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RESEARCH PRODUCT

Mössbauer-Active Transition Metals Other than Iron

Philipp GütlichEckhard BillAlfred X. Trautwein

subject

chemistryMössbauer effectTransition metalExcited stateMössbauer spectroscopyRadiochemistryAnalytical chemistryTantalumchemistry.chemical_elementIridiumRheniumSpectral line

description

The previous chapters are exclusively devoted to the measurements and interpretation of 57Fe spectra of various iron-containing systems. Iron is, by far, the most extensively explored element in the field of chemistry compared with all other Mossbauer-active elements because the Mossbauer effect of 57Fe is very easy to observe and the spectra are, in general, well resolved and they reflect important information about bonding and structural properties. Besides iron, there are a good number of other transition metals suitable for Mossbauer spectroscopy which is, however, less extensively studied because of technical and/or spectral resolution problems. In recent years, many of these difficulties have been overcome, and we shall see in the following sections a good deal of successful Mossbauer spectroscopy that has been performed on compounds of nickel (61Ni), zinc (67Zn), ruthenium (mainly 99Ru), tantalum (181Ta), tungsten (mainly 182W, 183W), osmium (mainly 189Os), iridium (191Ir, 193Ir), platinum (195Pt), and gold (197Au). The nuclear γ-resonance effect in the case of technetium (99Tc), silver (107Ag), hafnium (176Hf, 177Hf, 178Hf, 180Hf), rhenium (187Re), and mercury (199Hg, 201Hg) has been of relatively little use to the chemists, so far. There are various reasons responsible for this, viz., (1) extraordinary difficulties in measuring the resonance effect because of the long lifetime of the excited Mossbauer level and hence the extremely small transition line width (e.g., in 67Zn), (2) poor resolution of the resonance lines due to either very small nuclear moments or the very short lifetime of the excited Mossbauer level resulting in very broad resonance lines, (3) insufficient resonance effects due to unusually high transition energies between the excited and the ground nuclear levels, which in turn increase the recoil energy and thus reduces the recoilless fraction of emitted and observed γ-rays.

https://doi.org/10.1007/978-3-540-88428-6_7