ENSENANZA˜ REVISTA MEXICANA DE FISICA´ 48 (1) 67–75 FEBRERO 2002

Mathieu functions revisited: evaluation and generating functions

L. Chaos-Cador1 and E. Ley-Koo2 Instituto de F´ısica, Universidad Nacional Autonoma´ de Mexico´ Apartado postal 20-364, 01000 Mexico,´ D.F., Mexico e-mail: 1lorea@fisica.unam.mx, 2eleykoo@fisica.unam.mx Recibido el 24 de octubre de 2001; aceptado el 13 de noviembre de 2001

An updated didactical approach to Mathieu functions is presented as an alternative to the orthodox treatment. The matrix evaluation of the angular Mathieu functions is not only pertinent, but long over due, after seventy five years of matrix and with the availability of computing tools. Plane waves are identified as generating functions of the Mathieu functions, showing their explicit expansions. Some mathematical and physical applications are illustrated.

Keywords: Mathieu functions; matrix evaluation; generating functions

Se presenta un enfoque actualizado y didactico´ para las funciones de Mathieu como una alternativa a la presentacion´ ortodoxa. La evaluacion´ matricial de las funciones de Mathieu angulares es no solamente pertinente sino retrasada despues´ de setenta y cinco anos˜ de mecanica´ cuantica´ matricial y con la disponibilidad de herramientas computacionales. Se identifican las ondas planas como funciones generadoras de las funciones de Mathieu, mostrando sus desarrollos expl´ıcitos. Se ilustran algunas aplicaciones matematicas´ y f´ısicas.

Descriptores: Funciones de Mathieu; evaluacion´ matricial; funciones generadoras

PACS: 02.30.Jr; 02.30.Hq; 02.30.Gp

1. Introduction Recent physical applications of the Mathieu functions have been discussed by Ruby [17]. His opening sentence Mathieu functions were first investigated by that author in is “with few exceptions, notably Morse and Feshbach, and his “Memoire sur le movement vibratoire d’une membrane Mathews and Walker, most authors of textbooks on mathe- de forme elliptique” in 1868 [1], evaluating the lowest order matics for science and engineering choose to omit any dis- characteristic numbers and corresponding angular functions cussion of the Mathieu equation”. His review of the solution in ascending powers of the intensity parameter. A decade of the Mathieu equation follows the orthodox treatment [5], later, Heine defined the periodic Mathieu angular functions involving the evaluation of the characteristic numbers from of integer order as Fourier cosine and sine series, without the equation and then the evaluation of the evaluating the corresponding coefficients; obtained a tran- corresponding Fourier coefficients. scendental equation for the characteristic numbers expressed The authors of the present article have become involved in terms of an infinite continued fraction; and also demons- with Mathieu functions in connection with two recent works. trated that one set of periodic functions of integer order The first one was the review of the doctoral thesis “Formal could be expanded in a series of Bessel functions [2]. Flo- analysis of the propagation of invariant optical fields with quet published his mathematical work “Sur les equations elliptic symmetries” [18], in which the orthodox method of differentielles´ lineaires´ a´ coefficients periodiques” containing evaluating the Mathieu functions was also used. The second the theorem named after him [3], and Hill his memoir “On the one is about the bidimensional hydrogen molecular ion con- path of motion of the lunar perigee” introducing the determi- fined inside an , which can be solved in a matrix form nant named after him [4], both works having played relevant following the methods of quantum mechanics [19]. roles in subsequent investigations of the Mathieu functions The last two paragraphs contain the motivation to revisit and their extensions. the Mathieu functions. Section 2 is devoted to the separation For the purposes of the revisiting in the title of this pa- of the in elliptical coordinates leading per, reference is made to Chapter 20 on Mathieu functions to the canonical and modified forms of the Mathieu equa- by G. Blanch in Ref. 5. The reader is also referred to some tions. The orthodox method to construct the angular Mathieu of the classical books on mathematical methods [6–10] and functions is briefly described as a point of comparison. Its specific books on Mathieu functions [11–16] whose authors extension for the construction of the radial Mathieu func- made original contributions to establish mathematical pro- tions is also mentioned. In Sec. 3, their matrix evaluation is perties, to develop physical applications and to evaluate nu- formulated, recognizing that the output from the matrix dia- merical values of such functions. Humbert’s monograph con- gonalization provides simultaneously the values of both cha- tains the bibliography up to 1924 [11], and McLachlan’s book racteristic numbers and Fourier coefficients. In Sec. 4 another provides a historical introduction and updated bibliography gap in the study of the Mathieu functions is also filled in. It through 1947 [15]. is well known that the majority of the special functions can 68L.CHAOS-CADORANDE.LEY-KOO

be obtained from generating functions [5], but the Mathieu The substitution of Eq. (6) or (7) in the differential Eq. (5) functions have been so far an exception. We have identified leads to three-term recurrence relations for the Fourier coeffi- 2r+p 2r+p that plane waves are also their generating functions showing cients A2s+p(q) or B2s+p (q). Their explicit forms appear as the corresponding series expansions in products of radial and Eqs. 20.2.5–20.2.11 in Ref. 5. The ratios of consecutive coef- angular Mathieu functions. In the final section a discussion is ficients of the same parity then satisfy two types of continued made of illustrative mathematical and physical applications fractions, appearing as Eqs. 20.2.12–20.2.20 in Ref. 5. The of some of our results. convergence of the of Eqs. (6) and (7) requires that the coefficients Am and Bm vanish as m → ∞, which 2. Helmholtz equation in elliptical coordinates implies the vanishing of the respective infinite continued frac- tions. The corresponding roots are the characteristic numbers Elliptical coordinates (0 ≤ u < ∞, 0 ≤ v ≤ 2π), are de- a2r, a2r+1, b2r, b2r+1 from Eqs. 20.2.21–20.2.24 in Ref. 5. fined through the transformation equations to Cartesian coor- Ince developed the numerical methods to evaluate the char- dinates: acteristic numbers accurately, and from them the ratios of the Fourier coefficients, and finally the coefficients themselves x = c cosh u cos v, taking into account the normalization of Eqs. (6) and (7) [20]. y = c sinh u sin v, (1) Ince’s method became the orthodox method to evaluate Math- ieu functions. where c is the common semifocal distance of confocal el- The orthonormalization for the Mathieu functions in lipses with eccentricities 1/ cosh u, and confocal hyperbolas Eqs. (6) and (7) is the same as that of the cosine and sine with eccentricities 1/ cos v. functions, namely, Helmholtz equation in these coordinates takes the form Z 2π ½ · ¸ ¾ 2 ∂2 ∂2 cem(v, q)cen(v, q) dv = πδmn, (8) 2 0 2 2 + 2 +k ψ(u, v)=0, (2) c (cosh 2u−cos 2v) ∂u ∂v Z 2π and is separable. In fact, it admits factorizable solutions sem(v, q)sen(v, q) dv = πδmn. (9) 0 ψ(u, v) = U(u)V (v), (3) This normalization convention leads to the conditions on the respective Fourier coefficients: where the respective factors satisfy the ordinary differential equations 2r 2 2r 2 2r 2 2(A0 ) + (A2 ) + ... + (A2s) + ... = 1, (10) · ¸ d2 2r+1 2 2r+1 2 2r+1 2 + 2q cosh 2u U(u) = aU(u), (4) (A1 ) + (A3 ) + ... + (A2s+1) + ... = 1, (11) du2 2r 2 2r 2 2r 2 · ¸ (B2 ) + (B4 ) + ... + (B2s ) + ... = 1, (12) d2 − 2q cos 2v V (v) = −aV (v). (5) 2r+1 2 2r+1 2 2r+1 2 dv2 (B1 ) + (B3 ) + ... + (B2s+1 ) + ... = 1. (13)

Here q = k2c2/4 is the intensity parameter and a is the se- Notice the factor of 2 in the first term of Eq. (10), associ- paration constant. Equation (5) is the canonical form of Ma- ated with the normalization to 2π of cos mv for m = 0. thieu’s equation, and Eq. (4) is the modified form. They are In the limit in which q → 0, Eqs. (6) and (7) guarantee connected through the substitutions v → iu and V → U, so that the Mathieu functions tend to the respective cosine and that the elliptical or radial Mathieu functions U can be ob- sine functions of the same order. Mathieu made the analy- tained by analytical continuation of the hyperbolic or angular sis of the vibrations of an elliptic membrane for small values Mathieu functions V . of q obtaining power series in this parameter for the charac- The periodic angular Mathieu functions can be expressed teristic values and the periodic functions, corresponding to as Fourier series of four different types: Eqs. 20.2.25–20.2.26 and 20.2.27–20.2.28 in Ref. 5, respec- tively. In the context of quantum mechanics these expansions X∞ £ ¤ ce (v, q) = A2r+p(q) cos (2s + p)v , (6) can be understood as the result of applying perturbation the- 2r+p 2s+p ory in different orders of approximation, taking the circular s=0 membrane as the nonperturbed starting problem. X∞ £ ¤ se (v, q) = B2r+p(q) sin (2s + p)v ; (7) The radial Mathieu functions are obtained by analytical 2r+p 2s+p continuation from those of Eqs. (6) and (7): s=0 when p = 0 their period is π, and when p = 1 their period Ce2r+p(z, q) = ce2r+p(iz, q) is 2π. The characteristic numbers for the even solutions of X∞ £ ¤ Eq. (6) are represented as a2r+p(q), and for the odd solutions 2r+p = A2s+p(q) cosh (2s + p)z , (14) of Eq. (7) as b2r+p(q). s=0

Rev. Mex. F´ıs. 48 (1) (2002) 67–75 MATHIEUFUNCTIONSREVISITED:MATRIXEVALUATIONANDGENERATINGFUNCTIONS69 and X∞ 2r+p £ ¤ Se2r+p(z, q) = −ise2r+p(iz, q) = B2s+p (q) sinh (2s + p)z , (15) s=0 involving the same expansion coefficients. √ √ The radial Mathieu Eq. (4) can be rewritten in terms of the alternative arguments 2 q cosh u or 2 q sinh u. Then it can be solved as series of ordinary Bessel functions. The expansion coefficients turn out to satisfy three-term recurrence relations closely connected with the corresponding ones appearing in the angular Mathieu functions. Here we simply borrow Eqs. 20.6.3–20.6.6 in Ref. 5 to illustrate the point and as a reference for the analysis in Sec. 4:

ce ( π , q) X∞ √ ce (0, q) X∞ √ Ce (z, q) = 2r 2 (−)kA2r J (2 q cosh z) = 2r A2r J (2 q sinh z), (16) 2r A2r 2k 2k A2r 2k 2k 0 k=0 0 k=0 0 π X∞ ce2r+1( 2 , q) k+1 2r+1 √ Ce2r+1(z, q) = √ (−) A J (2 q cosh z) qA2r+1 2k+1 2k+1 1 k=0 X∞ ce2r+1(0, q) √ = √ coth z (2k + 1)A2r+1 J (2 q sinh z), (17) qA2r+1 2k+1 2k+1 1 k=0 se0 ( π , q) X∞ √ se0 (0, q) X∞ √ Se (z, q) = 2r 2 tanh z (−)k2kB2rJ (2 q cosh z) = 2r coth z 2kB2rJ (2 q sinh z), (18) 2r qB2r 2k 2k qB2r 2k 2k 2 k=1 2 k=0 π X∞ se2r+1( 2 , q) k 2r+1 √ Se2r+1(z, q) = √ tanh z (−) (2k + 1)B J (2 q cosh z) qB2r+1 2k+1 2k+1 1 k=0 0 X∞ se2r+1(0, q) √ = √ B2r+1J (2 q sinh z). (19) qB2r+1 2k+1 2k+1 1 k=0

3. Matrix evaluation of angular Mathieu functions √ In this section the matrix solution of Eq. (5) is formulated. The Fourier series of Eqs. (6) and (7): divided by π, in order to have basis functions normalized to one, are the starting point. Then it is straightforward to construct the matrices of Eq. (5), with a change of sign in its LHS and RHS, in the respective bases. The results are:  √  √  √  √0 2q 0 0 ... 2A0 2A0        2q 4 q 0 ...   A2   A2         0 q 16 q . . .   A4   A4   . . .   .   .   . . . ..   .   .   . . . .   .   .   . . . .   .   .   ......   .  = a2r  .  , (20)  . . . . .   .   .         ......   .   .   ......   .   .   2       q (2s) q   A2s   A2s  ......       1 + q q 0 0 ... A1 A1        q 9 q 0 ...   A3   A3         0 q 25 q . . .   A5   A5   . . . .   .   .   . . . ..   .   .   . . .   .   .   . . . . .   .   .   . . . . .   .  = a2r+1  .  , (21)  . . . . .   .   .         ......   .   .   ......   .   .   2       q (2s + 1) q  A2s+1 A2s+1 ......

Rev. Mex. F´ıs. 48 (1) (2002) 67–75 70 ENGLISHL. CHAOS-CADOR AND E. LEY-KOO       4 q 0 0 ... B2 B2       q 16 q 0 ...   B4   B4        0 q 36 q . . .   B6   B6  . . . .   .   .  . . . ..   .   .     .   .  . . . . .   .  = b2r  .  , (22) ......   .   .  . . . .      ......   .   .  ......   .   .   2       q (2s) q  B2s B2s ......       1 − q q 0 0 ... B1 B1  q 9 q 0 ...   B   B     3   3   0 q 25 q . . .   B   B     5   5   . . . ..   .   .   . . . .   .   .   . . . .   .   .   ......   .  = b2r+1  .  (23)  . . . . .   .   .   ......   .   .   ......   .   .   2       q (2s + 1) q  B2s+1 B2s+1 ......

For the√ sake of simplicity coefficients is not written. No- tice the 2 factor in the first element of the eigenvector√ of Eq. (20) needed to compensate for the extra factor 1/ 2π tion is no longer valid. In fact, our didactic and practical in the normalization of the respective basis function. Also proposition is to use the matrix form of Eqs. (20)–(23) to notice the tridiagonal and symmetric character of the matri- solve Eq. (5). Conceptually, the eigenvalue nature of the ces representing the Mathieu equation operator. The common problem is emphasized in this approach. Practically, the asso- and different elements in Eqs. (20) and (22), and in Eqs. (6) ciated secular determinant is simpler and more familiar than and (7), are also worth noticing. the Hill determinant. Computationally, the availability of re- Of course, these equations are equivalent to the three- liable, fast and accurate matrix diagonalization programs al- term recurrence relations behind the orthodox method lows the evaluation of N characteristic numbers and its res- of evaluating the Mathieu functions. A quotation from pective N eigenvectors, in a single run for an N × N matrix. Blanch [5] is pertinent in connection with the numerical As an illustration of the matrix evaluation of the Mathieu implementation of the orthodox method: function by using 10 × 10 matrices for q = 0 − 5 and 30 × 30 “. . . continued fractions can be converted to determi- matrices for q = 5–25, the respective characteristic numbers nant form. and eigenvectors are obtained, matching and improving the . . . a determinant with an infinite number of rows– a accuracy of their corresponding values tabulated in Ref. 5. special case of Hill’s determinant. Although the deter- We close this section by pointing out that Floquet solu- minant has actually been used in computations where tions X∞ high speed computers were available the direct use of i(ν+2k)z the continued fraction seems much less laborious.” Fv(z) = c2ke (24) After three decades and a half, the availability of comput- k=−∞ ing tools is so widespread that the last sentence of the quota- of Eq. (4) can also be formulated and evaluated in matrix form:       ......    .   .   2  c  c  q (−2n + ν) q   −2n  −2n  .   .   .   ..   .   .         0 q (−2 + ν)2 q 0   c   c     −2   −2   0 q ν2 q 0   c  = a  c  (25)    0   0   0 q (2 + ν)2 q 0   c   c     2   2   .   .   .   ..   .   .   2       q (2n + ν) q   c2n   c2n  ...... where ν is the characteristic exponent [5].

Rev. Mex. F´ıs. 48 (1) (2002) 67–75 MATHIEUFUNCTIONSREVISITED:MATRIXEVALUATIONANDGENERATINGFUNCTIONS71

4. Plane waves as generating functions of These equations also mean that the plane waves are genera- Mathieu functions ting functions for the circular waves. The perusal of the literature on Mathieu functions shows The plane waves that there are not explicitly recognized generating functions i~k·~ρ i(k x+ik y) ψ(x, y) = e = e x y (26) for them [1–16]. Since Mathieu functions are the solutions and circular waves of the Helmholtz equation in elliptical coordinates, the exis- tence of such generating functions could and should be ex- imϕ ψ(ρ, ϕ) = Jm(kρ)e (27) pected. Indeed, in this section plane waves are identified as are regular solutions of the Helmholtz equation satisfying generating functions of elliptical waves, showing their ex- orthogonality and completeness properties in their com- plicit expansions as series of products of regular radial and mon domain (∞ < x < ∞, −∞ < y < ∞) and angular Mathieu functions. (0 ≤ ρ < ∞, 0 ≤ ϕ ≤ 2π). Such properties allow the ex- The starting point is Eq. (28) using the elliptical coordi- pansions of plane waves as superpositions of circular waves: nate representation of the Cartesian coordinate, Eq. (1), with the result X∞ ikx ikρ cos ϕ m imϕ e = e = i Jm(kρ)e , (28) X∞ m=−∞ ikx ikc cosh u cos v m imv e = e = i Jm(kc cosh u)e . (30) X∞ m=−∞ iky ikρ sin ϕ m imϕ e = e = (−1) Jm(kρ)e . (29) m=−∞ Next, the even and odd terms in the summation are grouped together to obtain

∞ √ X i2 q cosh u cos v √ s √ e = J0(2 q cosh u) + 2 (−1) J2s(2 q cosh u) cos(2sv) s=1 X∞ s √ +2i (−1) J2s+1(2 q cosh u) cos[(2s + 1)v], (31) s=1 √ where the replacement kc = 2 q has been made. Since the Fourier and angular Mathieu function bases are Z 2π both complete and orthogonal in the same domain, the first ¯2s+p 1 A2r+p(q) = ce2r+p(q, v) cos[(2s + p)v] dv ones can be written as linear superpositions of the second π 0 ones: = A2r+p(q), (34) X∞ 2s+p 2s+p cos[(2s + p)v] = A¯ (q)ce (v, q), (32) Z 2π 2r+p 2r+p ¯2s+p 1 r=0 B2r+p(q) = se2r+p(q, v) sin[(2s + p)v] dv π 0 X∞ ¯2s+p 2r+p sin[(2s + p)v] = B2r+p(q)se2r+p(v, q). (33) = B2s+p (q); (35) r=0 ¯0 2r These are the inverse transformations of Eqs. (6) and (7). except for A2r = 2A0 , associated with the different norma- The corresponding transformation coefficients are connected lization of cos(2sv) for s = 0. by a simple transposition Then the successive substitutions of Eqs. (34) and (32), and the result in Eq. (31) leads to the result

∞ ∞ √ X X i2 q cosh u cos v s √ 2r e = 2 (−1) J2s(2 q cosh u) A2s(q)ce2r(v, q) s=0 r=0 X∞ X∞ s √ 2r+1 +2i (−) J2s(2 q cosh u) A2s+1(q)ce2r+1(v, q). (36) s=0 r=0

The exchange of the summations over the indices r and s gives

∞ ∞ √ X X i2 q cosh u cos v s 2r √ e = 2 ce2r(v, q) (−) A2s(q)J2s(2 q cosh u) r=0 s=0 X∞ X∞ s 2r+1 2r+1 √ +2i ce2r+1(v, q) (−1) A2s+1(q)J2s+1 (2 q cosh u), (37) r=0 s=0

Rev. Mex. F´ıs. 48 (1) (2002) 67–75 72L.CHAOS-CADORANDE.LEY-KOO

The final step is to recognize that the summations over the index s are the even and odd order regular radial Mathieu functions, except for the normalization factor, according to Eq . (16) and (17), respectively, with the final result

∞ ∞ √ √ X A2r X qA2r+1 ei2 q cosh u cos v = 2 0 Ce (u, q)ce (v, q) − 2i 1 Ce (u, q)ce (v, q). (38) ce ( π , q) 2r 2r ce0 ( π , q) 2r+1 2r+1 r=0 2r 2 r=0 2r+1 2

Similarly, if we start with the plane wave of Eqs. (29) and (2) for y, we obtain

∞ ∞ √ X X i2 q sinh u sin v m √ imv √ √ e = (−1) Jm(2 q sinh u)e = Jo(2 q sinh u) + 2 J2s(2 q sinh u) cos(2sv) m=−∞ s=1 X∞ √ +2i J2s+1(2 q sinh u) sin[(2s + 1)v]. (39) s=0

By writing the Fourier basis functions in terms of the Mathieu functions, Eqs. (32) and (33), and using the relations between the transformation coefficients of Eqs. (34) and (35), Eq. (39) becomes

∞ ∞ ∞ ∞ √ X X X X i2 q sinh u sin v 2r √ 2r+1 √ e = 2 ce2r(q, v) A2s(q)J2s(2 q sinh u) + 2i se2r+1(q, v) B2s+1 (q)J2s+1(2 q sinh u). (40) r=0 s=0 r=0 s=0

Now the sums over s are identified with the corresponding regular radial Mathieu functions of Eqs. (16) and (19), respec- tively, with the final expansion

∞ ∞ √ √ X A2r X qB2r+1 ei2 q sinh u sin v = 2 0 Ce (u, q)ce (v, q) + 2i 1 Se (u, q)se (v, q). (41) ce (0, q) 2r 2r se0 (0, q) 2r+1 2r+1 r=0 2r r=0 2r+1

Equations (38) and (41) represent plane waves as generating functions of the Mathieu functions. Next we analyze some of their specific values and of their derivatives with respect to the hyperbolic coordinate for the special values of v = 0 and π/2, in order to establish some of the other relationships and representations of the radial Mathieu functions of Eqs. (16)–(19). Equation (38) for v = π/2 and Eq. (41) for v = 0, give the same result

X∞ 2r 1 = 2 A0 (q)Ce2r(u, q), (42) r=0 analogous to 9.1.46 for Bessel functions in Ref. 5. The first derivative of Eq. (31) with respect to v is

∞ √ X √ i2 q cosh u cos v s √ −i2 q cosh u sin ve = −2 (−) J2s(2 q cosh u)2s sin(2sv) s=1 X∞ s √ −2i (−) J2s+1(2 q cosh u)(2s + 1) sin[(2s + 1)v]. (43) s=0

Then the use of Eqs. (33) and (35) allows rewriting it as

∞ ∞ √ X X √ i2 q cosh u cos v s 2r √ −i2 q cosh u sin ve = −2 se2r(v, q) (−1) 2sB2s J2s(2 q cosh u) r=1 s=1 X∞ X∞ s 2r+1 √ −2i se2r+1(v, q) (−) (2s + 1)B2s+1 J2s+1(2 q cosh u). (44) r=0 s=0

Now the value of the exponential for v = π/2 can be rewritten as ¡ ¢ X∞ se π , q X∞ √ 1 = √2r+1 2 (−1)s(2s + 1)B2r+1J (2 q cosh u). (45) q cosh u 2s+1 2s+1 r=0 s=0

Rev. Mex. F´ıs. 48 (1) (2002) 67–75 MATHIEUFUNCTIONSREVISITED:MATRIXEVALUATIONANDGENERATINGFUNCTIONS73

The first derivative of Eq. (41) with respect to v is

∞ √ √ X A2r i2 q sinh u cos vei2 q sinh u sin v = 2 0 Ce (u, q)ce0 (v, q) ce (0, q) 2r 2r r=0 2r √ X∞ qB2r+1 +2i 1 Se (u, q)se0 (v, q). (46) se0 (0, q) 2r+1 2r+1 r=0 2r+1 Now the value of the exponential for v = 0 becomes

X∞ B2r+1(q) 1 = 1 Se (u, q). (47) sinh u 2r+1 r=0 The comparison of Eq. (45) and (47) leads to the representation of the radial Mathieu functions, ¡ ¢ π X∞ se2r+1 2 , q s 2r+1 √ Se2r+1(u, q) = √ 2r+1 tanh u (−) (2s + 1)B2s+1 J2s+1(2 q cosh u), (48) qB1 s=0 as an alternative to the one used in going from Eq. (40) and (41), and which is the other form of Eq. (19). Similarly, the first derivative of Eq. (39) with respect to v is ∞ √ X √ i2 q sinh u sin v √ i2 q sinh u cos ve = −2 J2s(2 q sinh u)2s sin(2sv) s=1 X∞ √ +2i J2s+1(2 q sinh u)(2s + 1) cos[(2s + 1)v], (49) s=0 and can be rewritten in terms of angular Mathieu functions as ∞ ∞ √ X X √ i2 q sinh u sin v 2r √ i2 q sinh u cos ve = −2 se2r(v, q) (2s)B2s J2s(2 q sinh u) r=1 s=1 X∞ X∞ 2r+1 √ +2i ce2r+1(v, q) (2s + 1)B2s+1 J2s+1(2 q sinh u). (50) r=0 s=0 Now the value of the exponential function for v = 0 is represented as

X∞ ce (0, q) X∞ √ 1 = √2r+1 (2s + 1)B2r+1J (2 q sinh u). (51) q sinh u 2s+1 2s+1 r=0 s=0 The first derivative of Eq. (38) with respect to v is ∞ √ √ X A2r −i 2 cosh u sin vei2 q cosh u cos v = 2 0 Ce (u, q)ce0 (v, q) ce ( π , q) 2r 2r r=0 2r 2 √ X∞ qA2r+1 −2i ¡1 ¢Ce (u, q)ce0 (v, q). (52) ce0 π , q 2r+1 2r+1 r=0 2r+1 2

Now the value of the exponential function for v = π/2 takes the form

X∞ A2r+1(q) 1 = 1 Ce (u, q). (53) cosh u 2r+1 r=0 Then the comparison of Eqs. (51) and (53) leads to the representation of the radial Mathieu function, X∞ ce2r+1(0, q) 2r+1 √ Ce2r+1(u, q) = √ 2r+1 coth u (2s + 1)B2s+1 J2s+1(2 q sinh u), (54) qA1 s=0 as an alternative of the one going from Eqs. (37) and (38) corresponding to the other form of Eq. (17).

Rev. Mex. F´ıs. 48 (1) (2002) 67–75 74L.CHAOS-CADORANDE.LEY-KOO

On the other hand, the reader may notice that in Eqs. (38) and (41) the Mathieu functions of even order and sine type do not appear. Next, we establish their representations by taking their second derivatives with respect to v via Eq. (44) and (50), respectively,

∞ ∞ √ X X √ √ 2 i2 q cosh u cos v 0 s 2r √ [−i2 q cosh u cos v + (−i2 q cosh u sin v) ]e = −2 se2r(v, q) (−) (2s)B2s J2s(2 q cosh u) r=1 s=1 X∞ X∞ 0 s 2r+1 √ −2i se2r+1(v, q) (−1) (2s + 1)B2s+1 J2s+1(2 q cosh u), (55) r=0 s=0 ∞ ∞ √ X X √ √ 2 i2 q sinh u sin v 0 2r √ [−i2 q sinh u sin v + (i2 q sinh u cos v) ]e = −2 se2r(v, q) (2s)B2s J2s(2 q sinh u) r=1 s=1 X∞ X∞ 0 2r+1 √ +2i se2r+1(v, q) (2s + 1)B2s+1 J2s+1(2 q sinh u). (56) r=0 s=0

Now the exponential of Eq. (55) for v = π/2 takes the form orthogonality properties of the angular Mathieu functions of X∞ se0 ( π , q) X∞ √ Eqs. (8) and (9), allow the evaluation of the expansion co- 1 = 2r 2 (−1)s2sB2rJ (2 q cosh u). (57) 2q cosh2 u 2s 2s efficients of the respective generating functions of Eq. (38) r=1 s=1 and (41) with the results Correspondingly the exponential of Eq. (56) for v = 0 π ce2r( 2 , q) gives Ce2r(u, q) = 2r 2πA0 Z X∞ 0 X∞ 2π √ se2r(0, q) 2r √ × cos[2 q cosh u cos v]ce (v, q) dv, (60) 1 = 2 2sB2s J2s(2 q sinh u). (58) 2r 2q sinh u 0 r=1 s=1 ¡ ¢ 0 π −ce2r 2 , q The comparison of Eqs. (57) and (58) leads to the Ce2r+1(u, q) = √ 2π qA2r+1 equivalent representations for the radial Mathieu functions 1 Z 2π Se2r(u, q) of Eq. (18) with the conventional normalization. √ × sin[2 q cosh u cos v]ce2r+1(v, q) dv, (61) Also both Eq. (57) and (58) can be rewritten as 0

X∞ 2r ce2r(0, q) B2 (q) Ce2r(u, q) = 2r 1 = Se2r(u, q). (59) 2πA0 sinh 2u Z r=1 2π √ × cos[2 q sinh u sin v]ce2r(v, q) dv, (62) To sum up this section, Eqs. (38) and (41) are gener- 0 ating functions of the Mathieu functions. From the analy- 0 se2r+1(0, q) sis of some of their values and of their derivatives, differ- Se (u, q) = 2r+1 2πB2r+1 ent properties of the radial Mathieu functions have been ex- 1 Z 2π plicitly established. Specifically, their alternative represen- √ × sin[2 q sinh u sin v]se2r+1(v, q) dv. (63) tations of Eqs. (16)–(19) and alternative representations of 0 one, Eqs. (42), (47), (53) and (59). The reader can verify that The integrals involved are equivalent to four times the in- Eq. (47) is analogous to 9.1.47 and Eq. (53) to 9.1.48 for tegrals from 0 to π/2. Similar integral representations can be Bessel functions Ref. 5. Equation (59) is the corresponding obtained starting from the derivatives of the generating func- result for sinh 2u. The four equations can also be understood tions. Additional results follow from analytical continuation as particular cases of Eqs. (32) and (33) with (s = 0, p = 0) of the variable u. The reader can check that they correspond and (s = 0, p = 1), and (s = 0, p = 1) and (s = 0, p = 0), to Eqs. 20.7.20–20.7.24 in Ref. 5. and v → iu, respectively. Concerning the physical applications of the Mathieu functions, the reader is referred to [11, 15, 17–19]. The faster 5. Some applications and discussion and reliable matrix method to evaluate the characteristic num- bers and Fourier coefficients for the Mathieu functions may The analysis of the last part of the previous section illustrates be easily implemented by those interested in developing other some of the immediate applications of the generating func- physical applications. The explicit identification of plane tions of Eqs. (38) and (41). Other applications lead to integral waves as generating functions of elliptical waves has been representations of the radial Mathieu functions. In fact, the of special interest in our group in order to investigate optical

Rev. Mex. F´ıs. 48 (1) (2002) 67–75 MATHIEUFUNCTIONSREVISITED:MATRIXEVALUATIONANDGENERATINGFUNCTIONS75 diffraction and electron transport in bidimensional structures sults of Sec. 3 and 4 in their study of the Mathieu functions. with elliptical-hyperbolic boundaries. The revisiting in this paper does not pretend to be exhaustive, From a didactical point of view, we recommend to teach- and we anticipate additional insights and extensions. ers and students to incorporate some of the methods and re-

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Rev. Mex. F´ıs. 48 (1) (2002) 67–75