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Название: Dark Discrete Breather Modes in a Monoaxial Chiral Helimagnet with Easy-plane Anisotropy
Авторы: Bostrem, I. G.
Ekomasov, E. G.
Kishine, J.
Ovchinnikov, A. S.
Sinitsyn, V. E.
Дата публикации: 2021
Издатель: American Physical Society
American Physical Society (APS)
Библиографическое описание: Dark Discrete Breather Modes in a Monoaxial Chiral Helimagnet with Easy-plane Anisotropy / I. G. Bostrem, E. G. Ekomasov, J. Kishine et al. // Physical Review B. — 2021. — Vol. 104. — Iss. 21. — 214420.
Аннотация: Nonlinearity and discreteness are two pivotal factors for an emergence of discrete breather excitations in various media. We argue that these requirements are met in the forced ferromagnetic phase of the monoaxial chiral helimagnet CrNb3S6 due to the specific domain structure of the compound. The stationary, time-periodic breather modes appear as the discrete breather lattice solutions whose period mismatches with a system size. Thanks to easy-plane single-ion anisotropy intrinsic to CrNb3S6, these modes are of the dark type with frequencies lying within the linear spin-wave band, close to its bottom edge. They represent cnoidal states of magnetization, similar to the well-known soliton lattice ground state, with differing but limited number of embedded 2π kinks. The linear stability of these dark breather modes is verified by means of Floquet analysis. Their energy, which is controlled by two parameters, namely, the breather lattice period and amplitude, falls off linearly with a growth of the kink number. These results may pave a path to design spintronic resonators on the base of chiral helimagnets. © 2021 American Physical Society.
Ключевые слова: ANISOTROPY
GROUND STATE
NIOBIUM COMPOUNDS
SPIN WAVES
SULFUR COMPOUNDS
DISCRETE BREATHER
DOMAIN STRUCTURE
EASY PLANE
EASY-PLANE ANISOTROPY
FERROMAGNETIC PHASIS
LINEAR STABILITY
SINGLE ION ANISOTROPY
SOLITON LATTICE
SYSTEM SIZE
WAVEBANDS
CHROMIUM COMPOUNDS
URI: http://elar.urfu.ru/handle/10995/111432
Условия доступа: info:eu-repo/semantics/openAccess
Идентификатор РИНЦ: 47547626
Идентификатор SCOPUS: 85122023731
Идентификатор WOS: 000753810400006
Идентификатор PURE: 29207430
ISSN: 2469-9950
DOI: 10.1103/PhysRevB.104.214420
Сведения о поддержке: This work was supported by the Act of the Government of the Russian Federation (Contract No. 02.A03.21.0006). I.G.B., E.G.E., and V.E.S. acknowledge financial support by the Russian Foundation for Basic Research (RFBR), Grant No. 20-02-00213. A.S.O. thanks the Russian Foundation for Basic Research (RFBR), Grant No. 20-52-50005, and the Ministry of Science and Higher Education of the Russian Federation, Project No. FEUZ-2020-0054. J.K. acknowledges financial support by JSPS KAKENHI Grant No. 17H02923.
Располагается в коллекциях:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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