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Nature 452, 975-978 (24 April 2008) | doi:10.1038/nature06874; Received 10 October 2007; Accepted 21 February 2008

There is a Brief Communication Arising (2 October 2008) associated with this document.

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Small phonon contribution to the photoemission kink in the copper oxide superconductors

Feliciano Giustino1,2, Marvin L. Cohen1,2 & Steven G. Louie1,2

  1. Department of Physics, University of California at Berkeley,
  2. Materials Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

Correspondence to: Steven G. Louie1,2 Correspondence and requests for materials should be addressed to S.G.L. (Email: sglouie@berkeley.edu).

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Despite over two decades of intense research efforts, the origin of high-temperature superconductivity in the copper oxides remains elusive. Angle-resolved photoemission spectroscopy experiments1, 2 have revealed a kink in the dispersion relations (energy versus wavevector) of electronic states in the copper oxides at binding energies of 50-80 meV, raising the hope that this anomaly could be a key to understanding high-temperature superconductivity. The kink is often interpreted in terms of interactions between the electrons and a bosonic field. Although there is no consensus on the nature of the bosons (or even whether a boson model is appropriate), both phonons1 and spin fluctuations2 have been proposed as possible candidates. Here we report first-principles calculations of the role of phonons and the electron–phonon interaction in the photoemission spectra of La2 - xSrxCuO4. Our calculations within the standard formalism demonstrate that the phonon-induced renormalization of the electron energies and the Fermi velocity is almost one order of magnitude smaller than the effect observed in photoemission experiments. Therefore, our result rules out electron–phonon interaction in bulk La2 - xSrxCuO4 as the exclusive origin of the measured kink. Our conclusions are consistent with those reached independently in a recent study3 of the related compound YBa2Cu3O7.

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