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Theory of Pressure Dependence of Superconductivity in Bilayer Nickelate La3Ni2O7

Kai-Yue Jiang, Yu-Han Cao, Qing-Geng Yang, Hong-Yan Lu, Qiang-Hua Wang

DOI 10.1103/PhysRevLett.134.076001 · Physical Review Letters

T1

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Abstract

A recent experiment showed the superconducting transition temperature in the Ruddlesden-Popper bilayer La3Ni2O7 decreases monotonically with increasing pressure above 14 GPa. In order to unravel the underlying mechanism for this unusual dependence, we performed theoretical investigations by combining the density functional theory (DFT) and the unbiased functional renormalization group (FRG). Our DFT calculations show that the Fermi pockets are essentially unchanged with increasing pressure (above 14 GPa), but the bandwidth is enlarged, and particularly the interlayer hopping integral between the nickel 3d3z2−r2 orbitals is enhanced. From the DFT band structure, we construct the bilayer tight-binding model in terms of the nickel 3d3z2−r2 and 3dx2−y2 orbitals. On this basis, we investigate the superconductivity induced by correlation effects by FRG calculations. We find consistently s±-wave pairing triggered by spin fluctuations, but the latter are weakened by pressure and lead to a decreasing transition temperature versus pressure, in qualitative agreement with the experiment. We emphasize that the itinerancy of the d orbitals is important and captured naturally in our FRG calculations, and we argue that the unusual pressure dependence would be unnatural, if not impossible, in the otherwise local-moment picture of the nickel d orbitals. This sheds light on the pertinent microscopic description, and more importantly the mechanism, of superconductivity in La3Ni2O7.

Source-reported materials — not catalogue approval

FormulaReported Tc (K)Pressure (GPa)Type
La3Ni2O7

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Source-occurrence policy only; no material identity or catalogue acceptance is inferred from the formula.

8014 GPaunknown
La3Ni2O7

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Source-occurrence policy only; no material identity or catalogue acceptance is inferred from the formula.

8318 GPaunknown

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