Quantum Mechanics, Volume 3. Claude Cohen-Tannoudji
This expression does look like the stationarity condition at constant energy (77), but now the subscripts l and m are the same, and a term in
3. Temperature dependent mean field equations
Introducing a Hartree-Fock operator acting in the single particle state space allows writing the stationarity relations just obtained in a more concise and manageable form, as we now show.
3-a. Form of the equations
Let us define a temperature dependent Hartree-Fock operator as the partial trace that appears in the previous equations:
It is thus an operator acting on the single particle 1. It can be defined just as well by its matrix elements between the individual states:
Equation (77) is valid for any two chosen values l and m, as long as
is orthogonal to all the eigenvectors |θm〉 having an eigenvalue
(i) If
(ii) If this eigenvalue of
We now reason in this new basis where all the [K0 + V1 + WHF(β)]|φn〉 are proportional to |φn〉. Taking (83) into account, we get:
As we just saw, the basis change from the |θl〉 to the |φn〉 only occurs within the eigen-subspaces of
Inserting this relation in the definition (84) of WHF(β) leads to a set of equations only involving the eigenvectors |φn〉.
For all the values of n we get a set of equations (87), which, associated with (84) and (88) defining the potential WHF(β) as a function of the |φn〉, are called the temperature dependent Hartree-Fock equations.
3-b. Properties and limits of the equations
We now discuss how to apply the mean field equations we have obtained, and their limit of validity, which are more stringent for bosons than for fermions.
α. Using the equations
Hartree-Fock equations concern a self-consistent and nonlinear system: the eigenvectors |φn〉 and eigenvalues of the density operator