Skip to content

Hubbard Model Hamiltonian

A standard spinful fermionic Hubbard Hamiltonian is

H=−t∑⟨i,j⟩,σ(ciσ†cjσ+cjσ†ciσ)+U∑ini↑ni↓−μ∑i,σniσ.H = -t \sum_{\langle i,j\rangle,\sigma} \left( c_{i\sigma}^\dagger c_{j\sigma} + c_{j\sigma}^\dagger c_{i\sigma} \right) + U\sum_i n_{i\uparrow}n_{i\downarrow} - \mu\sum_{i,\sigma}n_{i\sigma}.

Here

niσ=ciσ†ciσ.n_{i\sigma}=c_{i\sigma}^\dagger c_{i\sigma}.
  • Fermionic lattice modes are used.
  • Lattice geometry, boundary conditions, filling, and spin convention are specified.
  • tt is a hopping amplitude and UU is an onsite interaction.
  • Longer-range hopping, longer-range interactions, disorder, and phonons are omitted unless added.
  • Treating the Hubbard model as automatically realistic for every material.
  • Forgetting the chemical-potential term when working grand canonically.
  • Dropping fermionic signs in finite-basis matrix construction.
  • Comparing results without specifying lattice, dimension, filling, and boundary conditions.
  • J. Hubbard, “Electron correlations in narrow energy bands”, Proceedings of the Royal Society A 276, 238-257, 1963.
  • A. Altland and B. Simons, Condensed Matter Field Theory, 2nd ed., Cambridge University Press, 2010.