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First we re-emphasized the difference between bound states and scattering states. From Griffiths we know that we can define bound states as those where the energy is less than zero. Scattering states are those where the energy is greater than zero. To illustrate the difference between bound state and scattering states we examined a few examples with which we are familiar. For each example we determined whether bound states, scattering states, or both are possible. Those examples and their possible states are:
Infinite Square Well – Bound States
Simple Harmonic Oscillator – Bound States
Negative Delta Function – Both
Positive Delta Function – Scattering States
Finite Square Well – Both
Free Paticle – Scattering States
E = 0 – To be honest, I didn't understand this part of the lecture very well.
Next we reviewed what we have covered from chapter 3 so far. Here are the main points we have covered thus far:
– Quantum mechanical operators are Hermitian operators. The eigenvalues of those Hermitian operators are real.
– Determinate states are eigenfunctions of Hermitian operators.
Next we listed the major topics from chapter 3 that we will cover in the next lecture or so.
– The generalized statistical interpretation of quantum mechanics.
– The uncertainty principle
– Momentum space
Finally, a question was raised concerning notation used in section 3.4 of Griffiths. The question related to equation 3.43 on page 106. What is the difference between fn and Psi? It should be noted that equation 3.43 is Fourier's trick in bracket notation. Fn is any function that is any stationary state wave function. You could also think of fn as the initial state of a wave function. Psi is the time-dependent wave function of the system.
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