In charge uncompensated CaX:YIG, magnetic anomalies and a photoinduced absorption spectrum have been reported. The temperature dependence of the photoinduced peak observed at 1.85 eV (width 0.5 eV) has the same temperature dependence as the low‐temperature anomalies observed in the magnetizations. A model to explain the low‐temperature magnetic anomaly assumes that a non‐S state iron ion, Fe4+, is created in the tetrahedral site that is ferromagnetically coupled to the octahedral Fe3+ ion. An alternative model recently proposed assumes that O− ions are formed which would influence the magnetic properties in similar fashion. The broad nature of the absorption at 1.85 eV is characteristic of a resonant transition of photocarriers. In this paper the absorption band is discussed in terms of a polaron hopping model.
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15 November 1991
The 5th Joint MMM−Intermag Conference
18−21 Jun 1991
Pittsburgh, Pennsylvania (USA)
Research Article|
November 15 1991
Polaronic absorption in uncompensated CaX:YIG Available to Purchase
A. Thavendrarajah;
A. Thavendrarajah
Department of Physics, The Ohio State University, Columbus, Ohio 43210
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Y. Song;
Y. Song
Department of Physics, The Ohio State University, Columbus, Ohio 43210
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P. E. Wigen
P. E. Wigen
Department of Physics, The Ohio State University, Columbus, Ohio 43210
Search for other works by this author on:
A. Thavendrarajah
Department of Physics, The Ohio State University, Columbus, Ohio 43210
Y. Song
Department of Physics, The Ohio State University, Columbus, Ohio 43210
P. E. Wigen
Department of Physics, The Ohio State University, Columbus, Ohio 43210
J. Appl. Phys. 70, 6389–6391 (1991)
Citation
A. Thavendrarajah, Y. Song, P. E. Wigen; Polaronic absorption in uncompensated CaX:YIG. J. Appl. Phys. 15 November 1991; 70 (10): 6389–6391. https://doi.org/10.1063/1.349952
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