We show that the coupling of charge and spin density fluctuations in the three-dimensional Hubbard model with total charge fixed severely restricts the occurrence of a continuous ferromagnetic transition.
In this work we use field-theoretic and renormalization-group methods to study the finite-temperature ferromagnetic phase transition in the three-dimensional Hubbard model. We show that the nature of the ferromagnetic transition may strongly depend on the constraint imposed on the system. For example, if the system is allowed to exchange particles with a reservoir, the stability criterion for the occurrence of a continuous phase transition can be calculated using the mean-field approximation. On the other hand, if the total charge is conserved and charge- and spin-density fluctuations are considered in the theory, a different criterion, quite distinct from the mean-field one, is found, resulting in a fluctuation-induced renormalized Heisenberg tricritical point. The tricritical behavior is studied by calculating the one-loop renormalized free energy and using scaling analysis to determine the tricritical exponents. Finally, the exact solution of the model in the spherical limit and near the ferromagnetic transition is presented, in which case no fluctuation-induced tricritical point is found.
We present results of quantum Monte Carlo simulations for the one-dimensional Hubbard model with next-nearest-neighbour hopping (t2). The appearance of double peaks in the spin and charge structure factors is identified with the doubling of ground states, each with its corresponding excitation modes. A quantitative phase diagram in the t2- (density) plane for fixed on-site coupling is obtained, and compared with weak-coupling renormalization group predictions. Four regions in this phase diagram are clearly identified: (i) singly peaked charge and spin structure factors; (ii) singly peaked ferromagnetic and charge fluctuations; (iii) singly peaked charge fluctuations and doubly peaked spin fluctuations; and (iv) doubly peaked spin and charge fluctuations.
We prove rigorously that the Hartree-Fock approximation to the ground state of the d-dimensional Hubbard model leads to saturated ferromagnetism when the particle density (more precisely, the chemical potential µ) is small and the coupling constant U is large, but finite. As in the usual Hartree-Fock theory we restrict attention to Slater determinants that are eigenvectors of the z-component of the total spin, Sz = ∑ x nx, ↑ − nx,↓, and we find that the choice 2Sz = N = particle number gives the lowest energy at fixed 0 < µ < 4d. 1 BLT, Version of 27-Jun-2005 2 1