The $s^\pm$-Wave Superconductivity in the Pressurized La$_4$Ni$_3$O$_{10}$
Ming Zhang, Hongyi Sun, Yu-Bo Liu, Qihang Liu, Wei-Qiang Chen, Fan, Yang

TL;DR
This study investigates the pairing mechanism and symmetry in pressurized La$_4$Ni$_3$O$_{10}$, proposing an $s^{}$-wave pairing driven by Fermi surface nesting and interlayer orbital interactions, supported by a six-orbital tight-binding model and RPA calculations.
Contribution
The paper introduces a detailed six-orbital model and identifies $s^{}$-wave pairing as the mechanism in La$_4$Ni$_3$O$_{10}$, highlighting the role of the non-bonding $d_{z^2}$ band and Fermi surface nesting.
Findings
Identification of $s^{}$-wave pairing symmetry.
Fermi surface nesting between specific pockets drives pairing.
Interlayer $d_{z^2}$ orbital pairing is dominant.
Abstract
Recently, evidence of superconductivity (SC) has been reported in pressurized LaNiO. Here we study the possible pairing mechanism and pairing symmetry in this material. Through fitting the density-functional-theory band structure, we provide a six-orbital tight-binding model. In comparison with the band structure of LaNiO, the additional non-bonding band is importance to the pairing mechanism here. When the multi-orbital Hubbard interactions are included, our random-phase-approximation based study yields an -wave pairing. The dominant FS nesting with nesting vector is between the -pocket contributed by the bonding band top and the -pocket contributed by the non-bonding band bottom, leading to the strongest pairing gap amplitude and opposite gap signs within the two…
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Taxonomy
TopicsHigh-pressure geophysics and materials · Magnetic and transport properties of perovskites and related materials · Advanced Condensed Matter Physics
