Nodal gap structure in Fe-based superconductors due to the competition between orbital and spin fluctuations
arXiv:1303.2871 · doi:10.1103/PhysRevB.88.045115
Abstract
To understand the origin of the nodal gap structure realized in BaFe(As,P), we study the three-dimensional gap structure based on the three-dimensional ten-orbital Hubbard model with quadrupole interaction. In this model, strong spin and orbital fluctuations develop by using the random-phase-approximation. By solving the Eliashberg gap equation, we obtain the fully-gapped s-wave state with (without) sign reversal between hole-like and electron-like Fermi surfaces due to strong spin (orbital) fluctuations, so called the -wave (-wave) state. When both spin and orbital fluctuations strongly develop, which will be realized near the orthorhombic phase, we obtain the nodal s-wave state in the crossover region between -wave and -wave states. The obtained nodal s-wave state possesses the loop-shape nodes on electron-like Fermi surfaces, due to the competition between attractive and repulsive interactions in k-space. In contrast, the SC gaps on the hole-like Fermi surfaces are fully-gapped due to orbital fluctuations. The present study explains the main characters of the anisotropic gap structure in BaFe(As,P) observed experimentally.
12 pages, 13 figures, accepted for publication in PRB. An appendix has been added
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