Motivated by recent experimental results in ultrathin helimagnetic holmium films, we have performed an extensive classical Monte Carlo simulation of films of different thickness, assuming a Hamiltonian with six interlayer exchange constants. Both magnetic structure and critical properties have been analyzed. For n>16, n being the number of spin layers in the film, a correct bulk limit is reached, while for lower n the film properties are clearly affected by the strong competition among the helical pitch and the surface effects, which involve the majority of the spin layers. In the thickness range n=9−16 three different magnetic phases emerge, with the high-temperature, disordered, paramagnetic phase and the low-temperature, long-range ordered one separated by an intriguing intermediate-temperature block phase, where outer ordered layers coexist with some inner disordered ones. The phase transition of these inner layers displays the signatures of a Kosterlitz- Thouless one. Finally, for n<=7 the film collapses once and for all to a quasicollinear order. A comparison of our Monte Carlo simulation outcomes to available experimental data is also proposed and further experimental investigations are suggested.
Monte Carlo simulations of rare-earth holmium ultrathin films / F. Cinti; A. Cuccoli; A. Rettori. - In: PHYSICAL REVIEW. B, CONDENSED MATTER AND MATERIALS PHYSICS. - ISSN 1098-0121. - STAMPA. - 79:(2009), pp. 134420:1-134420:11. [10.1103/PhysRevB.79.134420]
Monte Carlo simulations of rare-earth holmium ultrathin films
CINTI, FABIO;CUCCOLI, ALESSANDRO;RETTORI, ANGELO
2009
Abstract
Motivated by recent experimental results in ultrathin helimagnetic holmium films, we have performed an extensive classical Monte Carlo simulation of films of different thickness, assuming a Hamiltonian with six interlayer exchange constants. Both magnetic structure and critical properties have been analyzed. For n>16, n being the number of spin layers in the film, a correct bulk limit is reached, while for lower n the film properties are clearly affected by the strong competition among the helical pitch and the surface effects, which involve the majority of the spin layers. In the thickness range n=9−16 three different magnetic phases emerge, with the high-temperature, disordered, paramagnetic phase and the low-temperature, long-range ordered one separated by an intriguing intermediate-temperature block phase, where outer ordered layers coexist with some inner disordered ones. The phase transition of these inner layers displays the signatures of a Kosterlitz- Thouless one. Finally, for n<=7 the film collapses once and for all to a quasicollinear order. A comparison of our Monte Carlo simulation outcomes to available experimental data is also proposed and further experimental investigations are suggested.File | Dimensione | Formato | |
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