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Branch Points and Cuts in the Complex Plane
BRANCH POINTS AND CUTS IN THE COMPLEX PLANE Link to: physicspages home page. To leave a comment or report an error, please use the auxiliary blog and include the title or URL of this post in your comment. Post date: 6 July 2021. We’ve looked at contour integration in the complex plane as a technique for evaluating integrals of complex functions and finding infinite integrals of real functions. In some cases, the complex functions that are to be integrated are multi- valued. As a preliminary to the contour integration of such functions, we’ll look at the concepts of branch points and branch cuts here. The stereotypical function that is used to introduce branch cuts in most books is the complex logarithm function logz which is defined so that elogz = z (1) If z is real and positive, this reduces to the familiar real logarithm func- tion. (Here I’m using natural logs, so the real natural log function is usually written as ln. In complex analysis, the term log is usually used, so be careful not to confuse it with base 10 logs.) To generalize it to complex numbers, we write z in modulus-argument form z = reiθ (2) and apply the usual rules for taking a log of products and exponentials: logz = logr + iθ (3) = logr + iargz (4) To see where problems arise, suppose we start with z on the positive real axis and increase θ. Everything is fine until θ approaches 2π. When θ passes 2π, the original complex number z returns to its starting value, as given by 2. -
Asymptotic Estimates of Stirling Numbers
Asymptotic Estimates of Stirling Numbers By N. M. Temme New asymptotic estimates are given of the Stirling numbers s~mJ and (S)~ml, of first and second kind, respectively, as n tends to infinity. The approxima tions are uniformly valid with respect to the second parameter m. 1. Introduction The Stirling numbers of the first and second kind, denoted by s~ml and (S~~m>, respectively, are defined through the generating functions n x(x-l)···(x-n+l) = [. S~m)Xm, ( 1.1) m= 0 n L @~mlx(x -1) ··· (x - m + 1), ( 1.2) m= 0 where the left-hand side of (1.1) has the value 1 if n = 0; similarly, for the factors in the right-hand side of (1.2) if m = 0. This gives the 'boundary values' Furthermore, it is convenient to agree on s~ml = @~ml= 0 if m > n. The Stirling numbers are integers; apart from the above mentioned zero values, the numbers of the second kind are positive; those of the first kind have the sign of ( - l)n + m. Address for correspondence: Professor N. M. Temme, CWI, P.O. Box 4079, 1009 AB Amsterdam, The Netherlands. e-mail: [email protected]. STUDIES IN APPLIED MATHEMATICS 89:233-243 (1993) 233 Copyright © 1993 by the Massachusetts Institute of Technology Published by Elsevier Science Publishing Co., Inc. 0022-2526 /93 /$6.00 234 N. M. Temme Alternative generating functions are [ln(x+1)r :x n " s(ln)~ ( 1.3) m! £..,, n n!' n=m ( 1.4) The Stirling numbers play an important role in difference calculus, combina torics, and probability theory. -
Riemann Surfaces
RIEMANN SURFACES AARON LANDESMAN CONTENTS 1. Introduction 2 2. Maps of Riemann Surfaces 4 2.1. Defining the maps 4 2.2. The multiplicity of a map 4 2.3. Ramification Loci of maps 6 2.4. Applications 6 3. Properness 9 3.1. Definition of properness 9 3.2. Basic properties of proper morphisms 9 3.3. Constancy of degree of a map 10 4. Examples of Proper Maps of Riemann Surfaces 13 5. Riemann-Hurwitz 15 5.1. Statement of Riemann-Hurwitz 15 5.2. Applications 15 6. Automorphisms of Riemann Surfaces of genus ≥ 2 18 6.1. Statement of the bound 18 6.2. Proving the bound 18 6.3. We rule out g(Y) > 1 20 6.4. We rule out g(Y) = 1 20 6.5. We rule out g(Y) = 0, n ≥ 5 20 6.6. We rule out g(Y) = 0, n = 4 20 6.7. We rule out g(C0) = 0, n = 3 20 6.8. 21 7. Automorphisms in low genus 0 and 1 22 7.1. Genus 0 22 7.2. Genus 1 22 7.3. Example in Genus 3 23 Appendix A. Proof of Riemann Hurwitz 25 Appendix B. Quotients of Riemann surfaces by automorphisms 29 References 31 1 2 AARON LANDESMAN 1. INTRODUCTION In this course, we’ll discuss the theory of Riemann surfaces. Rie- mann surfaces are a beautiful breeding ground for ideas from many areas of math. In this way they connect seemingly disjoint fields, and also allow one to use tools from different areas of math to study them. -
Asymptotics of Singularly Perturbed Volterra Type Integro-Differential Equation
Konuralp Journal of Mathematics, 8 (2) (2020) 365-369 Konuralp Journal of Mathematics Journal Homepage: www.dergipark.gov.tr/konuralpjournalmath e-ISSN: 2147-625X Asymptotics of Singularly Perturbed Volterra Type Integro-Differential Equation Fatih Say1 1Department of Mathematics, Faculty of Arts and Sciences, Ordu University, Ordu, Turkey Abstract This paper addresses the asymptotic behaviors of a linear Volterra type integro-differential equation. We study a singular Volterra integro equation in the limiting case of a small parameter with proper choices of the unknown functions in the equation. We show the effectiveness of the asymptotic perturbation expansions with an instructive model equation by the methods in superasymptotics. The methods used in this study are also valid to solve some other Volterra type integral equations including linear Volterra integro-differential equations, fractional integro-differential equations, and system of singular Volterra integral equations involving small (or large) parameters. Keywords: Singular perturbation, Volterra integro-differential equations, asymptotic analysis, singularity 2010 Mathematics Subject Classification: 41A60; 45M05; 34E15 1. Introduction A systematic approach to approximation theory can find in the subject of asymptotic analysis which deals with the study of problems in the appropriate limiting regimes. Approximations of some solutions of differential equations, usually containing a small parameter e, are essential in the analysis. The subject has made tremendous growth in recent years and has a vast literature. Developed techniques of asymptotics are successfully applied to problems including the classical long-standing problems in mathematics, physics, fluid me- chanics, astrodynamics, engineering and many diverse fields, for instance, see [1, 2, 3, 4, 5, 6, 7]. There exists a plethora of examples of asymptotics which includes a wide variety of problems in rich results from the very practical to the highly theoretical analysis. -
The Monodromy Groups of Schwarzian Equations on Closed
Annals of Mathematics The Monodromy Groups of Schwarzian Equations on Closed Riemann Surfaces Author(s): Daniel Gallo, Michael Kapovich and Albert Marden Reviewed work(s): Source: Annals of Mathematics, Second Series, Vol. 151, No. 2 (Mar., 2000), pp. 625-704 Published by: Annals of Mathematics Stable URL: http://www.jstor.org/stable/121044 . Accessed: 15/02/2013 18:57 Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at . http://www.jstor.org/page/info/about/policies/terms.jsp . JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. Annals of Mathematics is collaborating with JSTOR to digitize, preserve and extend access to Annals of Mathematics. http://www.jstor.org This content downloaded on Fri, 15 Feb 2013 18:57:11 PM All use subject to JSTOR Terms and Conditions Annals of Mathematics, 151 (2000), 625-704 The monodromy groups of Schwarzian equations on closed Riemann surfaces By DANIEL GALLO, MICHAEL KAPOVICH, and ALBERT MARDEN To the memory of Lars V. Ahlfors Abstract Let 0: 7 (R) -* PSL(2, C) be a homomorphism of the fundamental group of an oriented, closed surface R of genus exceeding one. We will establish the following theorem. THEOREM. Necessary and sufficient for 0 to be the monodromy represen- tation associated with a complex projective stucture on R, either unbranched or with a single branch point of order 2, is that 0(7ri(R)) be nonelementary. -
An Introduction to Asymptotic Analysis Simon JA Malham
An introduction to asymptotic analysis Simon J.A. Malham Department of Mathematics, Heriot-Watt University Contents Chapter 1. Order notation 5 Chapter 2. Perturbation methods 9 2.1. Regular perturbation problems 9 2.2. Singular perturbation problems 15 Chapter 3. Asymptotic series 21 3.1. Asymptotic vs convergent series 21 3.2. Asymptotic expansions 25 3.3. Properties of asymptotic expansions 26 3.4. Asymptotic expansions of integrals 29 Chapter 4. Laplace integrals 31 4.1. Laplace's method 32 4.2. Watson's lemma 36 Chapter 5. Method of stationary phase 39 Chapter 6. Method of steepest descents 43 Bibliography 49 Appendix A. Notes 51 A.1. Remainder theorem 51 A.2. Taylor series for functions of more than one variable 51 A.3. How to determine the expansion sequence 52 A.4. How to find a suitable rescaling 52 Appendix B. Exam formula sheet 55 3 CHAPTER 1 Order notation The symbols , o and , were first used by E. Landau and P. Du Bois- Reymond and areOdefined as∼ follows. Suppose f(z) and g(z) are functions of the continuous complex variable z defined on some domain C and possess D ⊂ limits as z z0 in . Then we define the following shorthand notation for the relative!propertiesD of these functions in the limit z z . ! 0 Asymptotically bounded: f(z) = (g(z)) as z z ; O ! 0 means that: there exists constants K 0 and δ > 0 such that, for 0 < z z < δ, ≥ j − 0j f(z) K g(z) : j j ≤ j j We say that f(z) is asymptotically bounded by g(z) in magnitude as z z0, or more colloquially, and we say that f(z) is of `order big O' of g(z). -
A Note on the Asymptotic Expansion of the Lerch's Transcendent Arxiv
A note on the asymptotic expansion of the Lerch’s transcendent Xing Shi Cai∗1 and José L. Lópezy2 1Department of Mathematics, Uppsala University, Uppsala, Sweden 2Departamento de Estadística, Matemáticas e Informática and INAMAT, Universidad Pública de Navarra, Pamplona, Spain June 5, 2018 Abstract In [7], the authors derived an asymptotic expansion of the Lerch’s transcendent Φ(z; s; a) for large jaj, valid for <a > 0, <s > 0 and z 2 C n [1; 1). In this paper we study the special case z ≥ 1 not covered in [7], deriving a complete asymptotic expansion of the Lerch’s transcendent Φ(z; s; a) for z > 1 and <s > 0 as <a goes to infinity. We also show that when a is a positive integer, this expansion is convergent for Pm n s <z ≥ 1. As a corollary, we get a full asymptotic expansion for the sum n=1 z =n for fixed z > 1 as m ! 1. Some numerical results show the accuracy of the approximation. 1 Introduction The Lerch’s transcendent (Hurwitz-Lerch zeta function) [2, §25.14(i)] is defined by means of the power series 1 X zn Φ(z; s; a) = ; a 6= 0; −1; −2;:::; (a + n)s n=0 on the domain jzj < 1 for any s 2 C or jzj ≤ 1 for <s > 1. For other values of the variables arXiv:1806.01122v1 [math.CV] 4 Jun 2018 z; s; a, the function Φ(z; s; a) is defined by analytic continuation. In particular [7], 1 Z 1 xs−1e−ax Φ(z; s; a) = −x dx; <a > 0; z 2 C n [1; 1) and <s > 0: (1) Γ(s) 0 1 − ze ∗This work is supported by the Knut and Alice Wallenberg Foundation and the Ministerio de Economía y Competitividad of the spanish government (MTM2017-83490-P). -
NM Temme 1. Introduction the Incomplete Gamma Functions Are Defined by the Integrals 7(A,*)
Methods and Applications of Analysis © 1996 International Press 3 (3) 1996, pp. 335-344 ISSN 1073-2772 UNIFORM ASYMPTOTICS FOR THE INCOMPLETE GAMMA FUNCTIONS STARTING FROM NEGATIVE VALUES OF THE PARAMETERS N. M. Temme ABSTRACT. We consider the asymptotic behavior of the incomplete gamma func- tions 7(—a, —z) and r(—a, —z) as a —► oo. Uniform expansions are needed to describe the transition area z ~ a, in which case error functions are used as main approximants. We use integral representations of the incomplete gamma functions and derive a uniform expansion by applying techniques used for the existing uniform expansions for 7(0, z) and V(a,z). The result is compared with Olver's uniform expansion for the generalized exponential integral. A numerical verification of the expansion is given. 1. Introduction The incomplete gamma functions are defined by the integrals 7(a,*)= / T-Vcft, r(a,s)= / t^e^dt, (1.1) where a and z are complex parameters and ta takes its principal value. For 7(0,, z), we need the condition ^Ra > 0; for r(a, z), we assume that |arg2:| < TT. Analytic continuation can be based on these integrals or on series representations of 7(0,2). We have 7(0, z) + r(a, z) = T(a). Another important function is defined by 7>>*) = S7(a,s) = =^ fu^e—du. (1.2) This function is a single-valued entire function of both a and z and is real for pos- itive and negative values of a and z. For r(a,z), we have the additional integral representation e-z poo -zt j.-a r(a, z) = — r / dt, ^a < 1, ^z > 0, (1.3) L [i — a) JQ t ■+■ 1 which can be verified by differentiating the right-hand side with respect to z. -
Physics 112 Mathematical Notes Winter 2000 1. Power Series
Physics 112 Mathematical Notes Winter 2000 1. Power Series Expansion of the Fermi-Dirac Integral The Fermi-Dirac integral is defined as: ∞ 1 xn−1 dx fn(z) ≡ , Γ(n) z−1ex +1 0 µ/kT where x ≡ /kT and z ≡ e . We wish to derive a power series expansion for fn(z)that is useful in the limit of z → 0. We manipulate fn(z) as follows: ∞ z xn−1 dx fn(z)= Γ(n) ex + z 0 ∞ z xn−1 dx = Γ(n) ex(1 + ze−x) 0 ∞ ∞ z −x n−1 m −x m = e x dx (−1) (ze ) Γ(n) 0 m=0 ∞ ∞ z = (−1)mzm e−(m+1)xxn−1 dx . Γ(n) m=0 0 Using the well known integral: ∞ Γ(n) e−Axxn−1 dx = , An 0 and changing the summation variable to p = m + 1, we end up with: ∞ (−1)p−1zp fn(z)= n . (1) p=1 p which is the desired power series expansion. This result is also useful for deriving additional properties ofthe fn(z). For example, it is a simple matter use eq. (1) to verify: ∂ fn−1(z)=z fn(z) . ∂z Note that the classical limit is obtained for z 1. In this limit, which also corresponds to the high temperature limit, fn(z) z. One additional special case is noteworthy. If 1 z =1,weobtain ∞ (−1)p−1 fn(1) = n . p=0 p To evaluate this sum, we rewrite it as follows: 1 − 1 fn(1) = n n p odd p p even p 1 1 − 1 = n + n 2 n p odd p p even p p even p ∞ ∞ 1 − 1 = n 2 n p=1 p p=1 (2p) ∞ − 1 1 = 1 n−1 n . -
Sequential Discontinuities of Feynman Integrals and the Monodromy Group
Sequential Discontinuities of Feynman Integrals and the Monodromy Group Jacob L. Bourjaily1,2, Holmfridur Hannesdottir3, Andrew J. McLeod1, Matthew D. Schwartz3, and Cristian Vergu1 1Niels Bohr International Academy and Discovery Center, Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, DK-2100, Copenhagen Ø, Denmark 2Institute for Gravitation and the Cosmos, Department of Physics, Pennsylvania State University, University Park, PA 16892, USA 3Department of Physics, Harvard University, Cambridge, MA 02138, USA July 29, 2020 Abstract We generalize the relation between discontinuities of scattering amplitudes and cut diagrams to cover sequential discontinuities (discontinuities of discontinuities) in arbitrary momentum channels. The new relations are derived using time-ordered per- turbation theory, and hold at phase-space points where all cut momentum channels are simultaneously accessible. As part of this analysis, we explain how to compute se- quential discontinuities as monodromies and explore the use of the monodromy group in characterizing the analytic properties of Feynman integrals. We carry out a number of cross-checks of our new formulas in polylogarithmic examples, in some cases to all loop orders. arXiv:2007.13747v1 [hep-th] 27 Jul 2020 Contents 1 Introduction1 2 Cutting rules: a review4 2.1 Cutkosky, 't Hooft and Veltman . .5 2.2 Time-ordered perturbation theory . .7 3 Discontinuities 10 3.1 Covariant approach . 11 3.2 Discontinuities in TOPT . 14 4 Discontinuities as monodromies 17 4.1 Warm-up: the natural logarithm . 17 4.2 The monodromy group . 21 4.3 Monodromies of propagators . 31 5 Sequential discontinuities 33 5.1 Sequential discontinuities in the same channel . 34 5.2 Sequential discontinuities in different channels . -
Integral Formula for the Bessel Function of the First Kind
INTEGRAL FORMULA FOR THE BESSEL FUNCTION OF THE FIRST KIND ENRICO DE MICHELI ABSTRACT. In this paper, we prove a new integral representation for the Bessel function of the first kind Jµ (z), which holds for any µ,z C. ∈ 1. INTRODUCTION In this note, we prove the following integral representation of the Bessel function of the first kind Jµ (z), which holds for unrestricted complex values of the order µ: z µ π 1 izcosθ 1 iθ C C (1.1) Jµ (z)= e γ∗ µ, 2 ize dθ (µ ;z ), 2π 2 π ∈ ∈ Z− where γ∗ denotes the Tricomi version of the (lower) incomplete gamma function. Lower and upper incomplete gamma functions arise from the decomposition of the Euler integral for the gamma function: w t µ 1 (1.2a) γ(µ,w)= e− t − dt (Re µ > 0), 0 Z ∞ t µ 1 (1.2b) Γ(µ,w)= e− t − dt ( argw < π). w | | Z Analytical continuation with respect to both parameters can be based either on the integrals in (1.2) or on series expansions of γ(µ,w), e.g. [4, Eq. 9.2(4)]: ∞ ( 1)n wµ+n (1.3) γ(µ,w)= ∑ − , n=0 n! µ + n which shows that γ(µ,w) has simple poles at µ = 0, 1, 2,... and, in general, is a multi- valued (when µ is not a positive integer) function with− a− branch point at w = 0. Similarly, even Γ(µ,w) is in general multi-valued but it is an entire function of µ. Inconveniences re- lated to poles and multi-valuedness of γ can be circumvented by introducing what Tricomi arXiv:2012.02887v1 [math.CA] 4 Dec 2020 called the fundamental function of the incomplete gamma theory [11, §2, p. -
CHAPTER 4 Elementary Functions Dr. Pulak Sahoo
CHAPTER 4 Elementary Functions BY Dr. Pulak Sahoo Assistant Professor Department of Mathematics University Of Kalyani West Bengal, India E-mail : sahoopulak1@gmail:com 1 Module-3: Multivalued Functions-I 1 Introduction We recall that a function w = f(z) is called multivalued function if for all or some z of the domain, we find more than one value of w. Thus, a function f is said to be single valued if f satisfies f(z) = f[z(r; θ)] = f[z(r; θ + 2π)]: Otherwise, f is called as a multivalued function. We know that a multivalued function can be considered as a collection of single valued functions. For analytical properties of a multivalued function, we just consider those domains in which the functions are single valued. Branch By branch of a multivalued function f(z) defined on a domain D1 we mean a single valued function g(z) which is analytic in some sub-domain D ⊂ D1 at each point of which g(z) is one of the values of f(z). Branch Points and Branch Lines A point z = α is called a branch point of a multivalued function f(z) if the branches of f(z) are interchanged when z describes a closed path about α. We consider the function w = z1=2. Suppose that we allow z to make a complete circuit around the origin in the anticlockwise sense starting from the point P. Thus we p p have z = reiθ; w = reiθ=2; so that at P, θ = β and w = reiβ=2: After a complete p p circuit back to P, θ = β + 2π and w = rei(β+2π)=2 = − reiβ=2: Thus we have not achieved the same value of w with which we started.