Revisiting superconductivity in the extended one-band Hubbard model: pairing via spin and charge fluctuations

preprint2022arXivOpen access

Abstract

The leading superconducting instabilities of the two-dimensional extended repulsive one-band Hubbard model within spin-fluctuation pairing theory depend sensitively on electron density, band and interaction parameters. We map out the phase diagrams within a random phase approximation (RPA) spin- and charge-fluctuation approach, and find that while B1gB_{1g} (dx2−y2d_{x^2-y^2}) and B2gB_{2g} (dxyd_{xy}) pairing dominates in the absence of repulsive longer-range Coulomb interactions VNNV_{\rm NN}, the latter induces pairing in other symmetry channels, including e.g A2gA_{2g} (gg-wave), nodal A1gA_{1g} (extended ss-wave), or nodal EuE_u (pp-wave) spin-triplet superconductivity. At the lowest temperatures, transition boundaries in the phase diagrams between symmetry-distinct spin-singlet orders generate complex time-reversal symmetry broken superpositions. By contrast, we find that boundaries between singlet and triplet regions are characterized by first-order transitions. Finally, motivated by recent photoemission experiments, we have determined the influence of an additional explicitly attractive nearest-neighbor interaction, VNN<0V_{\rm NN}<0, on the superconducting gap structure. Depending on the electronic filling, such an attraction boosts EuE_u (pp-wave) spin-triplet or B1gB_{1g} (dx2−y2d_{x^2-y^2}) spin-singlet ordering.

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