Interplay of two orbitals in Superconducting LaNiO Under Pressure
arXiv:2310.02915
Abstract
The discovery of high- superconductivity (SC) in LaNiO (LNO) has aroused a great deal of interests. Previously, it was proposed that the Ni- orbital is crucial to realize the high- SC in LNO: The preformed Cooper pairs therein acquire coherence via hybridization with the orbital to form the SC. However, we held a different viewpoint that the interlayer pairing -wave SC is induced by the orbital, driven by the strong interlayer superexchange interaction. To include effects from both -orbitals , we establish a two-orbital bilayer - model. Our calculations reveal that due to the no-double-occupancy constraint, the band and the bonding band are flattened by a factor of about 2 and 10, respectively, which is consistent with recent angle-resolved-photo-emission-spectroscopy measurements. Consequently, a high temperature SC can be hardly induced in the -orbital due to the difficulty to develop phase coherence. However, it can be easily achieved by the orbital under realistic interaction strength. With electron doping, the -band gradually dives below the Fermi level, but continues to enhance, suggesting that it is not necessary for the high- SC in LNO. With hole doping, initially drops and then rises, accompanied by the crossover from the BCS to BEC-type superconducting transitions.
9.3 pages, 6 figures, with Appendix