Welcome to the Hubbard Model Explorer

1. The Hubbard Model

The Hubbard model was introduced by John Hubbard in 1963 to describe the behavior of electrons in a lattice, especially their interaction and collective motion. It is a cornerstone in the study of strongly correlated electron systems.

The model captures two key physical effects: the kinetic energy of electrons hopping between sites and the on-site Coulomb repulsion when two electrons occupy the same site.

\[ H = -t \sum_{\langle i,j \rangle, \sigma} \left( c^\dagger_{i\sigma} c_{j\sigma} + \text{h.c.} \right) + U \sum_i n_{i\uparrow} n_{i\downarrow} \]

With:

One can also use the extended Hubbard Hamiltonian, given by:

\[ H = -\sum_{\langle i,j \rangle, \sigma} t_{ij} \left( c^\dagger_{i\sigma} c_{j\sigma} + \text{h.c.} \right) + U \sum_i n_{i\uparrow} n_{i\downarrow} + V \sum_{\langle i,j \rangle} n_i n_j + K \sum_{\langle i,j \rangle} \vec{S}_i \cdot \vec{S}_j \]

With:

This previous Hamiltonians corresponds to the one-band Hubbard model, which is sufficient to describe some correlated systems.

However, in more complex materials such as transition metal oxides or systems with strong crystal field splitting, multi-band Hubbard models become necessary to accurately capture the low-energy physics.

The extended multi-band Hubbard Hamiltonian takes the form:

\[ \mathcal{\hat{H}} = - \sum_{R,R',\sigma} \sum_{i,i'} t_{Ri,R'i'} \hat{c}_{Ri,\sigma}^\dagger \hat{c}_{R'i',\sigma} + \frac{1}{2} \sum_{R_i, R_j, R_k, R_l} \sum_{i,j,k,l} \hat{c}^\dagger_{R_i, i} \hat{c}_{R_j, j} U_{R_i,i; R_j, j; R_k, k; R_l, l} \hat{c}_{R_k, k}^\dagger \hat{c}_{R_l, l}, \]

With:

The interaction parameter \( U_{R_i,i;\,R_j,j;\,R_k,k;\,R_l,l} \) is given by:

\[ U_{R_i,i;\,R_j,j;\,R_k,k;\,R_l,l} = \int d\mathbf{r} \, d \mathbf{r'} \,\phi_{R_i,i}^*(\mathbf{r})\,\phi_{R_j,j}^*(\mathbf{r'})\,\hat{\mathcal{H}}_U\, \phi_{R_k,k}(\mathbf{r})\,\phi_{R_l,l}(\mathbf{r'}). \]

The two-body operator \( \hat{\mathcal{H}}_U \) encapsulates more than just the bare Coulomb repulsion. Due to renormalization effects, such as screening by high-energy electrons, the effective interaction between low-energy degrees of freedom is modified. This results in a screened Coulomb interaction, often denoted \( W_r(\mathbf{r}, \mathbf{r}', \omega) \), which can be computed using constrained Random Phase Approximation (cRPA) techniques.

2. Search for Material Parameters

Type a material name below to search for its Hubbard model parameters. Then select a model type (e.g. one-band, two-band).

Enter full name like Sr2CuO3 and select a model type.

3. Computed Results

Type a material name below to search for its properties computed with its Hubbard parameters.

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