Thermal-Driven Evolution of Magnetic Domain Structures in Ultrathin Films

Article Preview

Abstract:

The thermal-driven evolution of stripe domain structures in ultrathin magnetic films is analyzed with regard to temperature dependencies of the film magnetic parameters. In the vicinity of the Curie temperature or points of the spin reorientation the equilibrium stripe domain period was found to exponentially decrease with increasing temperature. It is shown that the temperature dependence of the characteristic length is the key parameter controlling the domain period changes. Irreversible and reversible changes of the domain period as well as the so-called inverse domain melting are discussed.

You might also be interested in these eBooks

Info:

Periodical:

Solid State Phenomena (Volume 112)

Pages:

101-108

Citation:

Online since:

May 2006

Export:

Price:

Permissions CCC:

Permissions PLS:

Сopyright:

© 2006 Trans Tech Publications Ltd. All Rights Reserved

Share:

Citation:

[1] A. Vaterlaus, C. Stamm, U. Maier, M. G. Pini, P. Politi, and D. Pescia: Phys. Rev. Lett. Vol. 84 (2000), p.2247.

DOI: 10.1103/physrevlett.84.2247

Google Scholar

[2] M. Seul, R. Wolfe: Phys. Rev. Lett. Vol. 68 (1992), p.2460.

Google Scholar

[3] M. Seul, D. Andelman: Science. Vol. 267 (1995), p.476.

Google Scholar

[4] G. J. Kusinski, G. Thomas, G. Denbeaux, K. M. Krishnan and B. D. Terris: J. Appl. Phys. Vol. 91 (2002), p.7541.

Google Scholar

[5] O. Portmann, A. Vaterlaus, and D. Pescia: Nature Vol. 422 (2003), p.701.

Google Scholar

[6] N. Avraham et al.: Nature, Vol. 411 (2001), p.451.

Google Scholar

[7] A. Tarasenko, V. Zablotskii and L. Jastrabik: Europhys. Letters Vol. 62 (2003), p.63.

Google Scholar

[8] A. Maziewski, V. Zablotskii and M. Kisielewski: phys. status solidi (a) Vol. 189 (2002), p.1001.

Google Scholar

[9] H.P. Oepen, M. Speckmann, Y. Millev, and J. Kirschner: Phys. Rev. B Vol. 55 (1997), p.2752.

Google Scholar

[10] Z. Malek and V. Kambersky Czechosl. Journ. Phys.: Vol. 8 (1958), p.416.

Google Scholar

[11] C. Kooy and U. Enz, Phillps: Res. Repts. Vol. 15 (1960), p.7.

Google Scholar

[12] L. Driouch, R. Krishnan, M. Porte, K.V. Rao and M. Tessier: J. Appl. Phys. Vol. 81 (1997), p.4745.

Google Scholar

[13] J. -U. Thiele et al.: J. Appl. Phys. Vol. 91 (2002), p.6595.

Google Scholar

[14] S. Okamoto et al.: Phys. Rev. B Vol. 66 (2002), p.024413.

Google Scholar

[15] J. B. Staunton et al.: Phys. Rev. Lett. Vol. 93 (2004), pp.257204-1.

Google Scholar

[16] A. Enders, D. Peterka, D. Repetto, N. Lin, A. Dmitriev, and K. Kern : Phys. Rev. Lett. Vol. 90 (2003), pp.217203-1.

Google Scholar

[17] C. Kittel : Phys. Rev. Vol. 70 (1946), p.965.

Google Scholar

[18] E.M. Lifshitz, L.P. Pitaevskii, and L.D. Landau : Electrodynamics of Continuous Media (Butterworth-Heinemann Ltd, 1995).

Google Scholar

[19] B. Kaplan and G.A. Gehring: J. Magn. Magn. Mater. Vol. 128 (1993), p.111.

Google Scholar

[20] C. Won, Y. Z. Wu, J. Choi, W. Kim, A. Scholl, A. Doran, T. Owens, J. Wu, X. F. Jin, H. W. Zhao, and Z. Q. Qiu: Phys. Rev. B Vol. 71 (2005), p.224429.

Google Scholar

[21] M. Kisielewski, A. Maziewski, T. Polyakova, and V. Zablotskii: Phys. Rev. B Vol. 69 (2004), p.184419.

Google Scholar

[22] Y. Millev and J. Kirschner: Phys. Rev. B Vol. 54 (1996), p.4137.

Google Scholar

[23] M. Kisielewski, A. Maziewski, V. Zablotskii: J. Magn. Magn. Mater. Vol. 282 (2004), p.39.

Google Scholar

[24] R. P. Erickson and D. L. Mills: Phys. Rev. B Vol. 46 (1992), p.861.

Google Scholar

[25] D. P. Pappas : J. Vac. Sci. Technol. B Vol. 14 (1996), p.3203.

Google Scholar

[26] A. Enders, D. Repetto, D. Peterka, and K. Kern: Phys. Rev. B Vol. 72 (2005), p.054446.

Google Scholar

[27] P. Bruno: Mat. Res. Soc. Symp. Proc. Vol. 231 (1992).

Google Scholar

[11] curve 2, model.

Google Scholar

[19] and curve 3, model [17, 18]. Fig. 2. Equilibrium stripe DS period as a function of temperature changes of the characteristic length (solid line). The dashed line illustrates possible jumps in the domain period changes.

Google Scholar