Origin of metal-insulator transition in rare-earth Nickelates
Swagata Acharya, Brooks Tellekamp, Jerome Jackson, Dimitar Pashov, Jeffrey L. Blackburn, Kirstin Alberi, Mark van Schilfgaarde
TL;DR
The paper tackles the origin of the metal-insulator transition in rare-earth nickelates (RNiO3) and its entanglement with magnetism and lattice distortions. It employs a parameter-free, first-principles MBPT approach—Quasiparticle Self-Consistent GW (QSGW) in the Questaal package—across seven RNiO3 to separate the effects of structural symmetry breaking and magnetism. It finds a metallic Pbnm phase and an insulating P2_1/n phase across all compounds, with MIT driven by spin-disproportionation between two inequivalent Ni sites and accompanying charge/orbital redistribution, including an orbital-selective gap and a midgap state from oxygen, stabilized by the breathing-mode distortion. The results highlight the essential role of non-local correlations and real-space spin multiplets in RNiO3, argue for minimal models that include at least two Ni sites, and offer a parameter-free route to disentangle magnetic and lattice contributions with implications for nickelate-based devices.
Abstract
Rare-earth nickelates RNiO3 (R=rare-earth element) exhibit three kinds of phase transitions with decreasing temperature: a structural transition from a pseudo-cubic to a monoclinic phase, a metal- insulator transition (MIT), and a magnetic transition from a paramagnetic state to an ordered one. The first two occur at the same temperature, which has led to a consensus that the MIT is driven by lattice distortions. We show here that the primary driving force for the MIT is magnetic; however because of the unusual d7 configuration of Ni, additional flexibility in spin configurations are also needed which symmetry-lowing structural deformations make possible. The latter enable Ni to disproportionate into two kinds: a high-spin and a low-spin configuration, which allow the system to reduce its unfavorable orbital moment and also open a gap.
