Superconductivity by Kinetic Energy Saving?
Superconductivity by Kinetic Energy Saving?
A brief introduction is given in the generic microscopic framework of superconductivity. The consequences for the temperature dependence of the kinetic energy, and the correlation energy are discussed for two cases: The BCS scenario and the non-Fermi liquid scenario. A quantitative comparison is made between the BCS-prediction for d-wave pairing in a band with nearest neighbor and next-nearest neighbor hoppping and the experimental specific heat and the optical intraband spectral weight along the plane. We show that the BCS-prediction produces the wrong sign for the kink at Tc of the intraband spectral weight, even though the model calculation agrees well with the specific heat.
C. Presura、H. J. A. Molegraaf、I. Santoso、D. van der Marel
物理学
C. Presura,H. J. A. Molegraaf,I. Santoso,D. van der Marel.Superconductivity by Kinetic Energy Saving?[EB/OL].(2003-02-10)[2025-06-29].https://arxiv.org/abs/cond-mat/0302169.点此复制
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