Structural and Electronic Evolution of Bilayer Nickelates Under Biaxial Strain

TL;DR

This study uses first-principles calculations to analyze how epitaxial strain affects the structural and electronic properties of bilayer nickelates, providing insights relevant to high-temperature superconductivity.

Contribution

It systematically explores the effects of biaxial strain on Re3Ni2O7 bilayer nickelates, revealing key electronic structural changes and contrasting them with high-pressure phases.

Findings

Compressive strain increases Ni-O-Ni bond angle towards 180°.

Ni $d_{z^2}$ bands move away from the Fermi level under strain.

Presence of $d_{z^2}$ bands at Fermi level may not be essential for superconductivity.

Abstract

The discovery of high-Tc superconductivity around 80K in bilayer nickelate La3Ni2O7 under high pressure has expanded the family of high-Tc superconductors above the nitrogen boiling temperature. Recent studies have further shown that ambient pressure superconductivity with a Tc exceeding 40K can be achieved in compressively strained La3Ni2O7 thin films, offering a tunable platform for investigating the pairing mechanism in high-Tc nickelates. A comprehensive understanding of the structural and electronic properties of bilayer nickelate under epitaxial strain is essential to advance this active field. In this work, we employ first-principles calculations to systematically explore the entire rare-earth (Re) series of bilayer nickelates Re3Ni2O7 in the realistic orthorhombic Amam phase under various compressive and tensile strain conditions. We highlight the materials properties change when strain is applied, and compare these results with those observed under high pressure. Our findings show that 2.5\% compressive strain increases the apical Ni-O-Ni bond angle toward 180 degree, and causes the Ni $d_{z^2}$ bands to move away from the Fermi level. The tight-binding parameters for the 2.5\% compressively strained La3Ni2O7 are quite similar to those of the unstrained material, except that the on-site energy difference between the Ni $d_{z^2}$ and $d_{x^2-y^2}$ orbitals increases by about 50 percent. Notably, the absence of the $d_{z^2}$ bands at the Fermi energy under compressive strain contrasts sharply with the electronic structure in the high-pressure {\it Fmmm} phase, suggesting that the presence of $d_{z^2}$ bands at the Fermi energy may not be a requisite for superconductivity.