2014
DOI: 10.22226/2410-3535-2014-4-237-240
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Numerical simulation of the generation of multisoliton type magnetic inhomogeneities in ferromagnets with inhomogeneous parameters

Abstract: The generation and evolution of multisoliton type magnetic inhomogeneities, which appear in two flat layers with the magnetic anisotropy that are different from those in three thick layers after pinning a 180° domain wall, have been investigated theoretically. The structure of the multisoliton type magnetic inhomogeneities have been constructed for the revealed magnetic inhomogeneities, and the ranges of the parameters determining the possibility of their existence have been found.

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Cited by 4 publications
(6 citation statements)
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“…As has been shown before, at the scattering of a DW by a defect a part of its energy is expended on the excitation of a nonlinear magnetization wave localized in the defect region, or a «magnetic breather» (if the DW leaves the defect) [21,33,34]. Moreover, the magnitude of this energy can vary depending on the initial velocity of the DW υ 0 .…”
Section: Dynamics Of Nonlinear Waves Localized In the Defect Regionmentioning
confidence: 91%
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“…As has been shown before, at the scattering of a DW by a defect a part of its energy is expended on the excitation of a nonlinear magnetization wave localized in the defect region, or a «magnetic breather» (if the DW leaves the defect) [21,33,34]. Moreover, the magnitude of this energy can vary depending on the initial velocity of the DW υ 0 .…”
Section: Dynamics Of Nonlinear Waves Localized In the Defect Regionmentioning
confidence: 91%
“…Due to the complexity of the problem, the researchers considered, as a rule, the modulation of only certain magnetic system parameters. For instance, they often took into account the magnetic anisotropy modulation both for the case of point and extended defects [21,33]. It is shown that when a DW passes through a thin magnetic layer with a lower anisotropy value, high-amplitude localized nonlinear waves of magnetization can arise in it [19,33,34].…”
Section: Introductionmentioning
confidence: 99%
“…Обычно, при решении динамических задач, удобно перейти к сферическим координатам вектора намагни-ченности M(cos φ sinθ, sin φ, cos φ cos θ), где 0 ≤ θ ≤ 2π -угол в плоскости yz между направлением вектора маг-нитного момента и осью лёгкого намагничивания (ось Oz), -π /2 < φ < π/2 -угол, описывающий выход M из плоскости доменной границы (ДГ). Учитывая в плотно-сти энергии магнетика обменное взаимодействие и ани-зотропию, и считая φ << 1 [1], уравнение движения для намагниченности в угловых переменных можно пред-ставить в следующем обезразмеренном виде [12]:…”
Section: основные уравнения и результатыunclassified
“…Будем считать, что ε << 1, а слагаемые в правой части уравнения (1) малы. Применим приближенный коллективно-координатный подход, использованный ранее для анализа колебаний локализованных нели-нейных волн намагниченности на одиночном точечном дефекте [12]. Учитываем наличие локализованных волн намагниченности в области дефекта (или примесных мод) с помощью введения двух коллективных перемен-ных -a 1 = a 1 (t) и a 2 = a 2 (t) -являющихся амплитудами этих волн.…”
Section: основные уравнения и результатыunclassified
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