Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-25T17:29:11.892Z Has data issue: false hasContentIssue false
  • English
  • Français

Magneto-Optical Properties of Co Doped Bi3Fe5O12 Garnet Film

Published online by Cambridge University Press:  10 February 2011

T. Okuda ,
T. Mima ,
K. Ando ,
N. Ohmori ,
N. Adachi  and
H. Ohsato
T. Okuda
Affiliation:
Nagoya Inst. of Tech., Nagoya, 466-8555Japan, [email protected]
T. Mima
Affiliation:
Nagoya Inst. of Tech., Nagoya, 466-8555Japan, [email protected]
K. Ando
Affiliation:
Electrotechnical Laboratory, Tsukuba-shi 305-, Japan
N. Ohmori
Affiliation:
Nagoya Inst. of Tech., Nagoya, 466-8555Japan, [email protected]
N. Adachi
Affiliation:
Nagoya Inst. of Tech., Nagoya, 466-8555Japan, [email protected]
H. Ohsato
Affiliation:
Nagoya Inst. of Tech., Nagoya, 466-8555Japan, [email protected]
Get access

Abstract

Co-doped Bi3Fe5O12 garnet (BIG) films were prepared on Gd3(ScGa)5O12(GSGG) substrates using two types of ion-beam-sputtering (IBS) technique. In the films deposited by sputtering the Co and the BIG source targets alternately with short periodicity, the interface exchange coupling of BIG and Co-spinel ferrite was characteristically observed in the Faraday hysteresis loop. The magnetic and the Faraday hysteresis loops were found to have different coercivity. In the films deposited by conventional IBS method using the BIG target doubly substituted by Co and Ge, Co2+ ions were highly replaced up to 0.7 atoms/formula unit for Fe3+ in BIG. The specific Faraday rotation angle (θ F) at a wavelength of 1.5 μ m was 1.1 deg/μm/Co atom. The magnetic easy direction was normal to the film plane.

Type
Research Article
Information
MRS Online Proceedings Library (OPL) , Volume 517: Symposium F – Wide Bandgap Semiconductors for High Power, High Frequency , January 1998 , 493
Copyright
Copyright © Materials Research Society 1998

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1. Wood, D.L. and Remeika, J.P., J.Chem.Phys. 46, 3595(1967).Google Scholar
2. Egashira, K. and Manabe, T., IEEE Trans. Magn. MAG–8, 646(1972).10.1109/TMAG.1972.1067450Google Scholar
3. Ahrenkiel, R.K., Lee, T.H., Lyu, S.L., and Moser, F., Solid State Comm. 12, 1113 (1973).10.1016/0038-1098(73)90124-5Google Scholar
4. Okuda, T., Katayama, T., Kobayashi, H., Kobayashi, N., Satoh, K., and Yamamoto, H., J. Appl. Phys. 67, 4944(1990).Google Scholar
5. Okuda, T., Katoh, Y., Ohsato, H., Adachi, N., Ando, K., Abe, T. and Yamamoto, H., J. Magnetism and Magnetic Mat. 148, 275(1995).10.1016/0304-8853(95)00234-0Google Scholar
6. Okuda, T., Adachi, N., Ohsato, H., Katoh, Y. and Mima, T., J.Phys. IV France 7, Colloque C1, Suppl. au J.Phys.III, Cl–711(1997).Google Scholar
7. Mima, T., Okuda, T., Adachi, N. and Ohsato, H., accepted to J. Magnetics Soc. Jpn. (1998).Google Scholar
8. Geller, S., Williams, H.J., Espinosa, G.P., and Sherwood, R.C., Phys. Rev. 136, A1650 (1964).10.1103/PhysRev.136.A1650Google Scholar
9. Gomi, M. and Abe, M., J.Magn.Soc.Jpn. 11, Suppl.No. S1, 309 (1989).Google Scholar