Comparison of band structure and superconductivity in FeSe_(0.5)Te_(0.5) and FeS
Comparison of band structure and superconductivity in FeSe_(0.5)Te_(0.5) and FeS作者机构:College of Physics and Electronic Engineering Zhengzhou University of Light Industry College of Science Hohai University School of Physics and Electronic Information Huaibei Normal University Department of Physics Ningbo University
出 版 物:《Chinese Physics B》 (中国物理B(英文版))
年 卷 期:2017年第26卷第12期
页 面:526-532页
核心收录:
学科分类:080705[工学-制冷及低温工程] 07[理学] 070205[理学-凝聚态物理] 08[工学] 0807[工学-动力工程及工程热物理] 0702[理学-物理学]
基 金:Project supported by the National Natural Science Foundation of China(Grant Nos.11604303 11604168 and 11574108)
主 题:iron-based superconductors theories and models of superconducting state pairing symmetry
摘 要:The isovalent iron chalcogenides, FeSe0.5Te0.5 and FeS, share similar lattice structures but behave very differently in superconducting properties. We study the underlying mechanism theoretically. By first principle calculations and tight-binding fitting, we find the spectral weight of the dX2-Y2 orbital changes remarkably in these compounds. While there are both electron and hole pockets in FeSe0.5Te0.5 and FeS, a small hole pocket with a mainly dX2-Y2 character is absent in FeS. We find the spectral weights of dX2-Y2 orbital change remarkably, which contribute to electron and hole pockets in FeSe0.5Te0.5 but only to electron pockets in FeS. We then perform random-phase-approximation and unbiased singular-mode functional renormalization group calculations to investigate possible superconducting instabilities that may be triggered by electron-electron interactions on top of such bare band structures. For FeSe0.5Te0.5, we find a fully gapped s-wave pairing that can be associated with spin fluctuations connecting electron and hole pockets. For FeS, however, a nodal dxy (or dx2-y2 in an unfolded Broullin zone) is favorable and can be related to spin fluctuations connecting the electron pockets around the corner of the Brillouin zone. Apart from the difference in chacogenide elements, we propose the main source of the difference is from the dX2-Y2 orbital, which tunes the Fermi surface nesting vector and then influences the dominant pairing symmetry.