Effect of Pressure and Oxygen-Isotope Substitution on Density-Wave Transitions in LaNiO
arXiv:2503.04400 · doi:10.1103/nrqn-m22c
Abstract
Understanding the interplay between magnetism and superconductivity in nickelate systems is a key objective in condensed matter physics. Here, we present a systematic muon-spin rotation/relaxation (SR) and resistivity study of the trilayer Ruddlesden-Popper nickelate LaNiO under ambient and applied pressure, combined with oxygen-isotope substitution. At ambient pressure, two incommensurate spin-density-wave (SDW) transitions are identified at K and K. Comparison of the internal magnetic fields with dipole-field calculations reveals a magnetic structure consistent with antiferromagnetically coupled SDW order on the outer two Ni layers, with smaller moments on the inner layer. Above , the moments lie mainly in the plane, whereas below this temperature they develop a -axis component. The internal fields at the muon stopping sites appear abruptly at , suggesting a first-order-like SDW transition closely linked to the charge-density-wave (CDW) order occurring at the same temperature (). Under pressure, all transition temperatures -- , , and -- are suppressed at a nearly uniform rate of K/GPa. This contrasts with bilayer LaNiO, where pressure enhances the separation between the SDW and CDW transitions. Oxygen-isotope substitution (O O) shifts to higher values. The isotope effect on and differs markedly: when CDW and SDW are intertwined, a notable isotope effect is observed on , yielding nearly identical isotope shifts for and , whereas no isotope effect is detected at , where the SDW transition occurs independently of the CDW.
18 pages, 10 figures