Superconductivity and Electronic Structures of Nickelate Thin Film Superstructures
arXiv:2509.03502 · doi:10.1038/s41586-026-10352-7
Abstract
Ruddlesden-Popper (RP) nickelates have emerged as a crucial platform for exploring the mechanisms of high-temperature superconductivity. However, the Fermi surface topology required for superconductivity remains elusive. Here, beyond the superconducting pure bilayer (2222) phase, we report the thin film growth and ambient-pressure superconductivity of monolayer-bilayer (1212) and bilayer-trilayer (2323) superstructures, together with the absence of superconductivity in monolayer-trilayer (1313) superstructure, under identical compressive epitaxial strain. The onset superconducting transition temperatures range from 46 to 50 K, exceeding the McMillan limit. Angle-resolved photoemission spectroscopy reveals key Fermi surface differences in these atomically-engineered structures. In superconducting 1212 and 2222 films, a dispersive hole-like band () forms an underlying Fermi pocket, surrounding the Brillouin zone corner. In contrast, the top of the flat band () is observed ~70 meV below in the non-superconducting 1313 films. Particularly, the superconducting 2323 films host both and bands. The polarization dependence of the bands reveals their Ni origin. Our findings expand the family of ambient-pressure nickelate superconductors and establish a connection between structural configuration, electronic structure, and the emergence of superconductivity in nickelates.
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