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- W1636762458 abstract "The classical equation of motion for the magnetic moment vector in a thin magnetic film has been solved numerically for perpendicular (H⊥film) resonance for the conditions that (1) the static magnetization was spatially dependent and (2) the damping could be neglected. This solution was used to elucidate SWR data obtained on a single crystal YIG film on GGG at 9.2 GHz. The experimentally observed data was obtained at 77°K on a 0.37 μm film ([100]⊥film) for which 4πMs = 2350 Oe, 2A/Ms = 5.4 × 10−9 Oe ‐ CM2 and g = 2.025. The best agreement between the theoretically generated spectra and the experimental data was obtained by assuming variation of the static magnetization near the GGG interface. The relative field intensities were conputed and both even and odd modes were found to be present in agreement with experimental results. The intensities for the first four modes were found to vary approximately as 1/n2. Thus, it appears that it is essential to assume a variation of the static magnetization of the YIG‐GGG interface to explain the spin‐wave excitations in YIG films." @default.
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- W1636762458 date "1973-01-01" @default.
- W1636762458 modified "2023-09-26" @default.
- W1636762458 title "Physical Model for Spin-Wave Excitations in YIG Films" @default.
- W1636762458 doi "https://doi.org/10.1063/1.2946828" @default.
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