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7.3 Singular Points and the Method of Frobenius

Examples

While behavior of ODEs at singular points is more complicated, certain singular points are not especially difficult to solve. Let us look at some examples before giving a general method. We may be lucky and obtain a power series solution using the method of the previous section, but in general we may have to try other things.

Function graph showing the slope field of the differential equation dy/dx = r*y/x, drawn from 308 sample slopes, y = abs(x)^r, y = 0.5*abs(x)^r and y = -0.8*abs(x)^r. Adjustable parameter: Frobenius exponent r (r) = 0.5. Viewing window: x from -4 to 4, y from -2.47 to 2.47.
The slope field of x y′ = r y with three of its solutions y = C|x|^r drawn through it. The equation worked just below, 2xy′ − y = 0, is the case r = 1/2 — where the figure opens — because substituting y = x^r turns the ODE into the indicial equation for r. Drag the slider to watch the singular point change character: for r < 0 the solutions themselves blow up at x = 0; at r = 0 they flatten into the horizontal lines y = C; for 0 < r < 1, the range containing Lebl's r = 1/2, they reach the origin with a vertical tangent, which is why the trivial y = 0 is the only solution differentiable there; at r = 1 the two branches meet in a corner; and only for r > 1 do they arrive with zero slope and the singular point stop hurting.

Not every problem with a singular point has a solution of the form y=xr, of course. But perhaps we can combine the methods. What we will do is to try a solution of the form

y = x r f ( x )

where f(x) is an analytic function.

Method of Frobenius

Before giving the general method, let us clarify when the method applies. Let

p ( x ) y + q ( x ) y + r ( x ) y = 0

be an ODE. As before, if p(x0)=0, then x0 is a singular point. If, furthermore, the limits

lim x x 0   ( x x 0 ) q ( x ) p ( x ) and lim x x 0   ( x x 0 ) 2 r ( x ) p ( x )

both exist and are finite, then we say that x0 is a regular singular point.

Let us now discuss the general Method of Frobeniusto the power 1. Let us only consider the method at the point x=0 for simplicity. The main idea is the following theorem.

The method usually breaks down like this.

  1. We seek a Frobenius-type solution of the form

    y=k=0akxk+r.

    We plug this y into equation (7.3.7). We collect terms and write everything as a single series.
  2. The obtained series must be zero. Setting the first coefficient (usually the coefficient of xr) in the series to zero we obtain the indicial equation, which is a quadratic polynomial in r.
  3. If the indicial equation has two real roots r1 and r2 such that r1r2 is not an integer, then we have two linearly independent Frobenius-type solutions. Using the first root, we plug in

    y1=xr1k=0akxk,

    and we solve for all ak to obtain the first solution. Then using the second root, we plug in

    y2=xr2k=0bkxk,

    and solve for all bk to obtain the second solution.
  4. If the indicial equation has a doubled root r, then there we find one solution

    y1=xrk=0akxk,

    and then we obtain a new solution by plugging

    y2=xrk=0bkxk+(lnx)y1,

    into Equation (7.3.7) and solving for the constants bk.
  5. If the indicial equation has two real roots such that r1r2 is an integer, then one solution is

    y1=xr1k=0akxk,

    and the second linearly independent solution is of the form

    y2=xr2k=0bkxk+C(lnx)y1,

    where we plug y2 into (7.3.7) and solve for the constants bk and C.
  6. Finally, if the indicial equation has complex roots, then solving for ak in the solution

    y=xr1k=0akxk

    results in a complex-valued function---all the ak are complex numbers. We obtain our two linearly independent solutionssquared by taking the real and imaginary parts of y.

The main idea is to find at least one Frobenius-type solution. If we are lucky and find two, we are done. If we only get one, we either use the ideas above or even a different method such as reduction of order (Exercise 2.1.8) to obtain a second solution.

Bessel Functions

An important class of functions that arises commonly in physics are the Bessel functionscubed. For example, these functions appear when solving the wave equation in two and three dimensions. First we have Bessel's equation of order p:

x 2 y + x y + ( x 2 p 2 ) y = 0 .

We allow p to be any number, not just an integer, although integers and multiples of 12 are most important in applications. When we plug

y = k = 0 a k x k + r

into Bessel's equation of order p we obtain the indicial equation

r ( r 1 ) + r p 2 = ( r p ) ( r + p ) = 0 .

Therefore we obtain two roots r1=p and r2=p. If p is not an integer following the method of Frobenius and setting a0=1, we obtain linearly independent solutions of the form

y 1 = x p k = 0 ( 1 ) k x 2 k 2 2 k k ! ( k + p ) ( k 1 + p ) ( 2 + p ) ( 1 + p ) , y 2 = x p k = 0 ( 1 ) k x 2 k 2 2 k k ! ( k p ) ( k 1 p ) ( 2 p ) ( 1 p ) .

Bessel functions will be convenient constant multiples of y1 and y2. First we must define the gamma function

Γ ( x ) = 0 t x 1 e t d t .

Notice that Γ(1)=1. The gamma function also has a wonderful property

Γ ( x + 1 ) = x Γ ( x ) .

From this property, one can show that Γ(n)=(n1)! when n is an integer, so the gamma function is a continuous version of the factorial. We compute:

Γ ( k + p + 1 ) = ( k + p ) ( k 1 + p ) ( 2 + p ) ( 1 + p ) Γ ( 1 + p ) , Γ ( k p + 1 ) = ( k p ) ( k 1 p ) ( 2 p ) ( 1 p ) Γ ( 1 p ) .

We define the Bessel functions of the first kind of order p and p as

J p ( x ) = 1 2 p Γ ( 1 + p ) y 1 = k = 0 ( 1 ) k k ! Γ ( k + p + 1 ) ( x 2 ) 2 k + p , J p ( x ) = 1 2 Γ ( 1 p ) y 2 = k = 0 ( 1 ) k k ! Γ ( k p + 1 ) ( x 2 ) 2 k p .

As these are constant multiples of the solutions we found above, these are both solutions to Bessel's equation of order p. The constants are picked for convenience.

When p is not an integer, Jp and Jp are linearly independent. When n is an integer we obtain

J n ( x ) = k = 0 ( 1 ) k k ! ( k + n ) ! ( x 2 ) 2 k + n .

In this case it turns out that

J n ( x ) = ( 1 ) n J n ( x ) ,

and so we do not obtain a second linearly independent solution. The other solution is the so-called Bessel function of second kind. These make sense only for integer orders n and are defined as limits of linear combinations of Jp(x) and Jp(x) as p approaches n in the following way:

Y n ( x ) = lim p n cos ( p π ) J p ( x ) J p ( x ) sin ( p π ) .

As each linear combination of Jp(x) and Jp(x) is a solution to Bessel's equation of order p, then as we take the limit as p goes to n, Yn(x) is a solution to Bessel's equation of order n. It also turns out that Yn(x) and Jn(x) are linearly independent. Therefore when n is an integer, we have the general solution to Bessel's equation of order n

y = A J n ( x ) + B Y n ( x ) ,

for arbitrary constants A and B. Note that Yn(x) goes to negative infinity at x=0. Many mathematical software packages have these functions Jn(x) and Yn(x) defined, so they can be used just like say sin(x) and cos(x). In fact, they have some similar properties. For example, J1(x) is a derivative of J0(x), and in general the derivative of Jn(x) can be written as a linear combination of Jn1(x) and Jn+1(x). Furthermore, these functions oscillate, although they are not periodic. See Figure 1 for graphs of Bessel functions.

Two side-by-side plots for x from 0 to 10, each a pair of decaying oscillations about a quarter period out of step. On the left the blue curve starts at 1 and the green at 0, peaking near 0.58; on the right both plunge toward minus infinity as x approaches 0.
Figure 1: Plot of the J0(x) and J1(x) in the first graph and Y0(x) and Y1(x) in the second graph.

Footnotes

[1] Named after the German mathematician Ferdinand Georg Frobenius (1849 – 1917).

[2] See Joseph L. Neuringera, The Frobenius method for complex roots of the indicial equation, International Journal of Mathematical Education in Science and Technology, Volume 9, Issue 1, 1978, 71–77.

[3] Named after the German astronomer and mathematician Friedrich Wilhelm Bessel (1784 – 1846).

Adapted from Differential Equations for Engineers by Jiří Lebl (Oklahoma State University), hosted on LibreTexts (math.libretexts.org) and licensed under CC BY-SA 4.0. Changes were made. License: CC-BY-SA-4.0.