Temperature dependences of the interlayer exchange constant of three-layer FeNi/Dy/FeNi films studied by the resonance method
Vazhenina I.G. 1, Stolyar S.V. 2,3, Yakovchuk V.Y. 1, Rautskii M.V. 1, Iskhakov R.S. 1
1Kirensky Institute of Physics, Federal Research Center KSC SB, Russian Academy of Sciences, Krasnoyarsk, Russia
2Krasnoyarsk Scientific Center of the Siberian Branch of the Russian Academy of Sciences, Krasnoyarsk, Russia
3Siberian Federal University, Krasnoyarsk, Russia
Email: irina-vazhenina@mail.ru, stol@iph.krasn.ru, avay_08@mail.ru, rmv@iph.krasn.ru, rauf@iph.krasn.ru

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Three-layer FeNi/Dy/FeNi films were studied by ferromagnetic resonance method in the temperature range from 4 to 300 K. The acoustic and optical peaks recorded in microwave spectra demonstrate the presence of exchange coupling between the ferromagnetic FeNi layers of the planar system and allow us to establish the sign and value of the constant of the interlayer exchange interaction. Temperature dependences of the interlayer exchange interaction constant for three-layer films with intermediate layer thicknesses Dy 5 and 10 nm show a number of features (change in sign and extremum point), which reflect transformations of the magnetic structure Dy. Keywords: interlayer exchange coupling, helical magnetic structure, ferromagnetic resonance, three-layer films.
  1. P. Grunberg, R. Schreiber, Y. Pang, M.B. Brodsky, H. Sowers, Phys. Rev. Lett., 57, 2442 (1986). DOI: 10.1103/PhysRevLett.57.2442
  2. A.B. Rinkevich, Ya.A. Pakhomov, E.A. Kuznetsov, A.S. Klepikova, M.A. Milyaev, L.I. Naumova, V.V. Ustinov, Tech. Phys. Lett., 45 (3), 225 (2019). DOI: 10.1134/S1063785019030143
  3. Z. Zhang, L. Zhou, P.E. Wigen, K. Ounadjela, Phys. Rev. B, 50, 6094 (1994). DOI: 10.1103/PhysRevB.50.6094
  4. Z. Celinski, B. Heinrich, J. Magn. Magn. Mater., 99, L25 (1991). DOI: 10.1016/0304-8853(91)90043-A
  5. R.S. Iskhakov, S.V. Stolyar, L.A. Chekanova, V.Yu. Yakovchuk, M.V. Chizhik, Bull. Russ. Acad. Sci. Phys., 75 (2), 181 (2011). DOI: 10.3103/S1062873811020134
  6. B. Khodadadi, J.B. Mohammadi, J.M. Jones, A. Srivastava, C. Mewes, T. Mewes, C. Kaiser, Phys. Rev. Appl., 8, 014024 (2017). DOI: 10.1103/PhysRevApplied.8.014024
  7. R. Herz, H. Kronmuller, J. Magn. Magn. Mater., 9, 273 (1978). DOI: 10.1016/0304-8853(78)90069-0
  8. K. Dumesnil, C. Dufour, P. Mangin, G. Marchal, M. Hennion, Phys. Rev. B, 54, 6407 (1996). DOI: 10.1103/PhysRevB.54.6407
  9. S.V. Stolyar, V.Y. Yakovchuk, I.G. Vazhenina, R.S. Iskhakov, J. Supercond. Nov. Magn., 34, 2969 (2021). DOI: 10.1007/s10948-021-06001-x
  10. A. Layadi, J.O. Artman, J. Magn. Magn. Mater., 92, 143 (1990). DOI: 10.1016/0304-8853(90)90691-I
  11. P.J.H. Bloemen, H.W. van Kesteren, H.J.M. Swagten, W.J.M. de Jonge, Phys. Rev. B, 50, 13505 (1994). DOI: 10.1103/PhysRevB.50.13505
  12. Y. Ando, H. Koizumi, T. Miyazaki, J. Magn. Magn. Mater., 166, 75 (1997). DOI: 10.1016/S0304-8853(96)00413-1
  13. B. Heinrich, J.F. Cochran, M. Kowalewski, J. Kirschner, Z. Celinski, A.S. Arrott, K. Myrtle, Phys. Rev. B, 44, 9348 (1991). DOI: 10.1103/PhysRevB.44.9348
  14. E.E. Fullerton, D. Stoeffler, K. Ounadjela, B. Heinrich, Z. Celinski, J.A.C. Bland, Phys. Rev. B, 51, 6364 (1995). DOI: 10.1103/PhysRevB.51.6364
  15. V. Drchal, J. Kudrnovsky, P. Bruno, I. Turek, P.H. Dederichs, P. Weinberger, Phys. Rev. B, 60, 9588 (1999). DOI: 10.1103/PhysRevB.60.9588
  16. S. Schwieger, W. Nolting, Phys. Rev. B, 69, 224413 (2004). DOI: 10.1103/PhysRevB.69.224413
  17. W. Wang, P. Li, C. Cao, F. Liu, R. Tang, G. Chai, C. Jiang, Appl. Phys. Lett., 113, 042401 (2018). DOI: 10.1063/1.5040666
  18. T. McKinnon, B. Heinrich, E. Girt, Phys. Rev. B, 104, 024422 (2021). DOI: 10.1103/PhysRevB.104.024422
  19. R.E. Camley, R.L. Stamps, J. Phys.: Condens. Matter., 5, 3727 (1993). DOI: 10.1088/0953-8984/5/23/003
  20. I.E. Dzialoshinskii, JETP, 5 (6) 1259 (1957)
  21. T. Moriya, Phys. Rev., 120, 91 (1960). DOI: 10.1103/PhysRev.120.91
  22. K. Chen, A. Philippi-Kobs, V. Lauter, A. Vorobiev, E. Dyadkina, V.Y. Yakovchuk, S.V. Stolyar, D. Lott, Phys. Rev. Appl., 12, 024047 (2019). DOI: 10.1103/PhysRevApplied.12.024047

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