Modeling longitudinal spin fluctuations in chiral magnets.

作者: A M Belemuk , S M Stishov

DOI: 10.1088/1361-648X/AB00B7

关键词: Phase transitionMagnetCondensed matter physicsSpecific heatHamiltonian (quantum mechanics)AmplitudePhysicsMonte Carlo method

摘要: We investigate the effect of evolution energy longitudinal spin fluctuations on helimagnetic transition and specific heat in a Heisenberg magnet with Dzyaloshinskii-Moriya interaction that may arise result applied pressure. Using classical Monte Carlo calculations for spin-lattice Hamiltonian accounting variable amplitudes we find helical phase is pretty robust against fluctuations. At same time amplitude fluctuation hump seen dependence at [Formula: see text] its position are significantly affected. Depending mode either shifts to lower or higher temperatures increasing

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