Optical spectral weight distribution in d-wave superconductors
arXiv:cond-mat/0404192 · doi:10.1103/PhysRevB.69.224501
Abstract
The distribution in frequency of optical spectral weight remaining under the real part of the optical conductivity in the superconducting state of a d-wave superconductor depends on impurity concentration, on the strength of the impurity potential as well as on temperature and there is some residual absorption even at T = 0. In BCS theory the important weight is confined to the microwave region if the scattering is sufficiently weak. In an Eliashberg formulation substantial additional weight is to be found in the incoherent, boson assisted background which falls in the infrared and is not significantly depleted by the formation of the condensate, although it is shifted as a result of the opening of a superconducting gap.
14 Pages, 9 Figures, Accepted for publication in Phys. Rev. B
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- Optical determination of the superconducting energy gap in electron-doped Pr_{1.85}Ce_{0.15}CuO_4
- Zero temperature optical conductivity of ultra-clean Fermi liquids and superconductors
- Infrared Signature of the Superconducting State in Pr(2-x)Ce(x)CuO(4)
- Optical Sum Rule in Finite Bands
- Optical sum rule in metals with a strong interaction
- Optical sum in Nearly Antiferromagnetic Fermi Liquid Model