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arXiv · 1211.5967

Local Structure and Hyperfine Interactions of 57Fe in NaFeAs Studied by Mossbauer Spectroscopy

Igor Presniakov·Igor Morozov·Alexey Sobolev·Maria Roslova·Alexander Boltalin·Vladimir Son·Olga Volkova·Alexander Vasiliev·Sabine Wurmehl·Bernd Büchner
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Abstract

Detailed 57Fe Mossbauer spectroscopy measurements on superconducting NaFeAs powder samples have been performed in the temperature range 13 K < T < 300 K. The 57Fe spectra recorded in the paramagnetic range (T > TN ~ 46 K) were discussed supposing that most of the Fe2+ ions are located in distorted (FeAs4) tetrahedral of NaFeAs phase, while additional minor (< 10%) component of the spectra corresponds to impurity or intergrowth NaFe2As2 phase with a nominal composition near "NaFe2As2". Our results reveal that the structural transition (TS ~ 55K) has a weak effect on the electronic structure of iron ions, while at T < TN the spectra show a continuous distribution of hyperfine fields HFe . Shape of these spectra was analyzed in term of two models: (i) an incommensurate spin density wave modulation of iron magnetic structure, (ii) a formation of a microdomain structure or phase separation. It was shown that the hyperfine parameters obtained using these two methods have very similar values over the whole temperature range. The analysis of the temperature dependence HFe(T) with the Bean-Rodbell model leads to ksi = 1.16 +/- 0.05, suggesting that the magnetic phase transition is first-order in nature. A sharp evolution of the VZZ(T) and etha(T) parameters of the full Hamiltonian of hyperfine interactions near T ~ (TN, TS), were interpreted as a manifestation of the anisotropic electron redistribution between the dxz, dyz- and dxy-orbitals of the iron ions.

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Igor Presniakov, Igor Morozov, Alexey Sobolev, Maria Roslova, Alexander Boltalin, Vladimir Son, Olga Volkova, Alexander Vasiliev, Sabine Wurmehl, Bernd Büchner. 2013-02-28. Local Structure and Hyperfine Interactions of 57Fe in NaFeAs Studied by Mossbauer Spectroscopy. https://doi.org/10.1088/0953-8984%2F25%2F34%2F346003

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