2010
DOI: 10.1016/j.jmmm.2009.10.010
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Spin wave spectrum of magnetic nanotubes

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Cited by 60 publications
(45 citation statements)
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“…The corresponding dispersion relation reads Ω = 1 + µ 2 + R 2 q 2 . Existence of a gap in spectrum of the cylindrical magnetic shell was already predicted theoretically [28] and checked by numerical simulations [29].…”
Section: D Example: Linear Magnetisation Dynamics For a Cone Shellmentioning
confidence: 78%
“…The corresponding dispersion relation reads Ω = 1 + µ 2 + R 2 q 2 . Existence of a gap in spectrum of the cylindrical magnetic shell was already predicted theoretically [28] and checked by numerical simulations [29].…”
Section: D Example: Linear Magnetisation Dynamics For a Cone Shellmentioning
confidence: 78%
“…Figure 3(a) shows the result, which agrees with an analytical calculation. 13 The phase velocity (v p ) of the SWs is then extracted from the dispersion, as shown in Fig. 3(b).…”
Section: à11mentioning
confidence: 99%
“…Therefore, in general case, we have to solve the equation (12) with boundary conditions for the magnetization in order to obtain the dispersion relation. However, we can eliminate the orthogonal wavenumber component from (14) after noting that a typical nanotube thickness has the same order as the characteristic exchange interaction length lex. Therefore, we can consider the case when the "free" layer thickness is less than the exchange length and, therefore, neglect the radial dependence of the magnetic potential: k ⊥ = 0.…”
Section: Dispersion Relation and Condition Of Spin Wave Excitationmentioning
confidence: 99%
“…Therefore, we can consider the case when the "free" layer thickness is less than the exchange length and, therefore, neglect the radial dependence of the magnetic potential: k ⊥ = 0. Thus, we can put n = 0 and transform the equation (14) for k ≠ 0 in the following way:…”
Section: Dispersion Relation and Condition Of Spin Wave Excitationmentioning
confidence: 99%
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