Abstract
The relative line intensities of a magnetic hyperfine spectrum reflect the polarization of emitting and absorbing γ-rays. In resonatly thin absorbers spin orientation can be derived. In very thick samples each polarized line (circular or linear) can absorb by itself only up to one half of the resonant γ-rays from an unpolarized source. For the other half, with opposite helicity or linearity, the material is transparent (dichroism). Two effects in α-Fe will be described:
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1.
When two lines of opposite polarity are in close proximity an apparent line may developin between the actual resonance lines.
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2.
A thick absorber in a transverse magnetic field may exhibit small-but sharp-lines on top of the broad resonance lines.
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References
U. Gonser and H. Fischer: In:Mössbauer Spectroscopy, ed. U. Gonser, Topics Current Phys., Vol. 25 (Springer, Berlin, Heidelberg 1981) p. 99.
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Gonser, U., Aubertin, F., Stenger, S. et al. Polarization and thickness effects in Mössbauer spectroscopy. Hyperfine Interact 67, 701–709 (1991). https://doi.org/10.1007/BF02398222
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DOI: https://doi.org/10.1007/BF02398222