Interaction-enhanced nesting in Spin-Fermion and Fermi-Hubbard models
arXiv:2402.13238 · doi:10.1103/PhysRevResearch.6.L032058
Abstract
The spin-fermion (SF) model postulates that the dominant coupling between low-energy fermions in near critical metals is mediated by collective spin fluctuations (paramagnons) peaked at the Néel wave vector, , connecting hot spots on opposite sides of the Fermi surface. It has been argued that strong correlations at hot spots lead to a Fermi surface deformation (FSD) featuring flat regions and increased nesting. This conjecture was confirmed in the perturbative self-consistent calculations when the paramagnon propagator dependence on momentum deviation from is given by . Using diagrammatic Monte Carlo (diagMC) technique we show that such a dependence holds only at temperatures orders of magnitude smaller than any other energy scale in the problem, indicating that a different mechanism may be at play. Instead, we find that a dependence yields a robust finite- scenario for achieving FSD. To link phenomenological and microscopic descriptions, we applied the connected determinant diagMC method to the Hubbard model and found that in this case: (i) the FSD is not very pronounced, and, instead, it is the lines of zeros of the renormalized dispersion relation that deform towards nesting; (ii) this phenomenon appears at large before the formation of electron and hole pockets; (iii) the static spin susceptibility is well described by . Flat FS regions yield a non-trivial scenario for realizing a non-Fermi liquid state.
5 pages, 4 figures
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