- #1
kmm
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On page 160 in Shankar, he discusses how we get quantized energy levels of bound states - specifically for the particle in a box. We have three regions in space; region I from ## \ - \infty, -L/2 ##, region II from ## \ -L/2, L/2 ##, and region III from ## \ L/2, \infty ##. For the wavefunction in region I and II, we choose the coefficient of the rising exponential to be zero to get an admissible solution, leaving one free parameter for the falling exponentials in each region. In region II, the wavefunction is a sum with a sine and cosine, with a coefficient for each. This gives a total of four free parameters. Now, at each interface between the three regions at ## \ \pm L\2 ##, for a finite potential V, we require continuity of the wave function and its derivative. Thus, we impose four constraints on the wave function.
What confuses me is that Shankar goes on to say "Thus we impose four conditions on ## \psi ## which has only three free parameters. (It may seem that there are four-the coefficients of the two falling exponentials, the sine, and the cosine. However, the overall scale of ## \psi ## is irrelevant both in the eigenvalue equation and the continuity conditions, these being linear in ## \psi ## and ## \psi ' ##. Thus if say, ## \psi ' ## does not satisfy the continuity condition at ## \ x=L/2 ##, an overall rescaling of ## \psi ## and ## \psi ' ## will not help.)
It makes sense to me that overall scale doesn't matter in the eigenvalue equation and the continuity conditions, but I don't see how that takes us from apparently four free parameters to three free parameters. That there is one more constraint than there are free parameters is apparently important, because after this Shankar considers a general potential V(x) that binds a particle of energy E, where he slices space into many intervals, and after counting up the total parameters claims that we have one more constraint than we have parameters.
I also don't understand the full significance of having more constraints than free parameters. I don't see what the issue would be if we had more free parameters than constraints.
I appreciate any help!
What confuses me is that Shankar goes on to say "Thus we impose four conditions on ## \psi ## which has only three free parameters. (It may seem that there are four-the coefficients of the two falling exponentials, the sine, and the cosine. However, the overall scale of ## \psi ## is irrelevant both in the eigenvalue equation and the continuity conditions, these being linear in ## \psi ## and ## \psi ' ##. Thus if say, ## \psi ' ## does not satisfy the continuity condition at ## \ x=L/2 ##, an overall rescaling of ## \psi ## and ## \psi ' ## will not help.)
It makes sense to me that overall scale doesn't matter in the eigenvalue equation and the continuity conditions, but I don't see how that takes us from apparently four free parameters to three free parameters. That there is one more constraint than there are free parameters is apparently important, because after this Shankar considers a general potential V(x) that binds a particle of energy E, where he slices space into many intervals, and after counting up the total parameters claims that we have one more constraint than we have parameters.
I also don't understand the full significance of having more constraints than free parameters. I don't see what the issue would be if we had more free parameters than constraints.
I appreciate any help!