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Cu and O NMR studies of the magnetic properties ofYBa2Cu3O6.63(Tc=62 K)

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Takigawa, M., Reyes, A. P., Hammel, P. C., Thompson, J. D., Heffner, R. H., Fisk, Z., Ott, K. C.·1991·Physical Review B

Abstract

The microscopic magnetic properties of the ${\mathrm{CuO}}_{2}$ planes in ${\mathrm{YBa}}_{2}$${\mathrm{Cu}}_{3}$${\mathrm{O}}_{6.63}$ (${\mathit{T}}_{\mathit{c}}$=62 K) have been investigated in Cu and O NMR experiments. Unlike the fully oxygenated Y-Ba-Cu-${\mathrm{O}}_{7}$ (${\mathit{T}}_{\mathit{c}}$\ensuremath{\simeq}90 K), the various components of the Cu and O Knight-shift tensors show strong but identical temperature dependences in the normal state. This supports the picture that there is only one spin component in the ${\mathrm{CuO}}_{2}$ planes. The spin susceptibility deduced from Knight-shift results shows significant reduction with decreasing temperature in the normal state. The temperature dependences of the nuclear-spin-relaxation rates (1/${\mathit{T}}_{1}$) are very different for the Cu and the O sites. 1/(${\mathit{T}}_{1}$T) at the O sites is nearly proportional to the spin susceptibility. 1/(${\mathit{T}}_{1}$T) at the Cu sites shows a broad peak around 150 K. We discuss these relaxation behaviors based on a model of the dynamical spin susceptibility proposed by Millis, Monien, and Pines.

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Metadata

Authors
Takigawa, M., Reyes, A. P., Hammel, P. C., Thompson, J. D., Heffner, R. H., Fisk, Z., & Ott, K. C.
Venue
Physical Review B
Published
1991-01-01
Volume
43
Issue
1
Pages
247-257
ISSN
  • 0163-1829 (ISSN-L)
  • 1095-3795
OpenAlex
W2037391100
Cited by
662
References
0
FWCI
38.21
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Cu and O NMR studies of the magnetic properties ofYBa2Cu3O6.63(Tc=62 K). https://app.cochat.ai/papers/10.1103/physrevb.43.247
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Takigawa, M., Reyes, A. P., Hammel, P. C., Thompson, J. D., Heffner, R. H., Fisk, Z., & Ott, K. C. (1991). Cu and O NMR studies of the magnetic properties ofYBa2Cu3O6.63(Tc=62 K). Physical Review B. https://doi.org/10.1103/physrevb.43.247

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