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• W2019887531 endingPage "797" @default.
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• W2019887531 abstract "In the triangular diagram of Cu-Ni-Fe alloys, the line of zero linear magnetostriction ${ensuremath{lambda}}_{s}$ approximately coincides with the line of zero extraordinary Hall constant ${R}_{s}$ and may be interpreted as the line where a $3d$ orbital degeneracy crosses the Fermi level. The ferromagnetic anisotropy of resistivity $frac{({ensuremath{rho}}_{mathrm{II}}ensuremath{-}{ensuremath{rho}}_{ensuremath{perp}})}{{ensuremath{rho}}_{0}}$ of quenched Cu-Ni-Fe alloys containing more than 60 wt% Ni has been measured at 20ifmmode^circelsetextdegreefi{}K, where impurity scattering dominates. The large anisotropy values observed in Ni-Fe alloys decrease gradually by addition of copper. In particular, the anisotropy decrease along the line ${ensuremath{lambda}}_{s}=0$ suggests that the orbital degeneracy is partially lifted by the addition of copper. This line differs from a line of constant electron concentration, indicating a departure from the rigid-band model. A $3d$ band model with separate iron, nickel, and copper sub-bands correctly predicts the location of the line if the degeneracy is assumed to be located at the top of the nickel sub-band (bottom of the iron sub-band). The same assumption applies successfully to Me-Ni-Fe alloys, where Me is any metal (Cr, W, Mo, V, etc.) forming a nonmagnetic sub-band above the Fermi level. Existing data show that the extraordinary Hall conductivity ${ensuremath{gamma}}_{{H}_{s}}=frac{{R}_{s}{M}_{s}}{{ensuremath{rho}}^{2}}$ is roughly proportional to the magnetostriction ${ensuremath{lambda}}_{s}$ for all fcc Ni-Fe, Cu-Ni, and Cu-Ni-Fe alloys at $Tensuremath{ll}{T}_{c}$, with a slope ensuremath{approx}2.0ifmmodetimeselsetexttimesfi{}${10}^{+9}$ mks." @default.
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• W2019887531 date "1969-09-10" @default.
• W2019887531 modified "2023-09-28" @default.
• W2019887531 title "Galvanomagnetic Effects, Magnetostriction, and Spin-Orbit Interaction in Cu-Ni-Fe and Other Ferromagnetic Nickel Alloys" @default.
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• W2019887531 doi "https://doi.org/10.1103/physrev.185.792" @default.
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