Published March 18, 2025 | Published
Journal Article Open

First-principles electron-phonon interactions and polarons in the parent cuprate La₂CuO₄

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Paul Scherrer Institute
  • 3. ROR icon Beijing Institute of Technology
  • 4. ROR icon École Polytechnique Fédérale de Lausanne
An error occurred while generating the citation.

Abstract

Understanding electronic interactions in high-temperature superconductors is an outstanding challenge. In the widely studied cuprate materials, experimental evidence points to strong electron-phonon (𝑒-ph) coupling and broad photoemission spectra. Yet, the microscopic origin of this behavior is not fully understood. Here, we study 𝑒-ph interactions and polarons in a prototypical parent (undoped) cuprate, La₂⁢CuO₄ (LCO), by means of first-principles calculations. Leveraging parameter-free Hubbard-corrected density functional theory, we obtain a ground state with the band gap and Cu magnetic moment in nearly exact agreement with experiments. This enables a quantitative characterization of 𝑒-ph interactions. Our calculations reveal two classes of longitudinal optical (LO) phonons with strong 𝑒-ph coupling to hole states. These modes consist of bond stretching and bond bending in the Cu-O plane as well as vibrations of apical O atoms. The hole spectral functions, obtained with a cumulant method that can capture strong 𝑒-ph coupling, exhibit broad quasiparticle peaks with a small spectral weight (𝑍≈0.25) and pronounced LO-phonon sidebands characteristic of polaron effects. Our calculations predict features observed in photoemission spectra, including a 40-meV peak in the 𝑒-ph coupling distribution function not explained by existing models. These results show that the universal strong 𝑒-ph coupling found experimentally in doped lanthanum cuprates is also present in the parent compound, and elucidate its microscopic origin.

Copyright and License

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Acknowledgement

This work was primarily supported by the Air Force Office of Scientific Research (AFOSR) and Clarkson Aerospace Corp under Award No. FA9550-21-1-0460. Code development was supported by the National Science Foundation under Grant No. OAC-2209262. I.T. and N.M. acknowledge support by the NCCR MARVEL, a National Centre of Competence in Research, funded by the Swiss National Science Foundation (Grant No. 205602). This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility located at Lawrence Berkeley National Laboratory, operated under Contract No. DE-AC02-05CH11231.

Supplemental Material

The supplemental files include additional computational details, computed band gap and magnetic moment as a function of U, the phonon dispersion computed from DFPT+U, and animations for the strongly-coupled phonon modes.

Files

PhysRevResearch.7.L012073.pdf
Files (12.6 MB)
Name Size Download all
md5:8137b42736387e6d21be349def8de6c4
803.6 kB Preview Download
md5:8a8ffb595063672b7412cf853926d446
1.8 MB Preview Download
md5:e2180b6675ac031c7fff2cc41fcb40e1
10.0 MB Preview Download

Additional details

Created:
March 19, 2025
Modified:
March 19, 2025