Frobenius solution to the hypergeometric equation

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In the following we solve the second-order differential equation called the hypergeometric differential equation using Frobenius method, named after Ferdinand Georg Frobenius. This is a method that uses the series solution for a differential equation, where we assume the solution takes the form of a series. This is usually the method we use for complicated ordinary differential equations. The solution of the hypergeometric differential equation is very important. For instance, Legendre's differential equation can be shown to be a special case of the hypergeometric differential equation. Hence, by solving the hypergeometric differential equation, one may directly compare its solutions to get the solutions of Legendre's differential equation, after making the necessary substitutions. For more details, please check the hypergeometric differential equation.

We shall prove that this equation has three singularities, namely at x = 0, x = 1 and around x = infinity. However, as these will turn out to be regular singular points, we will be able to assume a solution on the form of a series. Since this is a second-order differential equation, we must have two linearly independent solutions.

The problem however will be that our assumed solutions may or not be independent, or worse, may not even be defined (depending on the value of the parameters of the equation). This is why we shall study the different cases for the parameters and modify our assumed solution accordingly.

The equation

Solve the hypergeometric equation around all singularities:

x(1x)y+{γ(1+α+β)x}yαβy=0

Solution around x = 0

Let

P0(x)=αβ,P1(x)=γ(1+α+β)x,P2(x)=x(1x)

Then

P2(0)=P2(1)=0.

Hence, x = 0 and x = 1 are singular points. Let's start with x = 0. To see if it is regular, we study the following limits:

limxa(xa)P1(x)P2(x)=limx0(x0)(γ(1+α+β)x)x(1x)=limx0x(γ(1+α+β)x)x(1x)=γlimxa(xa)2P0(x)P2(x)=limx0(x0)2(αβ)x(1x)=limx0x2(αβ)x(1x)=0

Hence, both limits exist and x = 0 is a regular singular point. Therefore, we assume the solution takes the form

y=r=0arxr+c

with a0 ≠ 0. Hence,

y=r=0ar(r+c)xr+c1y=r=0ar(r+c)(r+c1)xr+c2.

Substituting these into the hypergeometric equation, we get

xr=0ar(r+c)(r+c1)xr+c2x2r=0ar(r+c)(r+c1)xr+c2+γr=0ar(r+c)xr+c1(1+α+β)xr=0ar(r+c)xr+c1αβr=0arxr+c=0

That is,

r=0ar(r+c)(r+c1)xr+c1r=0ar(r+c)(r+c1)xr+c+γr=0ar(r+c)xr+c1(1+α+β)r=0ar(r+c)xr+cαβr=0arxr+c=0

In order to simplify this equation, we need all powers to be the same, equal to r + c − 1, the smallest power. Hence, we switch the indices as follows:

r=0ar(r+c)(r+c1)xr+c1r=1ar1(r+c1)(r+c2)xr+c1+γr=0ar(r+c)xr+c1(1+α+β)r=1ar1(r+c1)xr+c1αβr=1ar1xr+c1=0

Thus, isolating the first term of the sums starting from 0 we get

a0(c(c1)+γc)xc1+r=1ar(r+c)(r+c1)xr+c1r=1ar1(r+c1)(r+c2)xr+c1+γr=1ar(r+c)xr+c1(1+α+β)r=1ar1(r+c1)xr+c1αβr=1ar1xr+c1=0

Now, from the linear independence of all powers of x, that is, of the functions 1, x, x2, etc., the coefficients of xk vanish for all k. Hence, from the first term, we have

a0(c(c1)+γc)=0

which is the indicial equation. Since a0 ≠ 0, we have

c(c1+γ)=0.

Hence,

c1=0,c2=1γ

Also, from the rest of the terms, we have

((r+c)(r+c1)+γ(r+c))ar+((r+c1)(r+c2)(1+α+β)(r+c1)αβ)ar1=0

Hence,

ar=(r+c1)(r+c2)+(1+α+β)(r+c1)+αβ(r+c)(r+c1)+γ(r+c)ar1=(r+c1)(r+c+α+β1)+αβ(r+c)(r+c+γ1)ar1

But

(r+c1)(r+c+α+β1)+αβ=(r+c1)(r+c+α1)+(r+c1)β+αβ=(r+c1)(r+c+α1)+β(r+c+α1)

Hence, we get the recurrence relation

ar=(r+c+α1)(r+c+β1)(r+c)(r+c+γ1)ar1, for r1.

Let's now simplify this relation by giving ar in terms of a0 instead of ar−1. From the recurrence relation (note: below, expressions of the form (u)r refer to the Pochhammer symbol).

a1=(c+α)(c+β)(c+1)(c+γ)a0a2=(c+α+1)(c+β+1)(c+2)(c+γ+1)a1=(c+α+1)(c+α)(c+β)(c+β+1)(c+2)(c+1)(c+γ)(c+γ+1)a0=(c+α)2(c+β)2(c+1)2(c+γ)2a0a3=(c+α+2)(c+β+2)(c+3)(c+γ+2)a2=(c+α)2(c+α+2)(c+β)2(c+β+2)(c+1)2(c+3)(c+γ)2(c+γ+2)a0=(c+α)3(c+β)3(c+1)3(c+γ)3a0

As we can see,

ar=(c+α)r(c+β)r(c+1)r(c+γ)ra0, for r0

Hence, our assumed solution takes the form

y=a0r=0(c+α)r(c+β)r(c+1)r(c+γ)rxr+c.

We are now ready to study the solutions corresponding to the different cases for c1 − c2 = γ − 1 (this reduces to studying the nature of the parameter γ: whether it is an integer or not).

Analysis of the solution in terms of the difference γ − 1 of the two roots

γ not an integer

Then y1 = y|c = 0 and y2 = y|c = 1 − γ. Since

y=a0r=0(c+α)r(c+β)r(c+1)r(c+γ)rxr+c,

we have

y1=a0r=0(α)r(β)r(1)r(γ)rxr=a02F1(α,β;γ;x)y2=a0r=0(α+1γ)r(β+1γ)r(1γ+1)r(1γ+γ)rxr+1γ=a0x1γr=0(α+1γ)r(β+1γ)r(1)r(2γ)rxr=a0x1γ2F1(αγ+1,βγ+1;2γ;x)

Hence, y=Ay1+By2. Let A′ a0 = a and Ba0 = B. Then

y=A2F1(α,β;γ;x)+Bx1γ2F1(αγ+1,βγ+1;2γ;x)

γ = 1

Then y1 = y|c = 0. Since γ = 1, we have

y=a0r=0(c+α)r(c+β)r(c+1)r2xr+c.

Hence,

y1=a0r=0(α)r(β)r(1)r(1)rxr=a02F1(α,β;1;x)y2=yc|c=0.

To calculate this derivative, let

Mr=(c+α)r(c+β)r(c+1)r2.

Then

ln(Mr)=ln((c+α)r(c+β)r(c+1)r2)=ln(c+α)r+ln(c+β)r2ln(c+1)r

But

ln(c+α)r=ln((c+α)(c+α+1)(c+α+r1))=k=0r1ln(c+α+k).

Hence,

ln(Mr)=k=0r1ln(c+α+k)+k=0r1ln(c+β+k)2k=0r1ln(c+1+k)=k=0r1(ln(c+α+k)+ln(c+β+k)2ln(c+1+k))

Differentiating both sides of the equation with respect to c, we get:

1MrMrc=k=0r1(1c+α+k+1c+β+k2c+1+k).

Hence,

Mrc=(c+α)r(c+β)r(c+1)r2k=0r1(1c+α+k+1c+β+k2c+1+k).

Now,

y=a0xcr=0(c+α)r(c+β)r(c+1)r2xr=a0xcr=0Mrxr.

Hence,

yc=a0xcln(x)r=0(c+α)r(c+β)r(c+1)r2xr+a0xcr=0((c+α)r(c+β)r(c+1)r2{k=0r1(1c+α+k+1c+β+k2c+1+k)})xr=a0xcr=0(c+α)r(c+β)r(c+1)r)2(lnx+k=0r1(1c+α+k+1c+β+k2c+1+k))xr.

For c = 0, we get

y2=a0r=0(α)r(β)r(1)r2(lnx+k=0r1(1α+k+1β+k21+k))xr.

Hence, y = Cy1 + Dy2. Let Ca0 = C and Da0 = D. Then

y=C2F1(α,β;1;x)+Dr=0(α)r(β)r(1)r2(ln(x)+k=0r1(1α+k+1β+k21+k))xr

γ an integer and γ ≠ 1

γ ≤ 0

The value of γ is γ=0,1,2,. To begin with, we shall simplify matters by concentrating a particular value of γ and generalise the result at a later stage. We shall use the value γ=2. The indicial equation has a root at c=0, and we see from the recurrence relation

ar=(r+c+α1)(r+c+β1)(r+c)(r+c3)ar1,

that when r=3 that that denominator has a factor c which vanishes when c=0. In this case, a solution can be obtained by putting a0=b0c where b0 is a constant.

With this substitution, the coefficients of xr vanish when c=0 and r<3. The factor of c in the denominator of the recurrence relation cancels with that of the numerator when r3. Hence, our solution takes the form

y1=b0(2)×(1)((α)3(β)3(3!0!x3+(α)4(β)44!1!x4+(α)5(β)55!2!x5+)

=b0(2)2r=3(α)r(β)rr!(r3)!xr=b0(2)2(α)3(β)33!r=3(α+3)r3(β+3)r3(1+3)r3(r3)!xr.

If we start the summation at r=0 rather than r=3 we see that

y1=b0(α)3(β)3(2)2×3!x32F1(α+3,β+3;(1+3);x).

The result (as we have written it) generalises easily. For γ=1+m, with m=1,2,3, then

y1=b0(α)m(β)m(1m)m1×m!xm2F1(α+m,β+m;(1+m);x).

Obviously, if γ=2, then m=3. The expression for y1(x) we have just given looks a little inelegant since we have a multiplicative constant apart from the usual arbitrary multiplicative constant b0. Later, we shall see that we can recast things in such a way that this extra constant never appears

The other root to the indicial equation is c=1γ=3, but this gives us (apart from a multiplicative constant) the same result as found using c=0. This means we must take the partial derivative (w.r.t. c) of the usual trial solution in order to find a second independent solution. If we define the linear operator L as

L=x(1x)d2dx2(α+β+1)xddx+γddxαβ,

then since γ=2 in our case,

Lcr=0br(c)xr=b0c2(c3).

(We insist that b00.) Taking the partial derivative w.r.t c,

Lccr=0br(c)xr+c=b0(3c26c).

Note that we must evaluate the partial derivative at c=0 (and not at the other root c=3). Otherwise the right hand side is non-zero in the above, and we do not have a solution of Ly(x)=0. The factor c is not cancelled for r=0,1 and r=2. This part of the second independent solution is

[cb0(c+c(c+α)(c+β)(c+1)(c2)x+c(c+α)(c+α+1)(c+β)(c+β+1)(c+1)(c+2)(c2)(c1)x2)]|c=0. =b0(1+αβ1!×(2)x+α(α+1)β(β+1)2!×(2)×(1)x2)=b0r=031(α)r(β)rr!(13)rxr.

Now we can turn our attention to the terms where the factor c cancels. First

cb3=b0(c1)(c2)c(c+α)(c+α+1)(c+α+2)(c+β)(c+β+1)(c+β+2)c(c+1)(c+2)(c+3).

After this, the recurrence relations give us

cb4=cb3(c)(c+α+3)(c+β+3)(c+1)(c+4)).

cb5=cb3(c)(c+α+3)(c+α+4)(c+β+3)(c+β+4))(c+2)(c+1)(c+5)(c+4).

So, if r3 we have

cbr=b0(c1)(c2)(c+α)r(c+β)r(c+1)r3(c+1)r.

We need the partial derivatives

cb3(c)c|c=0=b0(13)31(α)3(β)30!3![11+12+1α+1α+1+1α+2 +1β+1β+1+1β+2111213].

Similarly, we can write

cb4(c)c|c=0=b0(13)31(α)4(β)41!4![11+12 +k=0k=31α+k+k=0k=31β+k1112131411],

and

cb5(c)c|c=0=b0(13)31(α)5(β)52!5![11+12 +k=0k=41α+k+k=0k=41β+k11121314151112].

It becomes clear that for r3

cbr(c)c|c=0=b0(13)31(α)r(β)r(r3)!r![H2+k=0k=r11α+k+k=0k=r11β+kHrHr3].

Here, Hk is the kth partial sum of the harmonic series, and by definition H0=0 and H1=1.

Putting these together, for the case γ=2 we have a second solution

y2(x)=logx×b0(2)2r=3(α)r(β)rr!(r3)!xr+b0r=031(α)r(β)rr!(13)rxr

+b0(2)2r=3(α)r(β)r(r3)!r![H2+k=0k=r11α+k+k=0k=r11β+kHrHr3]xr.

The two independent solutions for γ=1m (where m is a positive integer) are then

y1(x)=1(1m)m1r=m(α)r(β)rr!(rm)!xr

and

y2(x)=logx×y1(x)+r=0m1(α)r(β)rr!(1m)rxr

+1(1m)m1r=m(α)r(β)r(rm)!r![Hm1+k=0k=r11α+k+k=0k=r11β+kHrHrm]xr.

The general solution is as usual y(x)=Ay1(x)+By2(x) where A and B are arbitrary constants. Now, if the reader consults a ``standard solution" for this case, such as given by Abramowitz and Stegun [1] in §15.5.21 (which we shall write down at the end of the next section) it shall be found that the y2 solution we have found looks somewhat different from the standard solution. In our solution for y2, the first term in the infinite series part of y2 is a term in xm. The first term in the corresponding infinite series in the standard solution is a term in xm+1. The xm term is missing from the standard solution. Nonetheless, the two solutions are entirely equivalent.

The "Standard" Form of the Solution γ ≤ 0

The reason for the apparent discrepancy between the solution given above and the standard solution in Abramowitz and Stegun [1] §15.5.21 is that there are an infinite number of ways in which to represent the two independent solutions of the hypergeometric ODE. In the last section, for instance, we replaced a0 with b0c. Suppose though, we are given some function h(c) which is continuous and finite everywhere in an arbitrarily small interval about c=0. Suppose we are also given

h(c)|c=00, and dhdc|c=00.

Then, if instead of replacing a0 with b0c we replace a0 with b0h(c)c, we still find we have a valid solution of the hypergeometric equation. Clearly, we have an infinity of possibilities for h(c). There is however a ``natural choice" for h(c). Suppose that cbN(c)=b0f(c) is the first non zero term in the first y1(x) solution with c=0. If we make h(c) the reciprocal of f(c), then we won't have a multiplicative constant involved in y1(x) as we did in the previous section. From another point of view, we get the same result if we ``insist" that aN is independent of c, and find a0(c) by using the recurrence relations backwards.

For the first (c=0) solution, the function h(c) gives us (apart from multiplicative constant) the same y1(x) as we would have obtained using h(c)=1. Suppose that using h(c)=1 gives rise to two independent solutions y1(x) and y2(x). In the following we shall denote the solutions arrived at given some h(c)1 as y~1(x) and y~2(x).

The second solution requires us to take the partial derivative w.r.t c, and substituting the usual trial solution gives us

Lcr=0ch(c)brxr+c=b0(dhdcc2(c1)+2ch(c)(c1)+h(c)c2).

The operator L is the same linear operator discussed in the previous section. That is to say, the hypergeometric ODE is represented as Ly(x)=0.

Evaluating the left hand side at c=0 will give us a second independent solution. Note that this second solution y~2 is in fact a linear combination of y1(x) and y2(x).

Any two independent linear combinations (y~1 and y~2) of y1 and y2 are independent solutions of Ly=0.

The general solution can be written as a linear combination of y~1 and y~2 just as well as linear combinations of y1 and y2.


We shall review the special case where γ=13=2 that was considered in the last section. If we ``insist" a3(c)=const., then the recurrence relations yield

a2=a3c(3+c)(2+α+c)(2+β+c), a1=a3c(2+c)(3+c)(c1)(1+α+c)(2+α+c)(1+β+c)(2+β+c),

and

a0=a3c(1+c)(2+c)(3+c)(c1)(c2)(α+c)3(β+c)3=b0ch(c).

These three coefficients are all zero at c=0 as expected. We have three terms involved in y2(x) by taking the partiial derivative w.r.t c, we denote the sum of the three terms involving these coefficients as S3 where

S3=[c(a0(c)xc+a1(c)xc+1+a2(c)xc+2)]c=0, =a3[3×2×1(2)×(1)(α)3(β)3x33+3×2×(1)(α+1)(α+2)(β+1)(β+2)x32+3(α+2)(β+2)1x31].

The reader may confirm that we can tidy this up and make it easy to generalise by putting

S3=a3r=13(3)r(r1)!(1α3)r(1β3)rx3r.

Next we can turn to the other coefficients, the recurrence relations yield

a4=a3(3+c+α)(3+c+β)(4+c)(1+c) a5=a3(4+c+α)(3+c+α)(4+c+β)(3+c+α(5+c)(4+c)(1+c)(2+c)

Setting c=0 gives us

y~1(x)=a3x3r=0(α+3)r(β+3)r(3+1)rr!xr=a3x32F1(α+3,β+3;(1+3);z).

This is (apart from the multiplicative constant(a)3(b)3/2) the same as y1(x). Now, to find y~2 we need partial derivatives

a4c|c=0=a3[(3+c+α)(3+c+β)(4+c)(1+c)(1α+3+c+1β+3+c14+c11+c)]c=0

=a3(3+α)1(3+β)1(1+3)1×1(1α+3+1β+31411).

Then

a5c|c=0=a3(3+α)2(3+β)2(1+3)2×1×2(1α+3+1α+4+1β+3+1β+414151112).

we can re-write this as

a5c|c=0=a3(3+α)2(3+β)2(1+3)2×2![k=01(1α+3+k+1β+3+k)+k=131kk=151k1112].

The pattern soon becomes clear, and for r=1,2,3,

ar+3c|c=0=a3(3+α)r(3+β)r(1+3)r×r![k=0r1(1α+3+k+1β+3+k)+k=131kk=1r+31kk=1r1k].

Clearly, for r=0,

a3c|c=0=0.

The infinite series part of y~2 is S, where

S=x3r=1ar+3c|c=0xr.

Now we can write (disregarding the arbitrary constant) forγ=1m

y~1(x)=x32F1(α+m,β+m;1+m;z)

y~2(x)=y~1(x)logxr=1m(m)r(r1)!(1αm)r(1βm)rxmr. +x3r=0(α+m)r(β+m)r(1+m)r×r![k=0r1(1α+m+k+1β+m+k)+k=131kk=1r+31kk=1r1k]xr.

Some authors prefer to express the finite sums in this last result using the digamma function ψ(x). In particular, the following results are used

Hn=ψ(n+1)+γem. Here, γem=0.5772156649=ψ(1) is the Euler-Mascheroni constant. Also

k=0n11z+k=ψ(z+n)ψ(z).

With these results we obtain the form given in Abramamowitz and Stegun §15.5.21, namely

y~2(x)=y~1(x)logxr=1m(m)r(r1)!(1αm)r(1βm)rxmr. +x3r=0(α+m)r(β+m)r(1+m)r×r![ψ(α+r+m)ψ(α+m)+ψ(β+r+m)ψ(β+m) ψ(r+1+m)ψ(r+1)+ψ(1+m)+ψ(1)]xr.

The Standard" Form of the Solution γ > 1

In this section, we shall concentrate on the ``standard solution", and we shall not replace a0 with b0(c1+γ). We shall put γ=1+m where m=1,2,3,. For the root c=1γ of the indicial equation we had

Ar=[Ar1(r+α1+c)(r+β1+c)(r+c)(r+c+γ1)]c=1γ=Ar1(r+αγ)(r+βγ)(r+1γ)(r),

where r1 in which case we are in trouble if r=γ1=m. For instance, if γ=4, the denominator in the recurrence relations vanishes for r=3. We can use exactly the same methods that we have just used for the standard solution in the last section. We shall not (in the instance where γ=4) replace a0 with b0(c+3) as this will not give us the standard form of solution that we are after. Rather, we shall ``insist" that A3=const. as we did in the standard solution for γ=2 in the last section. (Recall that this defined the function h(c) and that a0 will now be replaced with b0(c+3)h(c).) Then we may work out the coefficients of x0 to x2 as functions of c using the recurrence relations backwards. There is nothing new to add here, and the reader may use the same methods as used in the last section to find the results of [1]§15.5.18 and §15.5.19, these are

y1=2F1(α,β;1+m;x),

and

y2=2F1(α,β;1+m;x)logx+zmr=1(α)r(β)rr!(1+m)r[ψ(α+r)ψ(α)+ψ(β+k)ψ(β) ψ(m+1+r)+ψ(m+1)ψ(r+1)+ψ(1)]zrk=1m(k1)!(m)k(1α)k(1β)kzr.

Note that the powers of z in the finite sum part of y2(x) are now negative so that this sum diverges as z0$

Solution around x = 1

Let us now study the singular point x = 1. To see if it is regular,

limxa(xa)P1(x)P2(x)=limx1(x1)(γ(1+α+β)x)x(1x)=limx1(γ(1+α+β)x)x=1+α+βγlimxa(xa)2P0(x)P2(x)=limx1(x1)2(αβ)x(1x)=limx1(x1)αβx=0

Hence, both limits exist and x = 1 is a regular singular point. Now, instead of assuming a solution on the form

y=r=0ar(x1)r+c,

we will try to express the solutions of this case in terms of the solutions for the point x = 0. We proceed as follows: we had the hypergeometric equation

x(1x)y+(γ(1+α+β)x)yαβy=0.

Let z = 1 − x. Then

dydx=dydz×dzdx=dydz=yd2ydx2=ddx(dydx)=ddx(dydz)=ddz(dydz)×dzdx=d2ydz2=y

Hence, the equation takes the form

z(1z)y+(α+βγ+1(1+α+β)z)yαβy=0.

Since z = 1 − x, the solution of the hypergeometric equation at x = 1 is the same as the solution for this equation at z = 0. But the solution at z = 0 is identical to the solution we obtained for the point x = 0, if we replace each γ by α + β − γ + 1. Hence, to get the solutions, we just make this substitution in the previous results. For x = 0, c1 = 0 and c2 = 1 − γ. Hence, in our case, c1 = 0 while c2 = γ − α − β. Let us now write the solutions. In the following we replaced each z by 1 - x.

Analysis of the solution in terms of the difference γ − α − β of the two roots

To simplify notation from now on denote γ − α − β by Δ, therefore γ = Δ + α + β.

Δ not an integer

y=A{2F1(α,β;Δ+1;1x)}+B{(1x)Δ2F1(Δ+β,Δ+α;Δ+1;1x)}

Δ = 0

y=C{2F1(α,β;1;1x)}+D{r=0(α)r(β)r(1)r2(ln(1x)+k=0r1(1α+k+1β+k21+k))(1x)r}

Δ is a non-zero integer

Δ > 0

y=E{1(Δ+1)Δ1 r=1Δαβ(α)r(β)r(1)r(1)rΔ(1x)r}++F{(1x)Δ r=0(Δ)(Δ+α)r(Δ+β)r(Δ+1)r(1)r(ln(1x)+1Δ+k=0r1(1Δ+α+k+1Δ+β+k1Δ+1+k11+k))(1x)r}

Δ < 0

y=G{(1x)Δ(Δ+1)Δ1 r=Δ(Δ+α)r(Δ+β)r(1)r(1)r+Δ(1x)r}++H{r=0(Δ)(Δ+α)r(Δ+β)r(Δ+1)r(1)r(ln(1x)1Δ+k=0r1(1α+k+1β+k1Δ+1+k11+k))(1x)r}

Solution around infinity

Finally, we study the singularity as x → ∞. Since we can't study this directly, we let x = s−1. Then the solution of the equation as x → ∞ is identical to the solution of the modified equation when s = 0. We had

x(1x)y+(γ(1+α+β)x)yαβy=0dydx=dyds×dsdx=s2×dyds=s2yd2ydx2=ddx(dydx)=ddx(s2×dyds)=dds(s2×dyds)×dsdx=((2s)×dyds+(s2)d2yds2)×(s2)=2s3y+s4y

Hence, the equation takes the new form

1s(11s)(2s3y+s4y)+(γ(1+α+β)1s)(s2y)αβy=0

which reduces to

(s3s2)y+((2γ)s2+(α+β1)s)yαβy=0.

Let

P0(s)=αβ,P1(s)=(2γ)s2+(α+β1)s,P2(s)=s3s2.

As we said, we shall only study the solution when s = 0. As we can see, this is a singular point since P2(0) = 0. To see if it is regular,

limsa(sa)P1(s)P2(s)=lims0(s0)((2γ)s2+(α+β1)s)s3s2=lims0(2γ)s2+(α+β1)ss2s=lims0(2γ)s+(α+β1)s1=1αβ.limsa(sa)2P0(s)P2(s)=lims0(s0)2(αβ)s3s2=lims0(αβ)s1=αβ.

Hence, both limits exist and s = 0 is a regular singular point. Therefore, we assume the solution takes the form

y=r=0arsr+c

with a0 ≠ 0. Hence,

y=r=0ar(r+c)sr+c1y=r=0ar(r+c)(r+c1)sr+c2

Substituting in the modified hypergeometric equation we get

(s3s2)y+((2γ)s2+(α+β1)s)y(αβ)y=0

And therefore:

(s3s2)r=0ar(r+c)(r+c1)sr+c2+((2γ)s2+(α+β1)s)r=0ar(r+c)sr+c1(αβ)r=0arsr+c=0

i.e.,

r=0ar(r+c)(r+c1)sr+c+1r=0ar(r+c)(r+c1)xr+c+(2γ)r=0ar(r+c)sr+c+1+(α+β1)r=0ar(r+c)sr+cαβr=0arsr+c=0.

In order to simplify this equation, we need all powers to be the same, equal to r + c, the smallest power. Hence, we switch the indices as follows

r=1ar1(r+c1)(r+c2)sr+cr=0ar(r+c)(r+c1)sr+c+(2γ)r=1ar1(r+c1)sr+c++(α+β1)r=0ar(r+c)sr+cαβr=0arsr+c=0

Thus, isolating the first term of the sums starting from 0 we get

a0((c)(c1)+(α+β1)(c)αβ)sc+r=1ar1(r+c1)(r+c2)sr+cr=1ar(r+c)(r+c1)xr+c++(2γ)r=1ar1(r+c1)sr+c+(α+β1)r=1ar(r+c)sr+cαβr=1arsr+c=0

Now, from the linear independence of all powers of s (i.e., of the functions 1, s, s2, ...), the coefficients of sk vanish for all k. Hence, from the first term we have

a0((c)(c1)+(α+β1)(c)αβ)=0

which is the indicial equation. Since a0 ≠ 0, we have

(c)(c+1+α+β1)αβ)=0.

Hence, c1 = α and c2 = β.

Also, from the rest of the terms we have

((r+c1)(r+c2)+(2γ)(r+c1))ar1+((r+c)(r+c1)+(α+β1)(r+c)αβ)ar=0

Hence,

ar=((r+c1)(r+c2)+(2γ)(r+c1))((r+c)(r+c1)+(α+β1)(r+c)αβ)ar1=((r+c1)(r+cγ))((r+c)(r+cαβ)+αβ)ar1

But

(r+c)(r+cαβ)+αβ=(r+cα)(r+c)β(r+c)+αβ=(r+cα)(r+c)β(r+cα).

Hence, we get the recurrence relation

ar=(r+c1)(r+cγ)(r+cα)(r+cβ)ar1,r1

Let's now simplify this relation by giving ar in terms of a0 instead of ar−1. From the recurrence relation,

a1=(c)(c+1γ)(c+1α)(c+1β)a0a2=(c+1)(c+2γ)(c+2α)(c+2β)a1=(c+1)(c)(c+2γ)(c+1γ)(c+2α)(c+1α)(c+2β)(c+1β)a0=(c)2(c+1γ)2(c+1α)2(c+1β)2a0

As we can see,

ar=(c)r(c+1γ)r(c+1α)r(c+1β)ra0r0

Hence, our assumed solution takes the form

y=a0r=0(c)r(c+1γ)r(c+1α)r(c+1β)rsr+c

We are now ready to study the solutions corresponding to the different cases for c1 − c2 = α − β.

Analysis of the solution in terms of the difference α − β of the two roots

α − β not an integer

Then y1 = y|c = α and y2 = y|c = β. Since

y=a0r=0(c)r(c+1γ)r(c+1α)r(c+1β)rsr+c,

we have

y1=a0r=0(α)r(α+1γ)r(1)r(α+1β)rsr+α=a0sα 2F1(α,α+1γ;α+1β;s)y2=a0r=0(β)r(β+1γ)r(β+1α)r(1)rsr+β=a0sβ 2F1(β,β+1γ;β+1α;s)

Hence, y = Ay1 + By2. Let Aa0 = A and Ba0 = B. Then, noting that s = x−1,

y=A{xα 2F1(α,α+1γ;α+1β;x1)}+B{xβ 2F1(β,β+1γ;β+1α;x1)}

α − β = 0

Then y1 = y|c = α. Since α = β, we have

y=a0r=0(c)r(c+1γ)r((c+1α)r)2sr+c

Hence,

y1=a0r=0(α)r(α+1γ)r(1)r(1)rsr+α=a0sα 2F1(α,α+1γ;1;s)y2=yc|c=α

To calculate this derivative, let

Mr=(c)r(c+1γ)r((c+1α)r)2

Then using the method in the case γ = 1 above, we get

Mrc=(c)r(c+1γ)r((c+1α)r)2k=0r1(1c+k+1c+1γ+k2c+1α+k)

Now,

y=a0scr=0(c)r(c+1γ)r((c+1α)r)2sr=a0scr=0Mrsr=a0sc(ln(s)r=0(c)r(c+1γ)r((c+1α)r)2sr+r=0(c)r(c+1γ)r((c+1α)r)2{k=0r1(1c+k+1c+1γ+k2c+1α+k)}sr)

Hence,

yc=a0scr=0(c)r(c+1γ)r((c+1α)r)2(ln(s)+k=0r1(1c+k+1c+1γ+k2c+1α+k))sr

Therefore:

y2=yc|c=α=a0sαr=0(α)r(α+1γ)r(1)r(1)r(ln(s)+k=0r1(1α+k+1α+1γ+k21+k))sr

Hence, y = C′y1 + D′y2. Let C′a0 = C and D′a0 = D. Noting that s = x−1,

y=C{xα2F1(α,α+1γ;1;x1)}+D{xαr=0(α)r(α+1γ)r(1)r(1)r(ln(x1)+k=0r1(1α+k+1α+1γ+k21+k))xr}

α − β an integer and α − β ≠ 0

α − β > 0

From the recurrence relation

ar=(r+c1)(r+cγ)(r+cα)(r+cβ)ar1

we see that when c = β (the smaller root), aα−β → ∞. Hence, we must make the substitution a0 = b0(cci), where ci is the root for which our solution is infinite. Hence, we take a0 = b0(c − β) and our assumed solution takes the new form

yb=b0r=0(cβ)(c)r(c+1γ)r(c+1α)r(c+1β)rsr+c

Then y1 = yb|c = β. As we can see, all terms before

(cβ)(c)αβ(c+1γ)αβ(c+1α)αβ(c+1β)αβsαβ

vanish because of the c − β in the numerator.

But starting from this term, the c − β in the numerator vanishes. To see this, note that

(c+1α)αβ=(c+1α)(c+2α)(cβ).

Hence, our solution takes the form

y1=b0((β)αβ(β+1γ)αβ(β+1α)αβ1(1)αβsαβ+(β)αβ+1(β+1γ)αβ+1(β+1α)αβ1(1)(1)αβ+1sαβ+1+)=b0(β+1α)αβ1r=αβ(β)r(β+1γ)r(1)r(1)r+βαsr

Now,

y2=ybc|c=α.

To calculate this derivative, let

Mr=(cβ)(c)r(c+1γ)r(c+1α)r(c+1β)r.

Then using the method in the case γ = 1 above we get

Mrc=(cβ)(c)r(c+1γ)r(c+1α)r(c+1β)r(1cβ+k=0r1(1c+k+1c+1γ+k1c+1α+k1c+1β+k))

Now,

yb=b0r=0((cβ)(c)r(c+1γ)r(c+1α)r(c+1β)rsr+c)=b0scr=0Mrsr

Hence,

yc=b0scln(s)r=0(cβ)(c)r(c+1γ)r(c+1α)r(c+1β)rsr+b0scr=0(cβ)(c)r(c+1γ)r(c+1α)r(c+1β)r(1cβ+k=0r1(1c+k+1c+1γ+k1c+1α+k1c+1β+k))sr

Hence,

yc=b0scr=0(cβ)(c)r(c+1γ)r(c+1α)r(c+1β)r(ln(s)+1cβ+k=0r1(1c+k+1c+1γ+k1c+1α+k1c+1β+k))sr

At c = α we get y2. Hence, y = Ey1 + Fy2. Let Eb0 = E and Fb0 = F. Noting that s = x−1 we get

y=E{1(β+1α)αβ1r=αβ(β)r(β+1γ)r(1)r(1)r+βαxr}++F{xαr=0(αβ)(α)r(α+1γ)r(1)r(α+1β)r(ln(x1)+1αβ+k=0r1(1α+k+1α+1+kγ11+k1α+1+kβ))xr}

α − β < 0

From the symmetry of the situation here, we see that

y=G{1(α+1β)βα1r=βα(α)r(α+1γ)r(1)r(1)r+αβxr}++H{xβr=0(βα)(β)r(β+1γ)r(1)r(β+1α)r(ln(x1)+1βα+k=0r1(1β+k+1β+1+kγ11+k1β+1+kα))xr}

References

  1. 1.0 1.1 1.2 Abramowitz and Stegun
  • Ian Sneddon (1966). Special functions of mathematical physics and chemistry. OLIVER B. ISBN 978-0-05-001334-2. 

Abramowitz, Milton; Stegun, Irene A. (1964). Handbook of Mathematical Functions. New York: Dover. ISBN 978-0-48-661272-0. https://archive.org/details/handbookofmathe000abra.