RUTA said:
The discussion about how one should best introduce QM is interesting. With applications to nuclear physics, solid state physics, quantum optics, quantum information/computing, particle physics, and foundations to name a few, one could start almost anywhere. There are three of us teaching intro courses in these areas for engineers at my small undergrad institution and there is very little overlap in content between the courses, even though all the courses analyze actual experiments and/or applications.
The problem is to get the radically new physical thinking as compared to classical physics which (apparently) is straight-forward from the very first moment. I don't think that just to put the "trace formula" for expectation values on top of a axiomatic is good for the introductory course lecture. It's very good for a treatment in an advanced lecture on quantum foundations, quantum information, or something similar.
The criticism about my "photon-polarization first" approach is also well justified. I made this choice, because the lecture about electrodynamics, which is part of my course on theoretical physics for high-school teachers, ends with a quite complete treatment of electromagnetic waves, including a discussion of plane-wave solutions, polarization and also of course diffraction on slits and gratings.
Then my idea was that it is best to start with the most simple case of a 2D quantum-mechanical Hilbert space, as is done in many textbooks I like using spin 1/2 and the Stern-Gerlach experiment. This is however in my opinion also not so good for an introductory QM lecture, i.e., one where the students never have heard about spin before, i.e., and that's why I start rather with the polarization of electromagnetic waves and then argue heuristically (and I don't think that you can introduce QM at this level in any sensible way purely deductively without a big portion of heuristics) what happens if you use single-photon sources (without of course being able to explain the subtle and in fact important difference between "dimmed laser light" and real one-photon Fock states). I see the advantage in the fact that you have all the material of electromagnetism lecture at hand, particularly the fact that the most intuitive observable of light, which is intensity (i.e., "brightness" as a qualitative entity), is an adequate (temporal) average over the energy density of the electromagnetic field, i.e., for a plane wave something ##\proportional |\vec{E}^2|##.
Then you have with the most simple example of using polaroid foil(s) doing experiments with polarized light (which is nowadays really no problem to do even in the introductory expermental-physics lecture, since one has lasers at hand to produce nicely coherent light; even with "natural light" it's no big deal to get polarized light using a polaroid filter) all the arguments at hand to motivate the QT formalism:
-polarization states as preparation procedure: Just take a polaroid to provide a source of linearly polarized light in a given direction
-self-adjoint operators as representants of polarization states: Just use another polaroid and describe it as projection operarator
-the superposition principle and complete orthonormal systems: You work within a framework of linear optics, where the em. field equations are linear equations, and you can find new solutions by superposition and even all solutions in terms of complete sets of orthonormal function systems (a concept also known from the E&M lecture, where this is treated in the context of Fourier series and Fourier integrals).
Of course there are also some drawbacks of this method, because it introduces photons at the introductory stage, and there's some danger that the students get the wrong idea as if one could treat photons in a kind of 1st-quantization approach, which of course then follows directly after the introduction with photon polarization, where the Hilbert space for one particle is introduced in the usual heuristics a la Schrödinger (in a very simplified form, not taking recourse to the Hamilton-Jacobi theory of classical mechanics).