00:01
All right, so we have a quantum harmonic oscillator with the addition of an external electric field.
00:09
And so our hamiltonian looks like this, p squared over 2m plus 1 1⁄2m of omega squared x squared.
00:19
So that's the normal quantum harmonic oscillator part.
00:21
And then we have minus qe times x.
00:27
And so we want to know what the new eigenfunction.
00:31
And eigenvalues of this hamiltonian are.
00:33
So there's actually a trick.
00:35
You may be familiar with it.
00:37
But if i complete the square of this term, i don't know why this happens.
00:42
If i complete the square of this term, i can actually write this single term as a square, and then we'll have a constant term outside of this.
00:51
So to show you what i mean, this can be rewritten as p squared over 2m, so that part doesn't change, plus 1⁄2m.
01:01
Omega squared times x minus q e over m omega squared squared and then we'll have a constant term which is minus q squared e squared over two m omega squared so i believe i have all that written down in my notes yeah so if we do that if you complete this square you'll notice that you know all the terms cancel out.
01:33
The reason this is useful is now we can define a new variable.
01:37
Just call it u, which is equal to x minus qe over m omega squared.
01:47
And the hamiltonian in terms of this variable u, well, the p squared over 2m part will actually look the same because we're just shifting x by a constant.
01:55
And so we can take derivatives with respect to you the same way we do with respect to x.
02:00
So the p squared over 2m, the kinetic turn doesn't change, and this becomes plus 1 half m omega squared, u squared, and then we have this constant term, minus q squared, e squared over 2m omega squared.
02:16
So this is just the hamiltonian of our ordinary harmonic oscillator that we already know, plus a constant term, which is not actually going to change the eigen functions.
02:27
So the eigen functions are going to be exactly the same as the standard.
02:31
Standard ones just with this one substitution.
02:34
So everywhere you see an x in your previous eigenfunction, you just replace it with x minus qe over m omega squared.
02:41
So for instance, psi of n in terms of x is going to be like one over, you know, we have all these coefficients and normalization terms...