2019
DOI: 10.3390/ma12223702
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Statistical Thermodynamics of Chiral Skyrmions in a Ferromagnetic Material

Abstract: Solitons are a challenging topic in condensed matter physics and materials science because of the interplay between their topological and physical properties and for the crucial role they play in topological phase transitions. Among them, chiral skyrmions hosted in ferromagnetic systems are axisymmetric solitonic states attracting a lot of attention for their dazzling physical properties and technological applications. In this paper, the equilibrium statistical thermodynamics of chiral magnetic skyrmions devel… Show more

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Cited by 9 publications
(15 citation statements)
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“…In this section, the main results of this work applied to an outwardly Néel skyrmion hosted in a Co dot of radius R d = 200 nm and t = 0.8 nm having the core magnetization m z (r = 0) = −1 (S = −1) and H ext applied along + z are discussed. The magnetic parameters are the ones used in the analytical and numerical calculations in [13,14]. In particular, the following magnetic parameters at T = 0 K were used: saturation magnetization M s = 600 KA/m, exchange stiffness constant A = 20 pJ/m, IDMI parameter D = 3.0 mJ/m 2 , K u = 0.6 MJ/m 3 (for example, Co).…”
Section: Resultsmentioning
confidence: 99%
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“…In this section, the main results of this work applied to an outwardly Néel skyrmion hosted in a Co dot of radius R d = 200 nm and t = 0.8 nm having the core magnetization m z (r = 0) = −1 (S = −1) and H ext applied along + z are discussed. The magnetic parameters are the ones used in the analytical and numerical calculations in [13,14]. In particular, the following magnetic parameters at T = 0 K were used: saturation magnetization M s = 600 KA/m, exchange stiffness constant A = 20 pJ/m, IDMI parameter D = 3.0 mJ/m 2 , K u = 0.6 MJ/m 3 (for example, Co).…”
Section: Resultsmentioning
confidence: 99%
“…The magnetic parameters A, D and K u at non-zero temperature are scaled from their zero temperature values, by using the scaling laws A(m) = A (T = 0 K) m (T) 3/2 , D (T) = D(T = 0 K) m(T) 3/2 , and K u (T) = K u (T = 0 K) m(T) 3.6 [15]. In Table 1 are summarized the values of a and of D 0sky used in the numerical calculations [13,14]. Table 1 does not contain the values of a and D 0sky at T = 0 K since the shown calculations are for T ≥ 50 K. Table 1.…”
Section: Resultsmentioning
confidence: 99%
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