL` O` Abstract. It is known that the ordered Bell numbers count all the ordered partitions of the set [n] = {1, 2,...,n}. In this paper, we introduce the de- ranged Bell numbers that count the total number of deranged partitions of [n]. We first study the classical properties of these numbers (generating function, explicit formula, convolutions, etc.), we then present an asymptotic behavior of the deranged Bell numbers. Finally, we give some brief results for their r-versions. 1. Introduction A permutation σ of a finite set [n] := {1, 2,...,n} is a rearrangement (linear ordering) of the elements of [n], and we denote it by σ([n]) = σ(1)σ(2) ··· σ(n). A derangement is a permutation σ of [n] that verifies σ(i) 6= i for all (1 ≤ i ≤ n) (fixed-point-free permutation). The derangement number dn denotes the number of all derangements of the set [n]. A simple combinatorial approach yields the two recursions for dn (see for instance [13]) dn = (n − 1)(dn−1 + dn−2) (n ≥ 2) and n dn = ndn−1 + (−1) (n ≥ 1), with the first values d0 = 1 and d1 = 0. The derangement number satisfies the explicit expression (see [3]) n (−1)i d = n! . n i! i=0 X The generating function of the sequence dn is given by tn e−t D(t)= dn = . arXiv:2102.00139v1 [math.GM] 30 Jan 2021 n! 1 − t n≥ X0 The first few values of dn are (dn)n≥0 = {1, 0, 1, 2, 9, 44, 265, 1854, 14833, 133496, 1334961,...}. -
On the Lambert W Function 329
On the Lambert W function 329 The text below is the same as that published in Advances in Computational Mathematics, Vol 5 (1996) 329 – 359, except for a minor correction after equation (1.1). The pagination matches the published version until the bibliography. On the Lambert W Function R. M. Corless1,G.H.Gonnet2,D.E.G.Hare3,D.J.Jeffrey1 andD.E.Knuth4 1Department of Applied Mathematics, University of Western Ontario, London, Canada, N6A 5B7 2Institut f¨ur Wissenschaftliches Rechnen, ETH Z¨urich, Switzerland 3Symbolic Computation Group, University of Waterloo, Waterloo, Canada, N2L 3G1 4Department of Computer Science, Stanford University, Stanford, California, USA 94305-2140 Abstract The Lambert W function is defined to be the multivalued inverse of the function w → wew. It has many applications in pure and applied mathematics, some of which are briefly described here. We present a new discussion of the complex branches of W ,an asymptotic expansion valid for all branches, an efficient numerical procedure for evaluating the function to arbitrary precision, and a method for the symbolic integration of expressions containing W . 1. Introduction In 1758, Lambert solved the trinomial equation x = q +xm by giving a series develop- ment for x in powers of q. Later, he extended the series to give powers of x as well [48,49]. In [28], Euler transformed Lambert’s equation into the more symmetrical form xα − xβ =(α − β)vxα+β (1.1) by substituting x−β for x and setting m = α/β and q =(α − β)v. Euler’s version of Lambert’s series solution was thus n 1 2 x =1+nv + 2 n(n + α + β)v + 1 n(n + α +2β)(n +2α + β)v3 6 (1.2) 1 4 + 24 n(n + α +3β)(n +2α +2β)(n +3α + β)v +etc.