First-principles electron-phonon interactions and polarons in the parent cuprate La₂CuO₄
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, La₂CuO₄ (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.
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Additional details
- United States Air Force Office of Scientific Research
- FA9550-21-1-0460
- National Science Foundation
- OAC-2209262
- Swiss National Science Foundation
- 205602
- United States Department of Energy
- DE-AC02-05CH11231
- Accepted
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2025-02-11Accepted
- Caltech groups
- Division of Engineering and Applied Science (EAS)
- Publication Status
- Published