Energy-Band Structure and Optical Spectrum of Grey Tin

Fred H. Pollak, Manuel Cardona, C. W. Higginbotham, Frank Herman, and John P. Van Dyke
Phys. Rev. B 2, 352 – Published 15 July 1970
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Abstract

A first-principles relativistic orthogonalized-plane-wave calculation has been used to determine the energy eigenvalues of grey tin at seven key points of the reduced zone. An extended zone k·p method has been used as an interpolation scheme to map out the band structure in the remainder of the zone. Optical constants and derivative optical constants have been calculated from the k·p parameters. The calculated normal incidence reflectivity is compared to experiment. A detailed critical-point analysis of the calculated optical spectra is presented. Valence-band mass parameters, effective masses, and g factors at several points in the zone have been obtained and are compared to available experimental data.

  • Received 2 December 1969

DOI:https://doi.org/10.1103/PhysRevB.2.352

©1970 American Physical Society

Authors & Affiliations

Fred H. Pollak, Manuel Cardona, and C. W. Higginbotham*

  • Department of Physics, Brown University, Providence, Rhode Island 02912

Frank Herman and John P. Van Dyke

  • IBM Research Laboratory, San Jose, California 95114

  • *Present address: General Telephone and Electronics Laboratories, Bayside, N. Y.
  • Present address: Sandia Laboratory, Albuquerque, N. M.

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Vol. 2, Iss. 2 — 15 July 1970

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