Application of the Generalized Shift Operator to the Hankel Transform Natalie Baddour

Total Page:16

File Type:pdf, Size:1020Kb

Application of the Generalized Shift Operator to the Hankel Transform Natalie Baddour View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Crossref Baddour SpringerPlus 2014, 3:246 http://www.springerplus.com/content/3/1/246 a SpringerOpen Journal SHORT REPORT Open Access Application of the generalized shift operator to the Hankel transform Natalie Baddour Abstract It is well known that the Hankel transform possesses neither a shift-modulation nor a convolution-multiplication rule, both of which have found many uses when used with other integral transforms. In this paper, the generalized shift operator, as defined by Levitan, is applied to the Hankel transform. It is shown that under this generalized definition of shift, both convolution and shift theorems now apply to the Hankel transform. The operation of a generalized shift is compared to that of a simple shift via example. Introduction Background It is well known that the Hankel transform does not satisfy Several definitions of the Hankel transform appear in the a convolution or shift theorem in the simple way as that literature. In this paper, we use the definition of the nth the Fourier and Laplace transforms (Piessens 2000), re- order Hankel transform as defined by Piessens in (Piessens ducing its apparent utility. This follows because the 2000) to define the Hankel transform as Bessel functions do not possess a simple addition formula in the same way that the exponentials satisfy ei(x + y) = eixeiy. Z∞ The operation of convolution between two functions FðÞ¼ρ ℍnðÞ¼frðÞ frðÞJ nðÞρr rdr; ð1Þ consists of a shift in one of the functions, a multiplica- 0 tion with the other function, followed by an integration (or summation for discrete transforms) over all allow- where J (z)isthenth order Bessel function. Here, n may able shifts. Thus, the lack of a convolution theorem for n be an arbitrary real or complex number. However, an inte- the Hankel transform follows because of the lack of a gral transform needs to be invertible in order to be useful simple expression for the shift of a function in the and this restricts the allowable values of n.Ifn is real and Hankel transform domain. n > − 1/2, and under suitable conditions of integrability of Levitan introduced the idea of a generalized displace- the function, the transform is self-reciprocating and the in- ment operator (Levitan 2002). As useful as this concept version formula is given by might be, to the best of the author’s knowledge it does not appear to have seen much application in the physics or en- Z∞ gineering literature. In this paper, Levitan’s generalized dis- ðÞ¼ ðÞρ ðÞρ ρ ρ ð Þ placement operator is made concrete via application to fr F J n r d 2 the Hankel transform. We show that this leads to shift 0 and convolution rules for the Hankel transform. By way of several examples, the Hankel (generalized) shift is com- Thus, the Hankel transforms takes a function f(r)in pared to the standard simple shift. the spatial r domain and transforms it to a function F(ρ) in the frequency ρ domain. This relationship is denoted symbolically as f(r) ⇔ F(ρ). Correspondence: [email protected] Department of Mechanical Engineering, University of Ottawa, Ottawa, Ontario K1N 6N5, Canada © 2014 Baddour; licensee Springer. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited. Baddour SpringerPlus 2014, 3:246 Page 2 of 6 http://www.springerplus.com/content/3/1/246 Generalized shift for the Hankel Transform where the order of integration has been reversed (Levitan 2002) introduced the idea of a generalized shift and where: operator. Using Levitan’s definition, the generalized shift Z∞ operator Rr0 indicates a shift of r acting on the function 0 ðÞ¼; ; ðÞρ ðÞρ ðÞρ ρ ρ ð Þ f(r) is defined by the formula (Levitan 2002). Dn r r0 x J n r J n r0 J n x d 6 0 Z∞ r0 R frðÞ¼frðÞ¼jr0 FðÞρ J nðÞρr0 J nðÞρr ρdρ ð3Þ The interpretation of the generalized shift operator from Equation (5) allows the shift to be seen directly 0 as an operation on the original untransformed func- where F(ρ) is the Hankel transform of f(r) and we write tion. The definition as given in (3) allows for better r0 the generalized-shifted function as frrð j 0Þ ≡ R frðÞ,asa physical interpretation of the definition (in particu- reminder that the shifted function is now a function of lar in comparison with the familiar Fourier trans- r0 forms) and also permits the simple proofs to follow r and r0. The operator R acting on the function f(r) indicates a shift in f(r)byr0. The intuitive definition of for the shift and convolution rules. the Hankel shift (generalized shift), as defined in (3), is that of the inverse Hankel transform of F(ρ)Jn(ρr0), whereas the unshifted function would be the inverse Generalized shift rule Hankel transform of F(ρ) alone, without the multipli- In keeping with the standard shift-modulation rule of the Fourier transform, the definition of the Hankel cation by Jn(ρr0). In essence, Equation (3) says that multi- plication by Jn(ρr0) in the Hankel domain is equivalent to generalized shift allows for a similar rule to be derived a generalized shift in the spatial domain. for the Hankel transform. The Hankel transform of This definition follows the same expression used for the generalized-shifted function is given by application the Fourier transform, that is: of Equation (1) to the generalized-shifted function in (3) as Z∞ Z∞ ÀÁ 8 9 1 − ω ω 1 ω à ω Z∞ Z∞ FðÞω e i t0 ei tdω ¼ FðÞω ei t0 ei tdω < = 2π 2π −∞ −∞ ℍnðÞ¼frðÞjr0 FxðÞJ nðÞxr0 J nðÞxr xdx J nðÞρr rdr Z∞ : ; 1 ωðÞ− 0 0 ¼ FðÞω ei t t0 dω ¼ ftðÞ−t Z∞ Z∞ 2π 0 −∞ ¼ FxðÞJ nðÞxr0 J nðÞxr J nðÞρr rdr xdx ð4Þ 0 0 ð7Þ In (4), the star denotes the complex conjugate and fol- lows the definition of generalized shift as given by Levi- where the order of integration has been reversed. tan. As previously pointed out, the simple shift, f(t − t0), Using the orthogonality (closure) of the Bessel func- ω − ω ωðÞ− follows from the definition because ei te i t0 ¼ ei t t0 . tions (Watson 1995; Abramowitz & Stegun 1964) For the Hankel transform with Bessel functions, no sim- Z∞ ple equivalent expression exists, but the general struc- 1 J ðÞxr J ðÞρr rdr ¼ δðÞx−ρ ; ð8Þ ture of the shift operation for the Fourier transform n n x (left-hand side of Equation (4)) is the same. 0 It is noted that using the definition of Hankel trans- r0 it then follows that: form given in (1), the shifted function R frðÞ¼frrð j 0Þ can also be written as Z∞ δðÞx−ρ 8 9 ℍnðÞ¼frðÞjr0 FxðÞJ nðÞxr0 xdx Z∞<Z∞ = x r0 0 R frðÞ¼frðÞ¼jr0 fxðÞJ nðÞρx xdx J nðÞρr0 J nðÞρr ρdρ : ; ¼ FðÞρ J nðÞρr0 ð9Þ 0 0 Z∞ Z∞ ¼ fxðÞ J nðÞρr0 J nðÞρr J nðÞρx ρdρxdx In other words, a (generalized) shift in the spatial do- main is equivalent to multiplication by Jn(ρr0)inthe Z0∞ 0 Hankel domain or, if f(r) ⇔ F(ρ)thenf(r|r0) ⇔ F(ρ)Jn ¼ fxðÞDnðÞr; r0; x xdx (ρr0). This follows the same rule as for the Fourier 0 transform where the Fourier transform of f(r − r0)is ð Þ − ω 5 given by FðÞω e i r0 . Baddour SpringerPlus 2014, 3:246 Page 3 of 6 http://www.springerplus.com/content/3/1/246 Modulation rule Z∞Z∞ ℍ ðÞ¼ðÞà ðÞ ðÞðÞj ðÞρ Since the Hankel transform is self-reciprocal, a “modu- n g H f r gr0 frr0 r0dr0J n r rdr 0 0 8 9 lation” rule similar to that of the Fourier transform can Z∞Z∞ <Z∞ = ρ ¼ ðÞ ðÞ ðÞðÞ ðÞρ easily be derived. The Hankel transform of Jn(r 0)f(r)is gr0 : FxJ n xr0 J n xr xdx; r0dr0J n r rdr given by 0 0 0 ð13Þ Z∞ ÀÁÀÁ ÀÁ ℍ ρ ðÞ ¼ ðÞ ρ ðÞρ Interchanging the order of integration gives: it then n J n r 0 fr frJ n r 0 J n r rdr ð Þ 10 follows that 0 ÀÁ ρ ¼ ρjρ ¼ 0 ðÞρ F 0 R F Z∞Z∞Z∞ ℍnðÞ¼ðÞgÃH f ðÞr grðÞ0 J nðÞxr0 r0dr0 JnðÞxr JnðÞρr rdrFðÞ x xdx where the definition of the shifted transform follows 0 0 |fflfflfflfflfflfflfflfflfflfflfflfflfflfflfflffl{zfflfflfflfflfflfflfflfflfflfflfflfflfflfflfflffl}0 by replacing r, r0, ρ, f with ρ, ρ0, r, F in the definition ¼GxðÞ Z∞ Z∞ (3)sothat ¼ GxðÞFxðÞ J nðÞxr J nðÞρr rdr xdx ¼ GðÞρ FðÞρ 0 |fflfflfflfflfflfflfflfflfflfflfflfflfflffl{zfflfflfflfflfflfflfflfflfflfflfflfflfflffl}0 Z∞ 1 ÀÁ ÀÁ ¼ δðÞx−ρ ρ x R 0 FðÞ¼ρ F ρjρ ¼ frðÞJ n rρ J nðÞρr rdr ð11Þ 0 0 ð Þ 0 14 In the preceding Equation, (14), the definition of the ⇔ ρ ÀÁIn other words,À if f(r) F( ) then it follows that J n Hankel transform of g(r) has been used, in addition to ρ ρ ðÞ⇔ ρρ Þ¼ 0 ðÞρ r 0 fr F 0 R F . the orthogonality of the Bessel functions. Equation (14) clearly states that the Hankel transform of the Hankel convolution is the product of the Hankel transforms, Convolution rule again in parallel with the standard result of Fourier With the definition of the generalized shift, we define transforms.
Recommended publications
  • Zero-Order Hankel Transform Method for Partial Differential Equations
    Naol Tufa Negero / International Journal of Modern Sciences and Engineering Technology (IJMSET) ISSN 2349-3755; Available at https://www.ijmset.com Volume 3, Issue 10, 2016, pp.24-36 Zero-Order Hankel Transform Method for Partial Differential Equations Naol Tufa Negero Faculty of Natural and Computational Science, Department of Mathematics, Wollega University, Nekemte,Ethiopia. [email protected] Abstract This paper deals with the solution of Partial Differential Equations (PDEs) by the method of Hankel transform. Firstly, Hankel transforms is derived using two dimensional Fourier transform, next its properties are presented because their results are used widely in solving partial differential equations in the polar and axisymmetric cylindrical configurations, finally it applied to partial differential equation with precise formulation of initial and boundary value problems. In this article, we use the Hankel transforms method, namely Hankel transforms of zero order and of order one are introduced, such that PDE reduced to an ODE, which can be subsequently solved using ODE techniques which involves the Bessel functions. Moreover the main result of this paper is the zero-order Hankel transform method for Partial differential equations in unbounded problems with radial symmetry that is appropriate in the polar and cylindrical coordinates, which is analyzed in some detail. Keywords: Radial Fourier transforms, Two Dimensional Fourier Transform, Polar, Cylindrical and spherical Coordinates, Zero-Order Hankel Transform, Partial Differential Equations 1. INTRODUCTION: There are several integral transforms which are frequently used as a tool for solving numerous scientific problems. In many real applications, Fourier transforms as well as Mellin transforms and Hankel transforms are all very useful.
    [Show full text]
  • The Bessel Function, the Hankel Transform and an Application to Differential Equations
    Georgia Southern University Digital Commons@Georgia Southern Electronic Theses and Dissertations Graduate Studies, Jack N. Averitt College of Summer 2017 The Bessel Function, the Hankel Transform and an Application to Differential Equations Isaac C. Voegtle Follow this and additional works at: https://digitalcommons.georgiasouthern.edu/etd Part of the Partial Differential Equations Commons Recommended Citation I. Voegtle, "The Bessel Function, the Hankel Transform and an Application to Differential Equations". Georgia Southern University, 2017. This thesis (open access) is brought to you for free and open access by the Graduate Studies, Jack N. Averitt College of at Digital Commons@Georgia Southern. It has been accepted for inclusion in Electronic Theses and Dissertations by an authorized administrator of Digital Commons@Georgia Southern. For more information, please contact [email protected]. THE BESSEL FUNCTION, THE HANKEL TRANSFORM AND AN APPLICATION TO DIFFERENTIAL EQUATIONS by ISAAC VOEGTLE (Under the Direction of Yi Hu) ABSTRACT In this thesis we explore the properties of Bessel functions. Of interest is how they can be applied to partial differential equations using the Hankel transform. We use an example in two dimensions to demonstrate the properties at work as well as formulate thoughts on how to take the results further. INDEX WORDS: Bessel function, Hankel transform, Schrodinger¨ equation 2009 Mathematics Subject Classification: 35, 42 THE BESSEL FUNCTION, THE HANKEL TRANSFORM AND AN APPLICATION TO DIFFERENTIAL EQUATIONS by ISAAC VOEGTLE B.A., Anderson University, 2015 A Thesis Submitted to the Graduate Faculty of Georgia Southern University in Partial Fulfillment of the Requirements for the Degree MASTER OF SCIENCE STATESBORO, GEORGIA c 2017 ISAAC VOEGTLE All Rights Reserved 1 THE BESSEL FUNCTION, THE HANKEL TRANSFORM AND AN APPLICATION TO DIFFERENTIAL EQUATIONS by ISAAC VOEGTLE Major Professor: Yi Hu Committee: Shijun Zheng Yan Wu Electronic Version Approved: 2017 2 DEDICATION This thesis is dedicated to my wonderful wife.
    [Show full text]
  • International Journal of Pure and Applied Mathematics ————————————————————————– Volume 55 No
    International Journal of Pure and Applied Mathematics ————————————————————————– Volume 55 No. 2 2009, 247-256 THE HANKEL CONVOLUTION OF ARBITRARY ORDER C.K. Li Department of Mathematics and Computer Science Brandon University Brandon, Manitoba, R7A 6A9, CANADA e-mail: [email protected] Abstract: Let µ> 1/2. The classical Hankel transform is defined by − ∞ (hµφ)(t)= xJµ(xt)φ(x)dx t (0, ), (1) Z0 ∈ ∞ where Jµ(x) denotes the Bessel function of the first kind and order µ. The goal of this paper is to construct the Hankel transform of arbitrary order hµ,k based −1 on the two differential operators and show that hµ,k = h on H 1 for µ R. µ,k µ− 2 ∈ Furthermore, the Hankel convolution of arbitrary order is introduced with the following identity −µ (hµ,kh)(t)= t (hµ,kφ)(t)(hµ,kψ)(t) on the spaces (H 1 , H 1 ) and (Sµ, H 1 ) respectively. µ− 2 µ− 2 µ− 2 AMS Subject Classification: 46F12 Key Words: Hankel transform, Bessel function, Hankel convolution and automorphism 1. Introduction Let R+ = (0, ) and a weight function ν(x) > 0 in R+. We define a set of ∞ functions L(R+,ν(x)) as ∞ L(R+,ν(x)) = f(x) f(x) ν(x)dx < . { | Z0 | | ∞} Different types of the Hankel transforms as well as their convolutions, including modified ones, have been investigated over the decades (for example, see [7]- Received: August 1, 2009 c 2009 Academic Publications 248 C.K. Li [5] and [1]) both in the classical sense and in spaces of generalized functions.
    [Show full text]
  • A Fast Transform for Spherical Harmonics
    A Fast Transform for Spherical Harmonics Martin J. Mohlenkamp The Journal of Fourier Analysis and Applications 5(2/3):159{184, 1999. A±liation. Department of Mathematics, Yale University; and Department of Applied Mathemat- ics, University of Colorado, Campus Box 526, Boulder CO 80309-0526, [email protected]. Math Subject Classi¯cation. Primary 65T20; Secondary 42C10, 33C55. Keywords and Phrases. Spherical Harmonics, Fast Transforms, Associated Legendre Functions. Acknowledgements and Notes. I would like to thank my thesis advisor, R.R. Coifman, for his help and guidance. Abstract Spherical Harmonics arise on the sphere S2 in the same way that the (Fourier) exponential functions ik e k2Z arise on the circle. Spherical Harmonic series have many of the same wonderful properties asf Fourierg series, but have lacked one important thing: a numerically stable fast transform analogous to the Fast Fourier Transform. Without a fast transform, evaluating (or expanding in) Spherical Harmonic series on the computer is slow|for large computations prohibitively slow. This paper provides a fast transform. For a grid of (N 2) points on the sphere, a direct calculation has computational complexity (N 4), but a simpleO separation of variables and Fast Fourier Transform reduce it to (N 3) time. HereO we present algorithms with times (N 5=2 log N) and (N 2(log N)2). O The problem quickly reduces to the fastO application of matricesO of Associated Legendre Functions of certain orders. The essential insight is that although these matrices are dense and oscillatory, locally they can be represented e±ciently in trigonometric series. 1 Introduction Spherical Harmonics arise on the sphere S2 in the same way that the (Fourier) exponential functions ik e k2Z arise on the circle.
    [Show full text]
  • Hankel Transform, Langlands Functoriality and Functional Equation of Automorphic L-Functions
    Hankel transform, Langlands functoriality and functional equation of automorphic L-functions Ngô Bảo Châu dedicated with affection to the memory of Hiroshi Saito 1 Introduction The functoriality conjecture of Langlands, as stated in [33], offers a general organizational scheme for all automorphic representations. This conjecture can be roughly stated as follows: if H and G are reductive groups defined over a global field k, ξ : L H L G a homomorphism between their Langlands dual groups, then it is possible to attach to! each automorphic rep- H H resentation π = vπv of H a packet of automorphic representations π = vπv of G. In ⊗ ⊗ the formula π = vπv, local components πv are irreducible admissible representations of ⊗ G(kv), kv being the completion of k at a place v k . The automorphic functoriality is expected to be of local nature in the sense that it should2 j j be compatible with the local func- toriality principle that consists in a map from the set of packets of irreducible admissible representations of H(kv) to the set of packets of irreducible admissible representations of G(kv). Since unramified representations of H(kv) at an unramified nonarchimedean place v are parametrized by certain semi-simple conjugacy classes in L H, the local functoriality is required to be compatible with the transfer of conjugacy classes from L H to L G. A crucial part of the functoriality program, known as endoscopy, is now almost completely understood thanks to cumulative efforts of many mathematicians over the last 40 years, see [5]. Its main ingredients include in particular the construction of the general trace formula, mainly due to Arthur [4] and the proof of the transfer conjecture and the fundamental lemma, L see [54] and [39].
    [Show full text]
  • Linear Restriction Estimates for the Wave Equation with Inverse Square Potential
    LINEAR RESTRICTION ESTIMATES FOR THE WAVE EQUATION WITH INVERSE SQUARE POTENTIAL JUNYONG ZHANG AND JIQIANG ZHENG Abstract. In this paper, we study a modified linear restriction estimates associated with the wave equation with inverse square potential. In particular, we show the classical linear restriction estimates hold in their almost sharp range when the initial data is radial. Key Words: Linear restriction estimate, Spherical harmonics, Bessel func- tion, Inverse square potential AMS Classification: 42B37, 35Q40, 47J35. Contents 1. Introduction and Statement of Main Result 1 2. Preliminary 4 2.1. Spherical harmonic expansions and the Bessel functions 4 3. Proof of the Main Theorem 6 3.1. Hankel transform and the solution 7 3.2. Estimates of Hankel transforms 8 3.3. Conclude the Proof of Theorem 1.2 13 4. Appendix: Vector valued inequality 15 References 17 References 17 1. Introduction and Statement of Main Result In this paper, we study a modified restriction estimate associated with the wave equation perturbed by an inverse square potential. More precisely, we consider the following wave equation with a singular potential: ( @2u − ∆u + a u = 0 (t; x) 2 R × Rn; a 2 R; t jxj2 (1.1) u(t; x)jt=0 = 0;@tu(t; x)jt=0 = f(x): − a The scale-covariance elliptic operator Pa := ∆ + jxj2 appearing in (1.1) plays a key role in many problems of physics and geometry. The heat and Schr¨odingerflows for the elliptic operator Pa have been studied in the theory of combustion (see [8]), and in quantum mechanics (see [6]). The wave equation (1.1) arises in the study of the wave propagation on conic manifolds [5].
    [Show full text]
  • Asymptotic Expansions of Some Integral Transforms by Using Generalized Functions by Ahmed I, Zayed
    TRANSACTIONS OF THE AMERICAN MATHEMATICAL SOCIElY Volume 272, Number 2, August 1982 ASYMPTOTIC EXPANSIONS OF SOME INTEGRAL TRANSFORMS BY USING GENERALIZED FUNCTIONS BY AHMED I, ZAYED ABSTRACT. The technique devised by Wong to derive the asymptotic expansions of multiple Fourier transforms by using the theory of Schwartz distributions is ex- tended to a large class of integral transforms. The extension requires establishing a general procedure to extend these integral transforms to generalized functions. Wong's technique is then applied to some of these integral transforms to obtain their asymptotic expansions. This class of integral transforms encompasses, among others, the Laplace, the Airy, the K and the Hankel transforms. 1. Introduction. Recently, the theory of generalized functions has been introduced into the field of asymptotic expansions of integral transforms; see [18, 19,6]. One of the advantages of this approach is to be able to interpret and to assign values to some divergent integrals. This approach goes back to Lighthill [10] who was the first to use generalized functions to study the asymptotic expansions of Fourier transforms. Borrowing Lighthill's idea, several people were able to derive asymptotic expan- sions for other types of integral transforms such as Laplace [2], Stieltjes [11], Riemann-Liouville fractional integral transforms [12] and Mellin convolution of two algebraically dominated functions [17]. The use of generalized functions in the theory of asymptotic expansions has another advantage; that is, in some cases it can provide explicit expressions for the error terms in shorter and more direct ways than the classical methods [9,11]. However, one should not overemphasize the importance of the generalized functions approach since, for the most part, it is an alternative but not an exclusive technique.
    [Show full text]
  • Orthogonal Fast Spherical Bessel Transform on Uniform Grid
    Orthogonal fast spherical Bessel transform on uniform grid Vladislav V. Serov Department of Theoretical Physics, Saratov State University, 83 Astrakhanskaya, Saratov 410012, Russia Abstract We propose an algorithm for the orthogonal fast discrete spherical Bessel transform on an uniform grid. Our approach is based upon the spherical Bessel transform factorization into the two subsequent orthogonal transforms, namely the fast Fourier transform and the orthogonal transform founded on the derivatives of the discrete Legendre orthogonal polynomials. The method utility is illustrated by its implementation for the numerical solution of the three-dimensional time-dependent Schr¨odinger equation. Keywords: Spherical Bessel functions, Hankel transforms, time-dependent Schr¨odinger equation PACS: 02.30.Uu, 31.15.-p arXiv:1509.07115v3 [math.NA] 12 May 2016 1. Introduction The discrete spherical Bessel transform (DSBT) arises in a number of ap- plications, such as, e.g., the analysis of the cosmic microwave background [1], the numerical solution of the differential equations [2, 3, 4], and the numeri- ∗Corresponding author. E-mail address: vladislav [email protected] Preprint submitted to Computer Physics Communications May 13, 2016 cal evaluation of multi-center integrals [5, 6]. Many different SBT algorithms have been proposed so far [7, 8, 9, 10]. But none of them possess all of the advantages of their trigonometric progenitor, namely the fast Fourier trans- form (FFT). These advantages are the performance fastness, the uniform coordinate grid, and the orthogonality. An example of the problem requiring the simultaneous presence of all the advantages is the solving of the Schr¨odinger-type equation (SE) by means of the pseudospectral approach [9].
    [Show full text]
  • A Study on Henkel Transform and Its Relation to the Fourier Transform
    International Journal of Multidisciplinary Research and Development Volume: 2, Issue: 5, 555-558 May 2015 A study on Henkel transform and its relation to the www.allsubjectjournal.com e-ISSN: 2349-4182 Fourier transform p-ISSN: 2349-5979 Impact Factor: 3.762 Parmod Kumar Parmod Kumar Abstract Designation... Assistant In mathematics, the Hankel transform expresses any given function f(r) as the weighted sum of an Prof Rajiv Gandhi S.D. infinite number of Bessel functions of the first kind Jν (kr). The Bessel functions in the sum are all of the Commerce and Science same order ν, but differ in a scaling factor k along the r-axis. The necessary coefficient Fν of each Bessel College Narwana (Jind) function in the sum, as a function of the scaling factor k constitutes the transformed function. Hrayana-126115 Keywords: Hankel Transform, Fourier Transform. Introduction The Hankel transform is an integral transform and was first developed by the mathematician Hermann Hankel. It is also known as the Fourier–Bessel transform. Just as the Fourier transform for an infinite interval is related to the Fourier series over a finite interval, so the Hankel transform over an infinite interval is related to the Fourier–Bessel series over a finite interval. The Hankel transform of order ν of a function f(r) is given by: Where is the Bessel function of the first kind of order with The inverse Hankel transform of Fν(k) is defined as: Which can be readily verified using the orthogonality relationship described below. Inverting a Hankel transform of a function f(r) is valid at every point at which f(r) is continuous provided that the function is defined in (0, ∞), is piecewise continuous and of bounded variation in every finite subinterval in (0, ∞), and However, like the Fourier Transform, the domain can be extended by a density argument to include some functions whose above integral is not finite, for example .
    [Show full text]
  • Discrete Two-Dimensional Fourier Transform in Polar Coordinates Part I: Theory and Operational Rules
    Article Discrete Two-Dimensional Fourier Transform in Polar Coordinates Part I: Theory and Operational Rules Natalie Baddour 1,* 1 Department of Mechanical Engineering, University of Ottawa, 161 Louis Pasteur, , Ottawa, Canada * Correspondence: [email protected]; Tel.: (+1(613)5625800 X2324; Received: 9 July 2019; Accepted: 26 July 2019; Published: 2 August 2019 Abstract: The theory of the continuous two-dimensional (2D) Fourier transform in polar coordinates has been recently developed but no discrete counterpart exists to date. In this paper, we propose and evaluate the theory of the 2D discrete Fourier transform (DFT) in polar coordinates. This discrete theory is shown to arise from discretization schemes that have been previously employed with the 1D DFT and the discrete Hankel transform (DHT). The proposed transform possesses orthogonality properties, which leads to invertibility of the transform. In the first part of this two- part paper, the theory of the actual manipulated quantities is shown, including the standard set of shift, modulation, multiplication, and convolution rules. Parseval and modified Parseval relationships are shown, depending on which choice of kernel is used. Similar to its continuous counterpart, the 2D DFT in polar coordinates is shown to consist of a 1D DFT, DHT and 1D inverse DFT. Keywords: Fourier Theory, DFT in polar coordinates, polar coordinates, multidimensional DFT, discrete Hankel Transform, discrete Fourier Transform, Orthogonality. 1. Introduction The Fourier transform (FT) in continuous and discrete forms has seen much application in various disciplines [1]. It easily expands to multiple dimensions, with all the same rules of the one- dimensional (1D) case carrying into the multiple dimensions.
    [Show full text]
  • Integral Equations Associated with Hankel
    INTEGRALEQUATIONS ASSOCIATED WITH HANKEL CONVOLUTIONS( ) BY DEBORAH TEPPER HAIMO Chapter I. Introduction 1. Objectives. We denote by V[au ■■ -,an] the number of variations of sign of the sequence alt--,an of real numbers. Hence, for example, V[-1,0,1 ]= 1, V[1,0,1] = 0, V[0,0,0]=-1. If / is a real function defined for 0 < x < <*>,then V[f(x)] = l.u.b. V[/(x,), ■• - ,/(xn)], taken over all sets 0 < X! < x2 < • • ■ < co. Let H be a real-valued function of L'( — °°, «), <ba real-valued, continu- ous function of L °°(— °°, °°) and let (1) H *<b(x) = j~ H(x - t)<fi(t)dt, -co<x<oo. H is said to be a variation diminishing *-kernel if and only if, for every such <b, (2) V[H*<Kx)]£V[<p(x)]. Let (3) 1 C~ C* a ~2t)_„E(s) ' where (4) E(s) = ecs2+1*"f](l - i^) e"/8*, the aA's being real, with Z*"=i(l/oit) < co> and 6 and c real, with c ^ 0. In 1947, I. J. Schoenberg proved that the kernel G defined by (3) is vari- Presented to the Society, November 4, 1963 under the title Inversion for Hankel convolu- tions, and January 25, 1964 under the title Representation for Hankel convolutions; received by the editors November 5, 1963. ( ) This paper includes the major part of the author's doctoral dissertation at Harvard University. Thanks are due to Professor I. I. Hirschman, Jr., of Washington University who suggested the problem and who gave invaluable guidance.
    [Show full text]
  • Arxiv:2003.10771V3 [Math.CA] 5 Jul 2021 Fqatmmcais Tcnb Xrse I Esnegsinequa Heisenberg’S Via Expressed Be Can It Mechanics
    NEW SIGN UNCERTAINTY PRINCIPLES FELIPE GONC¸ALVES, DIOGO OLIVEIRA E SILVA, AND JOAO˜ P. G. RAMOS Abstract. We prove new sign uncertainty principles which vastly generalize the recent de- velopments of Bourgain, Clozel & Kahane and Cohn & Gon¸calves, and apply our results to a variety of spaces and operators. In particular, we establish new sign uncertainty principles for Fourier and Dini series, the Hilbert transform, the discrete Fourier and Hankel trans- forms, spherical harmonics, and Jacobi polynomials, among others. We present numerical evidence highlighting the relationship between the discrete and continuous sign uncertainty principles for the Fourier and Hankel transforms, which in turn are connected with the sphere packing problem via linear programming. Finally, we explore some connections between the sign uncertainty principle on the sphere and spherical designs. Contents 1. Introduction 1 2. Sign Uncertainty for Classical Orthogonal Systems 9 3. Sign Uncertainty in Discrete Spaces 21 4. Sign Uncertainty for Convolution Operators 28 5. Proofs of Main Results 30 6. Numerical Evidence 36 Acknowledgements 43 References 43 arXiv:2003.10771v3 [math.CA] 5 Jul 2021 1. Introduction The uncertainty principle, discovered by W. Heisenberg in 1927, is one of the cornerstones of quantum mechanics. It can be expressed via Heisenberg’s inequality: 4 ∞ ∞ f 2 R inf (x a)2 f(x) 2 dx (ξ b)2 f(ξ) 2 dξ > k kL ( ) , a,b R ˆ − | | ˆ − | | 16π2 ∈ −∞ −∞ b 2010 Mathematics Subject Classification. 33C45, 33C55, 42B05, 42B10, 44A15, 52C17, 65D32, 90C05. Key words and phrases. Dini series, Fourier series, Fourier transform, Gegenbauer polynomials, Ham- ming cube, Hankel transform, Hilbert transform, Jacobi polynomials, linear programming, sphere packing, spherical design, spherical harmonics, uncertainty principle.
    [Show full text]