3
$\begingroup$

I'm going through "Advanced Quantum Mechanics" by Franz Schwabl, and he calculates the electron energy levels from the Coulomb interaction in a perturbative way (section 2.2.3). In the course of this, he calculates that: $$ \left< a^\dagger_{k + q, \sigma} (t) \: a_{k + q, \sigma} (t) \right> = \left< \phi_0 \right| a^\dagger_{k + q, \sigma} (t) \: a_{k + q, \sigma} (t) \left| \phi_0 \right> = n_{k + q, \sigma} $$ (eq. 2.2.18 to 2.2.19), where $\left| \phi_0 \right>$ is the filled Fermi sphere state, and $n_{k + q, \sigma}$ is 1 if $k + q < k_F$ (the Fermi momentum) and zero otherwise.

Why does this last equality hold? This is clearly true for $t = 0$ by how the creation and annihilation operators are defined, but it seems like this should be a time-dependent quantity if we are considering time-dependent creation and annihilation operators. That is, we should have to explicitly time-evolve these operators with the exponential of the Hamiltonian (given below) to calculate the expectation value. He seems to just do it without thinking. What am I missing?

The Hamiltonian (in case it is relevant) is just the Coulomb interaction Hamiltonian: $$ H = \sum_{\mathbf{k}, \sigma} \frac{\hbar^2 k^2}{2m} a^\dagger_{\mathbf{k} \,\sigma} a_{\mathbf{k} \, \sigma} + \frac{1}{2V} \sum_{\mathbf{q} \neq 0, \mathbf{p}, \mathbf{k}' \\ \sigma, \sigma'} \frac{4 \pi e^2}{q^2} a^\dagger_{\mathbf{p} + \mathbf{q} \, \sigma} a^\dagger_{\mathbf{k'} - \mathbf{q} \,\sigma} a_{\mathbf{k'} \, \sigma'} a_{\mathbf{p} \, \sigma} $$

$\endgroup$

1 Answer 1

2
$\begingroup$

I think he is implicitly assuming that the filled Fermi sea $\vert{\phi_0}\rangle$ is a good approximation for the ground state of the weakly interacting Hamiltonian. Therefore he is assuming that under time evolution, this state only picks up a phase.

In terms of Green's functions in terms of Feynman diagrams, we can say that he is approximating the interacting Green's function as the free Green's function $+$ the Fock Green's function. The Hartree term is zero because there is no interaction when $q=0$. (Ignore this paragraph if you do not know diagrammatic perturbation theory.)

In terms of usual perturbation theory, he is just finding the first-order correction to the ground state energy, which is given by $$ \Delta E = \langle \phi_0 \vert H_{\text{Coulomb}}\vert \phi_0\rangle $$ You can verify that this matches the correction to the energy he obtained. So we can say he is essentially doing first-order perturbation theory.

$\endgroup$

Your Answer

By clicking “Post Your Answer”, you agree to our terms of service and acknowledge you have read our privacy policy.

Not the answer you're looking for? Browse other questions tagged or ask your own question.