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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

DOI 10.1103/PhysRevB.51.644 · Physical Review B

T1

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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 (ω) of the apical oxygen (OA) in Hg-OA-Cu bonds of HgBa2Can−1CunO2n+2+δ superconductors. For both Hg-1201 and Hg-1223, Δ(ω2/ω02)/ΔP is found to be strongly correlated with ΔTc/ΔP, where ω0 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.

Source-reported materials — not catalogue approval

FormulaReported Tc (K)Pressure (GPa)Type
HgBa2CuO4+δ

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92Pressure unresolvedonset
HgBa2CuO4+δ

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92Pressure unresolvedonset
HgBa2Ca2Cu3O8+δ

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134Pressure unresolvedonset
HgBa2Ca2Cu3O8+δ

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134Pressure unresolvedonset
HgBa2Ca2Cu3O8+δ

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16430 GPaunknown

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