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The peculiar magnetic property evolution along (, La, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu): A first-principles study
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10.1063/1.3524527
/content/aip/journal/apl/97/23/10.1063/1.3524527
http://aip.metastore.ingenta.com/content/aip/journal/apl/97/23/10.1063/1.3524527
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

Evolution of the calculated energy difference between AFI and FM that corresponds to (blue star), along the series with the cell parameter, which relates to IR of rare earth (black rectangle). The red line is obtained by curve fitting, the lines are used to guide the eyes. Inset is the corresponding experimental results for comparison (see Ref. 18).

Image of FIG. 2.
FIG. 2.

Evolution of the partial density of states of Mn 3d orbital along the series (a) the beginning under the Fermi level and (b) the end above the Fermi level.

Image of FIG. 3.
FIG. 3.

Evolution of the energy differences between AFII and AFIII, which scales with (black star) and the atomic radius (blue rectangle) along the series with R changing from La to Lu. The lines are used to guide the eyes.

Image of FIG. 4.
FIG. 4.

Evolution of calculated magnetic anisotropic energy (black star) and the total angular magnetic moments of rare-earth ions (blue rectangle) along the series with R from La to Lu. The lines are used to guide the eyes.

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/content/aip/journal/apl/97/23/10.1063/1.3524527
2010-12-06
2014-04-19
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: The peculiar magnetic property evolution along RCu3Mn4O12 (R=Y, La, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu): A first-principles study
http://aip.metastore.ingenta.com/content/aip/journal/apl/97/23/10.1063/1.3524527
10.1063/1.3524527
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