Comparative optical study of the two-dimensional donor-type intercalation compounds graphite-KHx and their binary counterparts C8K and C24K

G. L. Doll, M. H. Yang, and P. C. Eklund
Phys. Rev. B 35, 9790 – Published 15 June 1987
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Abstract

We report the results of optical reflectivity studies of the stage-1 and -2 graphite-KHx intercalation compounds prepared by direct reaction of highly ordered pyrolytic graphite and KH powder. The stage-1 and -2 binary graphite-K compounds are studied for comparison. The optical data are analyzed in terms of a model involving two-dimensional (2D) graphitic π electrons and three-dimensional (3D) nearly free K(4s) electrons. The model is used to interpret the observed values of the free-carrier unscreened plasma frequencies and the position of the interband absorption threshold to determine experimental values for the Fermi level (EF) in the carbon π band(s) and the fractional occupation of the K(4s) band. For the hydrides, we find quantitative evidence that the hydrogen states lie below EF. Thus, hydrogen is present as H, acting as an acceptor, thereby compensating the electron donation to the π bands from the K(4s) states. This assumption and the optical data for the stage-1 and -2 hydrides results in a [H]/[K] ratio of 0.8, in excellent agreement with chemical analyses reported by Guérard and co-workers, and leads to very small values for the fractional K(4s) band occupation fK<0.03 electrons per K atom. Within the framework of a superimposed 2D (π) and 3D [K(4s)] rigid-band model, our experimental results support an empty K(4s) band (i.e., fK=0) in stage-2 C24K. In stage-1 C8K, the rigid-band model yields large values for fK (fK>0.5 electrons per K atom), unless the value of the optical mass of the electrons in the K(4s) states is larger than 2. The C8K results are also discussed in terms of more sophisticated energy-band calculations.

  • Received 17 February 1987

DOI:https://doi.org/10.1103/PhysRevB.35.9790

©1987 American Physical Society

Authors & Affiliations

G. L. Doll, M. H. Yang, and P. C. Eklund

  • Department of Physics and Astronomy, University of Kentucky, Lexington, Kentucky 40506

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Issue

Vol. 35, Iss. 18 — 15 June 1987

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