In mathematics, Mathieu functions, sometimes called angular Mathieu functions, are solutions of Mathieu's differential equation
d2y | |
dx2 |
+(a-2q\cos(2x))y=0,
They were first introduced by Émile Léonard Mathieu, who encountered them while studying vibrating elliptical drumheads.[1] [2] [3] They have applications in many fields of the physical sciences, such as optics, quantum mechanics, and general relativity. They tend to occur in problems involving periodic motion, or in the analysis of partial differential equation (PDE) boundary value problems possessing elliptic symmetry.[4]
In some usages, Mathieu function refers to solutions of the Mathieu differential equation for arbitrary values of
a
q
\pi
2\pi
a
q
q
a
an(q)
bn(q)
n=1,2,3,\ldots
cen(x,q)
sen(x,q)
As a result of assuming that
q
cen(x,q)
sen(x,q)
x
Function | Parity | Period | |
---|---|---|---|
cen, neven | even | \pi | |
cen, nodd | even | 2\pi | |
sen, neven | odd | \pi | |
sen, nodd | odd | 2\pi |
The indexing with the integer
n
cen(x,q)
sen(x,q)
\cosnx
\sinnx
q → 0
n
cen
sen
a
q
Closely related are the modified Mathieu functions, also known as radial Mathieu functions, which are solutions of Mathieu's modified differential equation
d2y | |
dx2 |
-(a-2q\cosh2x)y=0,
x\to\pm{\rmi}x
Cen(x,q)
Sen(x,q)
\begin{align} Cen(x,q)&=cen({\rmi}x,q).\\ Sen(x,q)&=-{\rmi}sen({\rmi}x,q). \end{align}
x
A common normalization,[8] which will be adopted throughout this article, is to demand
2\pi | |
\int | |
0 |
cen(x,q)2dx=
2\pi | |
\int | |
0 |
sen(x,q)2dx=\pi
as well as require
cen(x,q) → +\cosnx
sen(x,q) → +\sinnx
q → 0
The Mathieu equation has two parameters. For almost all choices of parameter, by Floquet theory (see next section), any solution either converges to zero or diverges to infinity.
Parametrize Mathieu equation as
\ddotx+k(1-m\cos(t))x=0
k\in\R,m\geq0
See main article: Floquet theory. Many properties of the Mathieu differential equation can be deduced from the general theory of ordinary differential equations with periodic coefficients, called Floquet theory. The central result is Floquet's theorem:
It is natural to associate the characteristic numbers
a(q)
a
\sigma=\pm1
y(x+\pi)=\sigmay(x)
a
q
a
\pi
2\pi
cen(x,q)
sen(x,q)
fen(x,q)
gen(x,q)
An equivalent statement of Floquet's theorem is that Mathieu's equation admits a complex-valued solution of form
F(a,q,x)=\exp(i\mux)P(a,q,x),
\mu
P
x
\pi
P(a,q,x)
Since Mathieu's equation is a second order differential equation, one can construct two linearly independent solutions. Floquet's theory says that if
a
cen(x,q)
sen(x,q)
fen(x,q)
gen(x,q)
z → \pminfty
The second solutions corresponding to the modified Mathieu functions
Cen(x,q)
Sen(x,q)
Fen(x,q)=-ifen(xi,q)
Gen(x,q)=gen(xi,q)
Mathieu functions of fractional order can be defined as those solutions
cep(x,q)
sep(x,q)
p
\cospx
\sinpx
q → 0
p
x → infty
An important property of the solutions
cep(x,q)
sep(x,q)
p
a
p
cep(x,q)
sep(x,q)
a
These classifications are summarized in the table below. The modified Mathieu function counterparts are defined similarly.
Order | First kind | Second kind | |
---|---|---|---|
Integral | cen(x,q) | fen(x,q) | |
Integral | sen(x,q) | gen(x,q) | |
Fractional( p | cep(x,q) | sep(x,q) |
Mathieu functions of the first kind can be represented as Fourier series:[5]
\begin{align} ce2n(x,q)&=
infty | |
\sum | |
r=0 |
(2n) | |
A | |
2r |
(q)\cos(2rx)\\ ce2n+1(x,q)&=
infty | |
\sum | |
r=0 |
(2n+1) | |
A | |
2r+1 |
(q)\cos\left[(2r+1)x\right]\\ se2n+1(x,q)&=
infty | |
\sum | |
r=0 |
(2n+1) | |
B | |
2r+1 |
(q)\sin\left[(2r+1)x\right]\\ se2n+2(x,q)&=
infty | |
\sum | |
r=0 |
(2n+2) | |
B | |
2r+2 |
(q)\sin\left[(2r+2)x\right]\\ \end{align}
(i) | |
A | |
j |
(q)
(i) | |
B | |
j |
(q)
q
x
ce2n
\begin{align} aA0-qA2&=0\\ (a-4)A2-q(A4+2A0)&=0\\ (a-4r2)A2r-q(A2r+2+A2r-2)&=0, r\geq2 \end{align}
2r
X2r
Y2r
A2r=c1X2r+c2Y2r
\begin{align} X2r&=r-2r-1\left(-
e2q | |
4 |
\right)r\left[1+l{O}(r-1)\right]\\ Y2r&=r2r-1\left(-
4 | |
e2q |
\right)r\left[1+l{O}(r-1)\right] \end{align}
X2r
Y2r
A2r=c1X2r+c2Y2r
ce2n
a
c2=0.
a
In general, however, the solution of a three-term recurrence with variable coefficientscannot be represented in a simple manner, and hence there is no simple way to determine
a
c2=0
A2r
r
a
c2
0
Y2r
r
To overcome these issues, more sophisticated semi-analytical/numerical approaches are required, for instance using a continued fraction expansion,[16] [5] casting the recurrence as a matrix eigenvalue problem,[17] or implementing a backwards recurrence algorithm.[15] The complexity of the three-term recurrence relation is one of the reasons there are few simple formulas and identities involving Mathieu functions.[18]
In practice, Mathieu functions and the corresponding characteristic numbers can be calculated using pre-packaged software, such as Mathematica, Maple, MATLAB, and SciPy. For small values of
q
n
q
There are several ways to represent Mathieu functions of the second kind.[20] One representation is in terms of Bessel functions:[21]
\begin{align} fe2n(x,q)&=-
\pi\gamman | |
2 |
infty | |
\sum | |
r=0 |
(-1)r+n
(2n) | |
A | |
2r |
(-q)
ix | |
Im[J | |
r(\sqrt{q}e |
)
-ix | |
Y | |
r(\sqrt{q}e |
)], where\gamman=\left\{ \begin{array}{cc} \sqrt{2},&ifn=0\\ 2n,&ifn\geq1 \end{array} \right.\\ fe2n+1(x,q)&=
\pi\sqrt{q | |
n,q>0
Jr(x)
Yr(x)
A traditional approach for numerical evaluation of the modified Mathieu functions is through Bessel function product series.[22] For large
n
q
There are relatively few analytic expressions and identities involving Mathieu functions. Moreover, unlike many other special functions, the solutions of Mathieu's equation cannot in general be expressed in terms of hypergeometric functions. This can be seen by transformation of Mathieu's equation to algebraic form, using the change of variable
t=\cos(x)
| ||||
(1-t |
-t
dy | |
dt |
+(a+2q(1-2t2))y=0.
Since this equation has an irregular singular point at infinity, it cannot be transformed into an equation of the hypergeometric type.[18]
For small
q
cen
sen
\cosnx
\sinnx
q
q
cem(x,q)
sem+1(x,q)
m
0<x<\pi
q → infty
x=\pi/2
For
q>0
x → infty
In the following, the
A
B
cen
sen
q
n
x
Due to their parity and periodicity,
cen
sen
\pi
\begin{align} &cen(x+\pi)=(-1)ncen(x)\\ &sen(x+\pi)=(-1)nsen(x)\\ &cen(x+\pi/2)=(-1)ncen(-x+\pi/2)\\ &sen+1(x+\pi/2)=(-1)nsen+1(-x+\pi/2) \end{align}
One can also write functions with negative
q
q
\begin{align} &ce2n+1(x,-q)=(-1)nse2n+1(-x+\pi/2,q)\\ &ce2n+2(x,-q)=(-1)nce2n+2(-x+\pi/2,q)\\ &se2n+1(x,-q)=(-1)nce2n+1(-x+\pi/2,q)\\ &se2n+2(x,-q)=(-1)nse2n+2(-x+\pi/2,q)\end{align}
Moreover,
\begin{align} &a2n+1(q)=b2n+1(-q)\\ &b2n+2(q)=b2n+2(-q) \end{align}
Like their trigonometric counterparts
\cosnx
\sinnx
cen(x,q)
sen(x,q)
2\pi | |
\begin{align} &\int | |
0 |
cencemdx=
2\pi | |
\int | |
0 |
sensemdx=\deltanm\pi
2\pi | |
\\ &\int | |
0 |
censemdx=0 \end{align}
Moreover, with
q
a
cen(x,q)
sen(x,q)
\pi
2\pi
x
cen(x,q)
sen(x,q)
\chi(x,x')
\partial2\chi | |
\partialx2 |
-
\partial2\chi | |
\partialx'2 |
=2q\left(\cos2x-\cos2x'\right)\chi
\phi(x)
a
q
\psi(x)\equiv\intC\chi(x,x')\phi(x')dx'
C
a
q
\chi(x,x')
\partial2\chi | |
\partialx2 |
-
\partial2\chi | |
\partialx'2 |
=2q\left(\cos2x-\cos2x'\right)\chi
\psi(x)
\chi(x,x')
\left(\phi
\partial\chi | |
\partialx' |
-
\partial\phi | |
\partialx' |
\chi\right)
C
Using an appropriate change of variables, the equation for
\chi
\chi(x,x')=\sinh(2q1/2\sinx\sinx')
\begin{align} se2n+1(x,q)&=
se'2n+1(0,q) | ||||||||
|
\pi | |
\int | |
0 |
\sinh(2q1/2\sinx\sinx')se2n+1(x',q)dx' (q>0)\\ Ce2n(x,q)&=
ce2n(\pi/2,q) | ||||||||
|
\pi | |
\int | |
0 |
\cos(2q1/2\coshx\cosx')ce2n(x',q)dx' (q>0) \end{align}
Identities of the latter type are useful for studying asymptotic properties of the modified Mathieu functions.[30]
There also exist integral relations between functions of the first and second kind, for instance:[21]
fe2n(x,q)=2n
x | |
\int | |
0 |
ce2n(\tau,-q) J0\left(\sqrt{2q(\cos2x-\cos2\tau)}\right)d\tau, n\geq1
x
q
The following asymptotic expansions hold for
q>0
Im(x)=0
Re(x) → infty
2q1/2\coshx\simeqq1/2ex
\begin{align} Ce2n(x,q)&\sim\left(
2 | |
\piq1/2 |
\right)1/2
ce2n(0,q)ce2n(\pi/2,q) | ||||||
|
⋅ e-x/2\sin\left(q1/2ex+
\pi | |
4 |
\right)\\ Ce2n+1(x,q)&\sim\left(
2 | |
\piq3/2 |
\right)1/2
ce2n+1(0,q)ce'2n+1(\pi/2,q) | ||||||
|
⋅ e-x/2\cos\left(q1/2ex+
\pi | |
4 |
\right)\\ Se2n+1(x,q)&\sim-\left(
2 | |
\piq3/2 |
\right)1/2
se'2n+1(0,q)se2n+1(\pi/2,q) | ||||||
|
⋅ e-x/2\cos\left(q1/2ex+
\pi | |
4 |
\right)\\ Se2n+2(x,q)&\sim\left(
2 | |
\piq5/2 |
\right)1/2
se'2n+2(0,q)se'2n+2(\pi/2,q) | ||||||
|
⋅ e-x/2\sin\left(q1/2ex+
\pi | |
4 |
\right) \end{align}
Thus, the modified Mathieu functions decay exponentially for large real argument. Similar asymptotic expansions can be written down for
Fen
Gen
For the even and odd periodic Mathieu functions
ce,se
a
q
N
N ≈ N0=2n+1,n=1,2,3,...,
\begin{align} a(N)={}&-2q+2q1/2N-
1 | |
23 |
(N2+1)-
1 | |
27q1/2 |
N(N2+3)-
1 | |
212q |
(5N4+34N2+9)\\ &-
1 | |
217q3/2 |
N(33N4+410N2+405)-
1 | |
220q2 |
(63N6+1260N4+2943N2+41807)+ l{O}(q-5/2) \end{align}
q1/2
N
-q1/2
-N
|q|-7/2
N
q\toinfty
\cos2x
N0
q
a\toa\mp
\left( |
| ||||
dx |
\right)\pi/2=0,
ce | |
N0 |
(\pi/2)=0, \left(
| |||||
dx |
\right)\pi/2=0,
se | |
N0+1 |
(\pi/2)=0.
a
N-N0=\mp2\left(
2 | |
\pi |
\right)1/2
| \left[1- | |||||||||||||||
|
| |||||||
26q1/2 |
+
1 | |
213q |
4 | |
(9N | |
0 |
3 | |
-40N | |
0 |
2 | |
+18N | |
0 |
-136N0+9)+...\right].
a(N)=a(N0)+(N-N0)\left(
\partiala | |
\partialN |
\right) | |
N0 |
+ … .
\begin{align} a(N)\toa\mp(N0)={}&-2q+2q1/2N0-
1 | |
23 |
2 | |
(N | |
0+1) |
-
1 | |
27q1/2 |
N0(N
2+3) | ||
- | ||
0 |
1 | |
212q |
2 | |
(5N | |
0 |
+9)- … \\ &\mp
| [1- | |||||||||||||||
|
N0 | |
26q1/2 |
2+8N | |
(3N | |
0+3) |
+ … ]. \end{align}
N0=1,3,5,...
ce | |
N0 |
ce | |
N0-1 |
se | |
N0+1 |
se | |
N0 |
Similar asymptotic expansions can be obtained for the solutions of other periodic differential equations, as for Lamé functions and prolate and oblate spheroidal wave functions.
Mathieu's differential equations appear in a wide range of contexts in engineering, physics, and applied mathematics. Many of these applications fall into one of two general categories: 1) the analysis of partial differential equations in elliptic geometries, and 2) dynamical problems which involve forces that are periodic in either space or time. Examples within both categories are discussed below.
Mathieu functions arise when separation of variables in elliptic coordinates is applied to 1) the Laplace equation in 3 dimensions, and 2) the Helmholtz equation in either 2 or 3 dimensions. Since the Helmholtz equation is a prototypical equation for modeling the spatial variation of classical waves, Mathieu functions can be used to describe a variety of wave phenomena. For instance, in computational electromagnetics they can be used to analyze the scattering of electromagnetic waves off elliptic cylinders, and wave propagation in elliptic waveguides.[35] In general relativity, an exact plane wave solution to the Einstein field equation can be given in terms of Mathieu functions.
More recently, Mathieu functions have been used to solve a special case of the Smoluchowski equation, describing the steady-state statistics of self-propelled particles.[36]
The remainder of this section details the analysis for the two-dimensional Helmholtz equation.[37] In rectangular coordinates, the Helmholtz equation is
\left( | \partial2 | + |
\partialx2 |
\partial2 | |
\partialy2 |
\right)\psi+k2\psi=0,
\begin{align} x&=c\cosh\mu\cos\nu\\ y&=c\sinh\mu\sin\nu \end{align}
0\leq\mu<infty
0\leq\nu<2\pi
c
1 | \left( | |
c2(\sinh2\mu+\sin2\nu) |
\partial2 | + | |
\partial\mu2 |
\partial2 | |
\partial\nu2 |
\right)\psi+k2\psi=0
\mu
c
\psi(\mu,\nu)=F(\mu)G(\nu)
\begin{align} & | d2F |
d\mu2 |
-\left(a-
c2k2 | |
2 |
\cosh2\mu\right)F=0\\ &
d2G | |
d\nu2 |
+\left(a-
c2k2 | |
2 |
\cos2\nu\right)G=0\\ \end{align}
a
As a specific physical example, the Helmholtz equation can be interpreted as describing normal modes of an elastic membrane under uniform tension. In this case, the following physical conditions are imposed:[38]
\nu
\psi(\mu,\nu)=\psi(\mu,\nu+2\pi)
\psi(0,\nu)=\psi(0,-\nu)
\psi\mu(0,\nu)=-\psi\mu(0,-\nu)
For given
k
Cen(\mu,q)cen(\nu,q)
Sen(\mu,q)sen(\nu,q)
q=c2k2/4
a
k
k
\mu=\mu0>0
\mu=\mu0
\psi(\mu0,\nu)=0
\begin{align} Cen(\mu0,q)=0\\ Sen(\mu0,q)=0 \end{align}
In dynamical problems with periodically varying forces, the equation of motion sometimes takes the form of Mathieu's equation. In such cases, knowledge of the general properties of Mathieu's equation— particularly with regard to stability of the solutions—can be essential for understanding qualitative features of the physical dynamics.[39] A classic example along these lines is the inverted pendulum.[40] Other examples are
Mathieu functions play a role in certain quantum mechanical systems, particularly those with spatially periodic potentials such as the quantum pendulum and crystalline lattices.
The modified Mathieu equation also arises when describing the quantum mechanics of singular potentials. For the particular singular potential
V(r)=g2/r4
d2y | |
dr2 |
+\left[k2-
\ell(\ell+1) | - | |
r2 |
g2 | |
r4 |
\right]y=0
d2\varphi | |
dz2 |
+\left[2h2\cosh2z-\left(\ell+
1 | |
2 |
\right)2\right]\varphi=0.
y=r1/2\varphi,r=\gammaez,\gamma=
ig | |
h |
,h2=ikg,h=eI\pi/4(kg)1/2.
2\pi
y(x+\pi)=-y(x)