corner
corner

Phys. Rev. B 37, 1587–1593 (1988)

Temperature-dependent far-infrared reflectance of La-Sr-Cu-O and La-Ca-Cu-O: Bardeen-Cooper-Schrieffer electrodynamics but uncertain energy gap

Download: PDF (777 kB) Buy this article Export: BibTeX or EndNote (RIS)

M. S. Sherwin, P. L. Richards, and A. Zettl
Department of Physics, University of California, Berkeley, California 94720
Materials and Chemical Sciences Division, Lawrence Berkeley Laboratory, Berkeley, California 94720

Received 21 September 1987; published in the issue dated 1 February 1988

The available far-infrared data for polycrystalline La-Sr-Cu-O and La-Ca-Cu-O show a reflectance edge with energy near 2.5kBTc. This edge has been variously interpreted as the onset of absorption due to an energy gap, and as a low-frequency plasma edge caused by strong far-infrared resonances. Our measured temperature dependence of the reflectance edge closely fits the temperature dependence of the order parameter in a mean-field theory, and hence is consistent with the energy-gap hypothesis. In this paper, we construct a model dielectric function for La1.85Sr0.15CuO4 which is consistent with mean-field theory and the hypothesis of a plasma edge. We find that the temperature dependence of the plasma frequency in this model also closely fits the measured temperature dependence of the reflectance edge. Furthermore, both hypotheses accurately predict the experimentally observed temperature dependence of the absorption at frequencies much less than the reflectance edge. This observation has significant implications for the construction of fast low-loss superconducting devices. We conclude that the electrodynamics of the superconducting transition in La1.85Sr0.15CuO4 are well described by a Bardeen-Cooper-Schrieffer-like mean-field theory. However, given the identical predictions of the energy-gap and plasma-edge hypotheses, it is premature to deduce a precise value for the magnitude of the energy gap from the infrared data.

© 1988 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.37.1587
DOI:
10.1103/PhysRevB.37.1587
PACS:
74.30.Gn, 74.70.Vy, 78.20.Ci