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Electron‐Phonon Interaction and Strong Correlations in High‐Temperature Superconductors: One can not avoid the unavoidable

 

作者: Miodrag L. Kulic´,  

 

期刊: AIP Conference Proceedings  (AIP Available online 1904)
卷期: Volume 715, issue 1  

页码: 75-158

 

ISSN:0094-243X

 

年代: 1904

 

DOI:10.1063/1.1800734

 

出版商: AIP

 

数据来源: AIP

 

摘要:

The important role of the electron‐phonon interaction (EPI) in explaining the properties of the normal state and pairing mechanism in high‐Tcsuperconductors (HTSC) is discussed. A number of experimental results are analyzed such as: dynamical conductivity, Raman scattering, neutron scattering, ARPES, tunnelling measurements, isotope effect and etc. They give convincing evidence that the EPI is strong and dominantly contributes to pairing in HTSC oxides. It is argued that strong electronic correlations in conjunction with the pronounced (in relatively weakly screened materials) EPI are unavoidable ingredients for the microscopic theory of pairing in HTSC oxides. I present the well defined and controllable theory of strong correlations and the EPI. It is shown that strong correlations give rise to the pronouncedforward scattering peakin the EPI — the FSP theory. The FSP theory explains in a consistent way several (crucial) puzzles such as much smaller transport coupling constant than the pairing one (&lgr;tr≪ &lgr;ph), which are present if one interprets the results in HTSC oxides by the old Migdal‐Eliashberg theory for the EPI. The ARPES non‐shift puzzle — where the nodal kink at 70 meV is unshifted in the superconducting state while the anti‐nodal one at 40 meV is shifted, can be explained at present only by the FSP theory. It predicts also: (1) a knee‐like shape of the imaginary part of the self‐energy at&ohgr; < &ohgr;ph(70)what has been recently confirmed in ARPES measurements; (2) that the Coulomb scattering gives very small coupling constant &lgr;C<< &lgr;ph, which is also confirmed in ARPES spectra where &lgr;C< 0.4 and &lgr;ph> 1. A number of other interesting predictions of the FSP theory are also discussed. © 2004 American Institute of Physics

 

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