The solutions of the differential equations of physics are analytic functions, and every analytic function has a Taylor Series, so the most straightforward way to seek solutions to differential equations is to attempt to find the power series. Power series is not so strange a way to define a function; after all cos and sin are algebraically defined in exactly that way. Hence we could approach our present problem of finding the solutions of Hy = Ey where
H=p2/(2m) + (1/2)mw2x2
or
-[hbar2/(2m)]d2y/dx2 +(1/2)mw2x2y = Ey
y(x) = Sn bn xn .
We would quickly drown in algebra. There are a couple of standard life preservers. First, get rid of a few constants, so that the algebra is as compact as possible, by defining
x = Ö(mw / hbar) x (7-0a)
K = 2 E / (hbar w) (7-0b)
in terms of which
d2y/dx2 = (x2 - K) y (7-1)
Second, find out how y behaves at large x [or x] and hope that this asymptotic behavior determines the most complicated part of the power series. At large x,
d2y/dx2 = x2 y . We can easily guess the solution of this equation (compare y0 from the last section):
y(x) = A e - x2/2 + B e + x2/2 The second of these is not normalizable and cannot be used, so we take B=0 so that, at large x at least,
y = A e - x2/2
The ghost of the second term will return to haunt us in a moment. We don't have the full solution, of course, since the differential equation was exact only for large x. However, we can use this result to suggest parametrizing the exact solution as
y(x) = h(x) e - x2/2 (7-2)
If y has a power series, then so does h. However, h is hopefully simpler than y, since its asymptotic behavior must not upset the known asymptotic behaviour of y. It turns out to be a lot simpler.
Now we apply the power-series idea, by seeking a solution h(x) in power-series form,
h(x) =Sn an xn (7-3)
(d2h/dx2) e - x2/2 - 2 x (dh/dx) e - x2/2 + h (x2 -1) e - x2/2 = (x2 - K) h e - x2/2
(d2h/dx2) - 2 x (dh/dx) + (K -1)h = 0
Now the power series:
Sn=0 ¥ an [n(n-1)xn-2 -2n xn +(K-1)xn] = 0
In the first term, let q=n-2, and let q=n in the other terms. Then all
the powers of x will be the same, except that
there will be terms for x-1, -2:
Sq=0
¥ {
aq+2[(q+2)(q+1)xq]
+aq[ -2q xq
+(K-1)xq]}
+ a-2[(0)(-1)x-2]
+ a-1[(1)(0)x-1]}
= 0
and the two extra terms have zero coefficients so that they don't mess up the algebra. The only way that this equation can vanish for all x is for each coefficient to vanish separately:
aq+2
= aq [2q+1-K]/[(q+1)(q+2)] (7-4) h(x) =Sq aq xq |
Hence we have a recursion relation. Given a0 we know all the even aq, and given a1 we know all the odd aq. In other words, we have two solutions for h, each multiplied by an arbitrary constant [a0 and a1]. However, for any given E [K] we should be able to discard one solution as not being normalizable, since that is what happened with y when we were exploring the asymptotic behavior of the wave function. Therefore one or the other solution for h must be too large at ¥ to normalize. How can we check for this? Try looking at the recursion relation when x is large. The behavior will be dominated by the terms with large q [at least if there are terms with large q], so we have approximately
aq+2 = aq[2q/q2]
= (2/q) aq
Hence
aq = a0(2/2)(2/4)(2/6)...(2/q)
= a0/[1*2*3*...*(q/2)]
aq = a0/(q/2)!
or
aq = a1(2/3)(2/5)(2/7)...(2/q)
> a1(2/4)(2/6)(2/8)...2/(q+1)
= a0/[2*3*...*(q+1)/2]
aq-1 > a1/(q/2)!
Therefore h(x) is -- or is greater than --
h(x) = Sq=0, 2, 4, ... Cxq /(q/2)!
= Sq=0, 1, 2, ... C(x2)q /q!
= exp( x2 )
which implies that
y(x) ³ exp( x2/2 ) for large x
and is therefore not normalizable. We cannot allow the series to reach large values of q. Therefore there must be some value of q, which we can call n, for which
an+2 = 0.
In this case, the asymptotic behavior of y is xn exp[-x2/2] which is normalizable. Examining 7-4, an+2 can vanish only if
2n+1-K=0,
K = 2n+1
implying that [see 7-0b]
E = (n + 1/2) hbar w (7-5)
which we had previously obtained by algebraic methods.
Note the following:
Show a few examples of yn superimposed on the potential and the value of the total energy.
Last Revised 02/09/23 |