Constrained Monte Carlo method and calculation of the temperature dependence of magnetic anisotropy

P. Asselin, R. F. L. Evans, J. Barker, R. W. Chantrell, R. Yanes, O. Chubykalo-Fesenko, D. Hinzke, and U. Nowak
Phys. Rev. B 82, 054415 – Published 11 August 2010

Abstract

We introduce a constrained Monte Carlo method which allows us to traverse the phase space of a classical spin system while fixing the magnetization direction. Subsequently we show the method’s capability to model the temperature dependence of magnetic anisotropy, and for bulk uniaxial and cubic anisotropies we recover the low-temperature Callen-Callen power laws in M. We also calculate the temperature scaling of the two-ion anisotropy in L10 FePt, and recover the experimentally observed M2.1 scaling. The method is newly applied to evaluate the temperature-dependent effective anisotropy in the presence of the Néel surface anisotropy in thin films with different easy-axis configurations. In systems having different surface and bulk easy axes, we show the capability to model the temperature-induced reorientation transition. The intrinsic surface anisotropy is found to follow a linear temperature behavior in a large range of temperatures.

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  • Received 31 May 2010

DOI:https://doi.org/10.1103/PhysRevB.82.054415

©2010 American Physical Society

Authors & Affiliations

P. Asselin

  • Seagate Technology, Bloomington, Minnesota 55435, USA

R. F. L. Evans*, J. Barker, and R. W. Chantrell

  • Department of Physics, University of York, Heslington, York YO10 5DD, United Kingdom

R. Yanes and O. Chubykalo-Fesenko

  • Instituto de Ciencia de Materiales de Madrid, CSIC, Cantoblanco, Madrid 28049, Spain

D. Hinzke and U. Nowak

  • Universitat Konstanz, Fachbereich Physik, Universitätsstraße 10, D-78464 Konstanz, Germany

  • *rfle500@york.ac.uk

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Issue

Vol. 82, Iss. 5 — 1 August 2010

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