Skip to main content
Proceedings of the National Academy of Sciences of the United States of America logoLink to Proceedings of the National Academy of Sciences of the United States of America
. 1972 Apr;69(4):933–937. doi: 10.1073/pnas.69.4.933

Optical Versus Thermal Transitions in Solids at High Pressure

H G Drickamer 1, C W Frank 1, C P Slichter *
PMCID: PMC426598  PMID: 16591977

Abstract

Pressure-induced electronic transitions have been observed in a wide variety of materials. In particular, Mössbauer resonance studies under high pressure have revealed changes of oxidation state and spin state of iron as a function of pressure. These processes involve the thermal transfer of an electron to a new ground state of the system. The difference in energy between states is frequently measured by optical absorption. In this paper, we relate the energy of the optical absorption peak and its half-width to the difference in thermal energy between the two states as a function of pressure. We show that the optical peak will broaden with pressure only if there is a difference between the force constants of the ground and excited states. These relationships permit the prediction from optical absorption data of the pressure at which a new ground state will be obtained. We demonstrate that the predictions are qualitatively correct for the reduction of Fe(III) in a series of ferric hydroxamates, and for the low-spin to high-spin transition of Fe(II) in ferrous phenanthroline complexes.

Keywords: electrons, excitations, theoretical

Full text

PDF
937

Selected References

These references are in PubMed. This may not be the complete list of references from this article.

  1. Grenoble D. C., Drickamer H. G. Effect of pressure on the electronic structure of ferric hydroxamates and ferrichrome A. Proc Natl Acad Sci U S A. 1971 Mar;68(3):549–553. doi: 10.1073/pnas.68.3.549. [DOI] [PMC free article] [PubMed] [Google Scholar]

Articles from Proceedings of the National Academy of Sciences of the United States of America are provided here courtesy of National Academy of Sciences

RESOURCES