Impact of the orbital current order on the superconducting properties of the kagome superconductors
Hong-Min Jiang, Ming-Xun Liu, Shun-Li Yu
DOI 10.1103/PhysRevB.107.064506 · Physical Review B
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Abstract
Motivated by recent experimental evidence signaling chiral charge order in vanadium-based kagome superconductors, we investigate theoretically the impact of chiral flux charge order on the experimental outcomes for normal and superconducting (SC) properties. It is revealed that the spectral weight on the Fermi surface (FS) is partially gapped by chiral flux charge order, with the reservation of the spectral weight on the M points and the midpoint between the two adjacent M points, resulting in the momentum-dependent energy gap being consistent with recent experimental observations. More importantly, by considering the influence of chiral flux charge order, we find that a conventional fully gapped SC pairing state evolves into a nodal gap feature for the spectral weight due to the spectral gap modulations on the FS. As a result, the U-shaped density of states (DOS) deforms to the V-shaped DOS along with the residual DOS near the Fermi energy. These results bear some resemblance to the experimental observations, and they may serve as a promising proposal to mediate the divergent or seemingly contradictory experimental outcomes regarding SC pairing symmetry.
Source-reported materials — not catalogue approval
| Formula | Reported Tc (K) | Pressure (GPa) | Type |
|---|---|---|---|
| CsV3Sb5 Archive — visibility unverified Source-occurrence policy only; no material identity or catalogue acceptance is inferred from the formula. | — | Pressure not reported | unknown |
| KV3Sb5 Archive — visibility unverified Source-occurrence policy only; no material identity or catalogue acceptance is inferred from the formula. | — | Pressure not reported | unknown |
| RbV3Sb5 Archive — visibility unverified Source-occurrence policy only; no material identity or catalogue acceptance is inferred from the formula. | — | Pressure not reported | unknown |
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