I am learning the Debye Model and am having trouble understanding how to interpret it within the framework of statistical mechanics.
I understand that in the Einstein model, we consider a solid as our system, and then consider one atom in that solid as a closed subsystem, i.e. energy can pass between that atom and the rest of the lattice. We can then treat this setup using the canonical ensemble. Letting the atom be a quantum SHO which is independent of any other atom in the lattice and has a fixed frequency parameter $\omega$, we see that its microstates are just the quantized excitations of the oscillator, and from there we can find the partition function and all of the other fun quantities such as $\langle E\rangle$, $C_v$, etc.
In the Debye model, we make some fundamental changes to the model: atoms are now coupled and so we can no longer consider just one atom as its own independent subsystem, so the previous approach using the canonical ensemble will not work. However, we can turn to the grand canonical ensemble and one of its main results, which is that if we treat an actual state of a system as an open subsystem, we can find a distribution function associated with it which depends on the type of particles which can occupy it (leading to the Bose-Einstein, Planck, Fermi-Dirac, and Boltzmann distributions). This is where my confusion starts. From what I've read online:
- oscillations in the lattice are carried by the displacement of atoms from their equilibrium position, and there are three possible modes of displacement: 1 longitudinal and 2 transverse
- oscillations in the lattice must adhere to the boundary condition of being periodic, which introduces a quantization of the wavenumber $k_n$ of the allowed oscillations
- because we care about macroscopic bulk quantities (e.g. heat capacity), the boundary shape of our model shouldn't actually matter, so we can choose to make our solid a perfect cube with sidelength L
- each oscillation with a unique wavenumber can be considered a state (why?) which is occupied by 'bosons' (why?) so we can apply our distribution results to each one to see that it has an average of $n_B(E)$ bosons occupying it
- I suspect this last answer has to do with the fact that increasing the level of a harmonic oscillator is somehow "the same as" (why?) populating it with another boson with the energy identical to the oscillator's energy spacing $\Delta E = \hbar \omega$: is this only an interpretational thing or does this manifest in a physical way?
- we now consider the regime where the dispersion relation is roughly linear...my understanding is that the dispersion relation can be derived analytically from considering the mechanical equations of motion of the atoms in the solid, but my wave theory is really shoddy so I'm taking it as given for now that $\omega = v_s |\vec{k}|$
- we can find the density of states in quantization space, $g(n)$, and then do a transformation to get the density of states in k space ($g(n)dn = g(k)dk$) or energy space as needed
- the allowed wavenumber quantization is limited by an upper bound: because the lattice is discrete, the wave is a sinusoid which is sampled at discrete positions (the position of each atom), and if the wavelength is too small, aliasing will occur and the wave will be nonphysical
To summarize, my questions are:
- Why can each oscillation with a unique wavenumber be considered a state?
- Why can this state be "occupied" by some type of boson?
- How we know that the "normal modes" of the lattice are all of the states that need to be considered?
- Do these answers follow somehow from the Hamiltonian of the system? This question sort of touches on this.