2.6 Distributional Methods2.8 Differential Equations with a Parameter

§2.7 Differential Equations

Contents

§2.7(i) Regular Singularities: Fuchs–Frobenius Theory

An ordinary point of the differential equation

2.7.1\frac{{d}^{2}w}{{dz}^{2}}+f(z)\frac{dw}{dz}+g(z)w=0

is one at which the coefficients f(z) and g(z) are analytic. All solutions are analytic at an ordinary point, and their Taylor-series expansions are found by equating coefficients.

Other points z_{0} are singularities of the differential equation. If both (z-z_{0})f(z) and (z-z_{0})^{2}g(z) are analytic at z_{0}, then z_{0} is a regular singularity (or singularity of the first kind). All other singularities are classified as irregular.

In a punctured neighborhood \mathbf{N} of a regular singularity z_{0}

2.7.2
f(z)=\sum _{{s=0}}^{{\infty}}f_{s}(z-z_{0})^{{s-1}},
g(z)=\sum _{{s=0}}^{{\infty}}g_{s}(z-z_{0})^{{s-2}},

with at least one of the coefficients f_{0}, g_{0}, g_{1} nonzero. Let \alpha _{1}, \alpha _{2} denote the indices or exponents, that is, the roots of the indicial equation

2.7.3Q(\alpha)\equiv\alpha(\alpha-1)+f_{0}\alpha+g_{0}=0.

Provided that \alpha _{1}-\alpha _{2} is not zero or an integer, equation (2.7.1) has independent solutions w_{j}(z), j=1,2, such that

2.7.4w_{j}(z)=(z-z_{0})^{{\alpha _{j}}}\sum _{{s=0}}^{{\infty}}a_{{s,j}}(z-z_{0})^{s},z\in\mathbf{N},

with a_{{0,j}}=1, and

2.7.5Q(\alpha _{j}+s)a_{{s,j}}=-\sum _{{r=0}}^{{s-1}}\left((\alpha _{j}+r)f_{{s-r}}+g_{{s-r}}\right)a_{{r,j}},

when s=1,2,3,\dots.

If \alpha _{1}-\alpha _{2}=0,1,2,\dots, then (2.7.4) applies only in the case j=1. But there is an independent solution

2.7.6w_{2}(z)=(z-z_{0})^{{\alpha _{2}}}\sum _{{\substack{s=0\\
s\neq\alpha _{1}-\alpha _{2}}}}^{{\infty}}b_{s}(z-z_{0})^{s}+cw_{1}(z)\mathop{\ln\/}\nolimits\!\left(z-z_{0}\right),z\in\mathbf{N}.

The coefficients b_{s} and constant c are again determined by equating coefficients in the differential equation, beginning with c=1 when \alpha _{1}-\alpha _{2}=0, or with b_{0}=1 when \alpha _{1}-\alpha _{2}=1,2,3,\dots.

The radii of convergence of the series (2.7.4), (2.7.6) are not less than the distance of the next nearest singularity of the differential equation from z_{0}.

To include the point at infinity in the foregoing classification scheme, we transform it into the origin by replacing z in (2.7.1) with 1/z; see Olver (1997b, pp. 153–154). For corresponding definitions, together with examples, for linear differential equations of arbitrary order see §§16.8(i)16.8(ii).

§2.7(ii) Irregular Singularities of Rank 1

If the singularities of f(z) and g(z) at z_{0} are no worse than poles, then z_{0} has rank \ell-1, where \ell is the least integer such that (z-z_{0})^{{\ell}}f(z) and (z-z_{0})^{{2\ell}}g(z) are analytic at z_{0}. Thus a regular singularity has rank 0. The most common type of irregular singularity for special functions has rank 1 and is located at infinity. Then

2.7.7
f(z)=\sum _{{s=0}}^{{\infty}}\frac{f_{s}}{z^{s}},
g(z)=\sum _{{s=0}}^{{\infty}}\frac{g_{s}}{z^{s}},

these series converging in an annulus |z|>a, with at least one of f_{0}, g_{0}, g_{1} nonzero.

Formal solutions are

2.7.8e^{{\lambda _{j}z}}z^{{\mu _{j}}}\sum _{{s=0}}^{{\infty}}\frac{a_{{s,j}}}{z^{s}},j=1,2,

where \lambda _{1}, \lambda _{2} are the roots of the characteristic equation

2.7.9\lambda^{2}+f_{0}\lambda+g_{0}=0,
2.7.10\mu _{j}=-(f_{1}\lambda _{j}+g_{1})/(f_{0}+2\lambda _{j}),

a_{{0,j}}=1, and

2.7.11(f_{0}+2\lambda _{j})sa_{{s,j}}=(s-\mu _{j})(s-1-\mu _{j})a_{{s-1,j}}+\sum _{{r=1}}^{{s}}\left(\lambda _{j}f_{{r+1}}+g_{{r+1}}-(s-r-\mu _{j})f_{r}\right)a_{{s-r,j}},

when s=1,2,\dots. The construction fails iff \lambda _{1}=\lambda _{2}, that is, when f_{0}^{2}=4g_{0}: this case is treated below.

For large s,

where \Lambda _{1} and \Lambda _{2} are constants, and the Jth remainder terms in the sums are \mathop{O\/}\nolimits\!\left(\mathop{\Gamma\/}\nolimits\!\left(s+\mu _{2}-\mu _{1}-J\right)\right) and \mathop{O\/}\nolimits\!\left(\mathop{\Gamma\/}\nolimits\!\left(s+\mu _{1}-\mu _{2}-J\right)\right), respectively (Olver (1994a)). Hence unless the series (2.7.8) terminate (in which case the corresponding \Lambda _{j} is zero) they diverge. However, there are unique and linearly independent solutions w_{j}(z), j=1,2, such that

2.7.14w_{j}(z)\sim e^{{\lambda _{j}z}}((\lambda _{2}-\lambda _{1})z)^{{\mu _{j}}}\sum _{{s=0}}^{{\infty}}\frac{a_{{s,j}}}{z^{s}}

as z\to\infty in the sectors

2.7.15-\tfrac{3}{2}\pi+\delta\leq\mathop{\mathrm{ph}\/}\nolimits\!\left((\lambda _{2}-\lambda _{1})z\right)\leq\tfrac{3}{2}\pi-\delta,j=1,
2.7.16-\tfrac{1}{2}\pi+\delta\leq\mathop{\mathrm{ph}\/}\nolimits\!\left((\lambda _{2}-\lambda _{1})z\right)\leq\tfrac{5}{2}\pi-\delta,j=2,

\delta being an arbitrary small positive constant.

Although the expansions (2.7.14) apply only in the sectors (2.7.15) and (2.7.16), each solution w_{j}(z) can be continued analytically into any other sector. Typical connection formulas are

2.7.17
w_{1}(z)=e^{{2\pi i\mu _{1}}}w_{1}(ze^{{-2\pi i}})+C_{1}w_{2}(z),
w_{2}(z)=e^{{-2\pi i\mu _{2}}}w_{2}(ze^{{2\pi i}})+C_{2}w_{1}(z),

in which C_{1}, C_{2} are constants, the so-called Stokes multipliers. In combination with (2.7.14) these formulas yield asymptotic expansions for w_{1}(z) in \frac{1}{2}\pi+\delta\leq\mathop{\mathrm{ph}\/}\nolimits\!\left((\lambda _{2}-\lambda _{1})z\right)\leq\frac{5}{2}\pi-\delta, and w_{2}(z) in -\frac{3}{2}\pi+\delta\leq\mathop{\mathrm{ph}\/}\nolimits\!\left((\lambda _{2}-\lambda _{1})z\right)\leq\frac{1}{2}\pi-\delta. Furthermore,

2.7.18
\Lambda _{1}=-ie^{{(\mu _{2}-\mu _{1})\pi i}}C_{1}/(2\pi),
\Lambda _{2}=iC_{2}/(2\pi).

Note that the coefficients in the expansions (2.7.12), (2.7.13) for the “late” coefficients, that is, a_{{s,1}}, a_{{s,2}} with s large, are the “early” coefficients a_{{j,2}}, a_{{j,1}} with j small. This phenomenon is an example of resurgence, a classification due to Écalle (1981a, b). See §2.11(v) for other examples.

The exceptional case f_{0}^{2}=4g_{0} is handled by Fabry’s transformation:

2.7.19
w=e^{{-f_{0}z/2}}W,
t=z^{{1/2}}.

The transformed differential equation either has a regular singularity at t=\infty, or its characteristic equation has unequal roots.

For error bounds for (2.7.14) see Olver (1997b, Chapter 7). For the calculation of Stokes multipliers see Olde Daalhuis and Olver (1995b). For extensions to singularities of higher rank see Olver and Stenger (1965). For extensions to higher-order differential equations see Stenger (1966a, b), Olver (1997a, 1999), and Olde Daalhuis and Olver (1998).

§2.7(iii) Liouville–Green (WKBJ) Approximation

For irregular singularities of nonclassifiable rank, a powerful tool for finding the asymptotic behavior of solutions, complete with error bounds, is as follows:

Liouville–Green Approximation Theorem

In a finite or infinite interval (a_{1},a_{2}) let f(x) be real, positive, and twice-continuously differentiable, and g(x) be continuous. Then in (a_{1},a_{2}) the differential equation

2.7.20\frac{{d}^{2}w}{{dx}^{2}}=(f(x)+g(x))w

has twice-continuously differentiable solutions

such that

2.7.23|\epsilon _{j}(x)|,\;\;\tfrac{1}{2}f^{{-1/2}}(x)|\epsilon _{j}^{{\prime}}(x)|\leq\mathop{\exp\/}\nolimits\!\left(\tfrac{1}{2}\mathop{\mathcal{V}_{{a_{j},x}}\/}\nolimits\!\left(F\right)\right)-1,j=1,2,

provided that \mathop{\mathcal{V}_{{a_{j},x}}\/}\nolimits\!\left(F\right)<\infty. Here F(x) is the error-control function

2.7.24F(x)=\int\left(\frac{1}{f^{{1/4}}}\frac{{d}^{2}}{{dx}^{2}}\left(\frac{1}{f^{{1/4}}}\right)-\frac{g}{f^{{1/2}}}\right)dx,

and \mathop{\mathcal{V}\/}\nolimits denotes the variational operator (§2.3(i)). Thus

2.7.25\mathop{\mathcal{V}_{{a_{j},x}}\/}\nolimits\!\left(F\right)=\int _{{a_{j}}}^{{x}}\left|\left(\frac{1}{f^{{1/4}}(t)}\frac{{d}^{2}}{{dt}^{2}}\left(\frac{1}{f^{{1/4}}(t)}\right)-\frac{g(t)}{f^{{1/2}}(t)}\right)dt\right|.

Assuming also \mathop{\mathcal{V}_{{a_{1},a_{2}}}\/}\nolimits\!\left(F\right)<\infty, we have

2.7.26w_{1}(x)\sim f^{{-1/4}}(x)\mathop{\exp\/}\nolimits\!\left(\int f^{{1/2}}(x)dx\right),x\to a_{1}+,
2.7.27w_{2}(x)\sim f^{{-1/4}}(x)\mathop{\exp\/}\nolimits\!\left(-\int f^{{1/2}}(x)dx\right),x\to a_{2}-.

Suppose in addition |\int f^{{1/2}}(x)dx| is unbounded as x\to a_{1}+ and x\to a_{2}-. Then there are solutions w_{3}(x), w_{4}(x), such that

2.7.28w_{3}(x)\sim f^{{-1/4}}(x)\mathop{\exp\/}\nolimits\!\left(\int f^{{1/2}}(x)dx\right),x\to a_{2}-,
2.7.29w_{4}(x)\sim f^{{-1/4}}(x)\mathop{\exp\/}\nolimits\!\left(-\int f^{{1/2}}(x)dx\right),x\to a_{1}+.

The solutions with the properties (2.7.26), (2.7.27) are unique, but not those with the properties (2.7.28), (2.7.29). In fact, since

2.7.30w_{1}(x)/w_{4}(x)\to 0,x\to a_{1}+,

w_{1}(x) is a recessive (or subdominant) solution as x\to a_{1}+, and w_{4}(x) is a dominant solution as x\to a_{1}+. Similarly for w_{2}(x) and w_{3}(x) as x\to a_{2}-.

Example

2.7.31\frac{{d}^{2}w}{{dx}^{2}}=(x+\mathop{\ln\/}\nolimits x)w,0<x<\infty.

We cannot take f=x and g=\mathop{\ln\/}\nolimits x because \int gf^{{-1/2}}dx would diverge as x\to+\infty. Instead set f=x+\mathop{\ln\/}\nolimits x, g=0. By approximating

2.7.32f^{{1/2}}=x^{{1/2}}+\tfrac{1}{2}x^{{-1/2}}\mathop{\ln\/}\nolimits x+\mathop{O\/}\nolimits\!\left(x^{{-3/2}}(\mathop{\ln\/}\nolimits x)^{2}\right),

we arrive at

as x\to+\infty, w_{2}(x) being recessive and w_{3}(x) dominant.

For other examples, and also the corresponding results when f(x) is negative, see Olver (1997b, Chapter 6), Olver (1980a), Taylor (1978, 1982), and Smith (1986). The first of these references includes extensions to complex variables and reversions for zeros.

§2.7(iv) Numerically Satisfactory Solutions

One pair of independent solutions of the equation

2.7.35\ifrac{{d}^{2}w}{{dz}^{2}}=w

is w_{1}(z)=e^{z}, w_{2}(z)=e^{{-z}}. Another is w_{3}(z)=\mathop{\cosh\/}\nolimits z, w_{4}(z)=\mathop{\sinh\/}\nolimits z. In theory either pair may be used to construct any other solution

2.7.36w(z)=Aw_{1}(z)+Bw_{2}(z),

or

2.7.37w(z)=Cw_{3}(z)+Dw_{4}(z),

where A,B,C,D are constants. From the numerical standpoint, however, the pair w_{3}(z) and w_{4}(z) has the drawback that severe numerical cancellation can occur with certain combinations of C and D, for example if C and D are equal, or nearly equal, and z, or \realpart{z}, is large and negative. This kind of cancellation cannot take place with w_{1}(z) and w_{2}(z), and for this reason, and following Miller (1950), we call w_{1}(z) and w_{2}(z) a numerically satisfactory pair of solutions.

The solutions w_{1}(z) and w_{2}(z) are respectively recessive and dominant as \realpart{z}\to-\infty, and vice versa as \realpart{z}\to+\infty. This is characteristic of numerically satisfactory pairs. In a neighborhood, or sectorial neighborhood of a singularity, one member has to be recessive. In consequence, if a differential equation has more than one singularity in the extended plane, then usually more than two standard solutions need to be chosen in order to have numerically satisfactory representations everywhere.

In oscillatory intervals, and again following Miller (1950), we call a pair of solutions numerically satisfactory if asymptotically they have the same amplitude and are \tfrac{1}{2}\pi out of phase.