Detailed Monte Carlo simulations of Ho magnetic thin films are here presented. The system is described by a Heisenberg model with easy-plane single-ion anisotropy and seven coupling constants, as obtained by experimental neutron scattering measurements. The critical behavior landscape comes out extremely complex and fascinating. In fact, for the analyzed thicknesses of 8-16, it is seen that by increasing the temperature the films show, after the distorted helical configuration, a temperature range where disordered inner planes coexist with surface ones in a block ordered state. At low temperature, it is also found that the progressive reduction in the number of layers do not imply a sudden helical order suppression but rather, as a consequence of surface effects, a gradual passage to a fanlike order, accompanied by the helix distortion, is observed. (C) 2009 American Institute of Physics.
Magnetic phases in ultrathin helimagnetic holmium films / F. Cinti; A. Cuccoli; A. Rettori. - In: JOURNAL OF APPLIED PHYSICS. - ISSN 0021-8979. - STAMPA. - 105:(2009), pp. 07E117-1-07E117-3. [10.1063/1.3068482]
Magnetic phases in ultrathin helimagnetic holmium films
CINTI, FABIO;CUCCOLI, ALESSANDRO;RETTORI, ANGELO
2009
Abstract
Detailed Monte Carlo simulations of Ho magnetic thin films are here presented. The system is described by a Heisenberg model with easy-plane single-ion anisotropy and seven coupling constants, as obtained by experimental neutron scattering measurements. The critical behavior landscape comes out extremely complex and fascinating. In fact, for the analyzed thicknesses of 8-16, it is seen that by increasing the temperature the films show, after the distorted helical configuration, a temperature range where disordered inner planes coexist with surface ones in a block ordered state. At low temperature, it is also found that the progressive reduction in the number of layers do not imply a sudden helical order suppression but rather, as a consequence of surface effects, a gradual passage to a fanlike order, accompanied by the helix distortion, is observed. (C) 2009 American Institute of Physics.File | Dimensione | Formato | |
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