Micro-Raman study of the role of pressure in mercury-based superconductors

In Sang Yang, Hye Soo Shin, Hye Gyong Lee, Seung Joon Jeon, Hang Sun Ahn, Jaejun Yu, Sergey Lee, Sung Ik Lee, Nam H. Hur

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Abstract

Understanding the role of pressure in increasing Tc is a crucial issue in mercury-based superconductors. We report on the effect of pressure on the Raman frequency () of the apical oxygen (OA) in Hg-OA-Cu bonds of HgBa2Can-1CunO2n+2+ superconductors. For both Hg-1201 and Hg-1223, (2/02)/P is found to be strongly correlated with Tc/P, where 0 is the frequency at ambient pressure. Together with our local-density approximation total-energy phonon study of the OA-A1g Raman mode, it is concluded that the change of the OA Raman frequency is due to the change in Hg-OA bond strength, which may be directly related to the charge transfer between the CuO2 planes and the Hg-O layers.

Original languageEnglish
Pages (from-to)644-647
Number of pages4
JournalPhysical Review B
Volume51
Issue number1
DOIs
Publication statusPublished - 1995 Jan 1

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ASJC Scopus subject areas

  • Condensed Matter Physics

Cite this

Yang, I. S., Shin, H. S., Lee, H. G., Jeon, S. J., Ahn, H. S., Yu, J., Lee, S., Lee, S. I., & Hur, N. H. (1995). Micro-Raman study of the role of pressure in mercury-based superconductors. Physical Review B, 51(1), 644-647. https://doi.org/10.1103/PhysRevB.51.644