0
$\begingroup$

For a Hubbard hamiltonian, $$\hat{H} = \sum_{i,j,\sigma} t_{i j} \hat{c}^\dagger_{i \sigma} \hat{c}_{j \sigma} + \sum_i U_i \hat{n}_{i \uparrow} \hat{n}_{i \downarrow}, $$ the mean-field solution can be obtained by using: $ \hat{n}_{i \uparrow} \hat{n}_{i \downarrow} \approx n_{i \uparrow} \hat{n}_{i \downarrow} + n_{i \downarrow} \hat{n}_{i \uparrow} - n_{i \uparrow} n_{i \downarrow} $ and solving self-consistenly the resulting one-electron hamiltonian. In general, for a generic many-body term $\hat{c}^\dagger_{i \sigma}\hat{c}^\dagger_{j \sigma^\prime}\hat{c}_{k \sigma^\prime}\hat{c}_{l \sigma},$ the approximation is: $$\hat{c}^\dagger_{i \sigma}\hat{c}^\dagger_{j \sigma^\prime}\hat{c}_{k \sigma^\prime}\hat{c}_{l \sigma} \approx \langle \hat{c}^\dagger_{i \sigma} \hat{c}_{l \sigma} \rangle \hat{c}^\dagger_{j \sigma^\prime}\hat{c}_{k \sigma^\prime} + \langle \hat{c}^\dagger_{j \sigma^\prime}\hat{c}_{k \sigma^\prime} \rangle \hat{c}^\dagger_{i \sigma} \hat{c}_{l \sigma} - \langle \hat{c}^\dagger_{j \sigma^\prime}\hat{c}_{k \sigma^\prime} \rangle \langle \hat{c}^\dagger_{i \sigma} \hat{c}_{l \sigma} \rangle \\ -\langle \hat{c}^\dagger_{i \sigma} \hat{c}_{k \sigma^\prime} \rangle \hat{c}^\dagger_{j \sigma^\prime}\hat{c}_{l \sigma} - \langle \hat{c}^\dagger_{j \sigma^\prime} \hat{c}_{l \sigma}\rangle \hat{c}^\dagger_{i \sigma}\hat{c}_{k \sigma^\prime} + \langle \hat{c}^\dagger_{j \sigma^\prime} \hat{c}_{l \sigma} \rangle \langle \hat{c}^\dagger_{i \sigma}\hat{c}_{k \sigma^\prime} \rangle $$

(we assume the particle number is conserved, so that terms like $\langle \hat{c}^\dagger \hat{c}^\dagger \rangle $ are not important). Now, $S_z$ also being a good quantum number, if $\sigma \neq \sigma^\prime$ we will also ignore the terms on the second line, as done for the approximation above for Hubbard model. The Hubbard model on a lattice can be solved easily on mean-field thanks to the fact that on the self-consistency loop we only need the charges, and never non-diagonal charges (other elements of the density matrix) like $\langle \hat{c}^\dagger_{j \sigma^\prime} \hat{c}_{l \sigma} \rangle$.

However think now of a slightly more complicated model on a lattice. It's like the hamiltonian $\hat{H}$ above but now we add many-body interactions between neighboring sites; something like: $$ \dfrac{1}{2}\sum_{i,j, \sigma,\sigma^\prime} J_{ij} \hat{n}_{i \sigma} \hat{n}_{j \sigma^\prime}.$$ Now, for the terms with $\sigma \neq \sigma^\prime$ we have the simple approximation $\hat{n}_{i \uparrow} \hat{n}_{j \downarrow} \approx n_{i \uparrow} \hat{n}_{j \downarrow} + n_{j \downarrow} \hat{n}_{i \uparrow} - n_{i \uparrow} n_{j \downarrow}$. However, for terms like $\hat{n}_{i \sigma} \hat{n}_{j \sigma}$, when doing the mean-field approximation we will unavoidable find terms like those of the second line for the generic equation above; that is, the term: $$-\langle \hat{c}^\dagger_{i \sigma} \hat{c}_{j \sigma} \rangle \hat{c}^\dagger_{j \sigma}\hat{c}_{i \sigma} - \langle \hat{c}^\dagger_{j \sigma} \hat{c}_{i \sigma}\rangle \hat{c}^\dagger_{i \sigma}\hat{c}_{j \sigma} + \langle \hat{c}^\dagger_{i \sigma} \hat{c}_{j \sigma} \rangle \langle \hat{c}^\dagger_{j \sigma}\hat{c}_{i \sigma} \rangle,$$ and here is the problem. We need to include somehow in the self-consistency the non-diagonal charges $n_{ij\sigma}:=\langle \hat{c}^\dagger_{i \sigma} \hat{c}_{j \sigma} \rangle. $

In order to do self-consistency on the charges we should express the $n_{ij \sigma}$ in terms of the $n_{i \sigma},$ but I don't think there is any analytical way of doing this even when all expected values are taken over Slater deterinants. Am I right? I know that I can express sums of non-diagonal charges, $\sum_j n_{i j \sigma}$ comfortably as sums of electron-hole interactions, $\sum_{i \neq j} n_{i \sigma} \left( 1 - n_{i \sigma} \right)$, which is convenient to write the Hartree-Fock energy of lattice models when the $J_{ij}$ parameters are constant. But in general, an isolated $n_{ij \sigma}$ seems untreatable. Two possible solutions come to mind:

  1. Finding approximations for $n_{ij \sigma}$ in terms of $n_{k \sigma}$. How can this be done? Can the identity with $\sum_{i \neq j} n_{i \sigma} \left( 1 - n_{i \sigma} \right)$ (that is exact over Slater determinants) be used?

  2. Doing self-consistency in terms of $n_{ij \sigma}$ instead of just the charges. I have tried this last option for things like PPP parametrization on hydrocarbons and I've encountered cases on which, even using a mixing algorithm on all the density matrix, the convergence is quite problematic. Has this be done before and how? (meaning, Lattice Hartree-Fock where self-consistency is done in terms of the full density matrix)

$\endgroup$

1 Answer 1

0
$\begingroup$

Once the Hartree-Fock approximation is done in the Hamiltonian, it becomes a quadratic one, i.e., it can be exactly diagonalized. In terms of the operators it means a linear transformation like $$ c_{j\sigma}=\sum_kU_{jk}a_{k\sigma}\leftrightarrow a_{k\sigma}=\sum_jV_{kj}c_{j\sigma} $$ One can then express any product of operators in terms of new operators in the diagonal basis: $$ n_{j\sigma}=c_{j\sigma}^\dagger c_{j\sigma}=...\text{etc.} $$ Thus, there are no conceptual difficulties, although the non-diagonal terms might make solving the equations self-consistenly trather tedious or require some numerics (like diagonalizing a matrix).

$\endgroup$
2
  • $\begingroup$ Sorry, maybe I misunderstood your point, but in principle I do not see how does this answer the question. I know the diagonalization is easy for the quadratic hamiltonian. The point is how to deal with the non-diagonal charges in the self-consistency: do we rewrite them in terms of the charges, or do we do self-consistency in terms of the full density matrix? I have edited the question and highlighted with bold letters the question to make this clearer. $\endgroup$
    – Qwertuy
    Commented May 19, 2022 at 13:19
  • $\begingroup$ @Qwertuy self-consistency means that you solve the closed system of equations for $\langle c_{i\sigma}^\dagger c_{j\sigma}\rangle$. These quantities can be expressed in terms of the solutions of the quadratic Hamiltonian, i.e., in terms of the coefficients $U_{jk}, V_{kj}$, which in turn depend on the quantities $\langle c_{i\sigma}^\dagger c_{j\sigma}\rangle$, since these are coefficients in the Hamiltonian. I am not sure I understand where the problem lies... perhaps, you could elaborate further in your post, how you set up the self-consistent equations. $\endgroup$
    – Roger V.
    Commented May 19, 2022 at 13:26

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.