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Magnetism and electronic structure of the intermetallic compound Ce5CuBi3

We have studied the electronic structure as well as magnetic, electronic transport and thermodynamic properties of the intermetallic compound Ce 5 CuBi 3 . It was found that Ce 5 CuBi 3 undergoes three successive phase transitions at 25 K, 13.7 K and 3.5 K. We attribute the multiple magnetic phase t...

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Bibliographic Details
Published in:Philosophical magazine (Abingdon, England) England), 2007-11, Vol.87 (32), p.5089-5107
Main Authors: Tran, V. H., Gamża, M., Ślebarski, A., Jarmulska, J.
Format: Article
Language:English
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Summary:We have studied the electronic structure as well as magnetic, electronic transport and thermodynamic properties of the intermetallic compound Ce 5 CuBi 3 . It was found that Ce 5 CuBi 3 undergoes three successive phase transitions at 25 K, 13.7 K and 3.5 K. We attribute the multiple magnetic phase transition to be associated with the two non-equivalent magnetic sublattices of the magnetic Ce ions. The investigated compound is characterized by an enhanced ratio C p /T at 2 K, which may be interpreted as being due to the nearness of the 4f-level to the Fermi level and some contribution of magnon excitation. The core-level photoemission spectra indicate that Ce ions in Ce 5 CuBi 3 are very close to trivalent which is consistent with the magnetic susceptibility data. The calculated band structures using the scalar-relativistic linear muffin-tin orbital method in the atomic sphere approximation and the all-electron full potential linear augmented plane wave plus local orbitals method have been performed for the non-magnetic ground state and as well as for collinear ferromagnetic and ferrimagnetic spin alignments. The largest stabilization energy is found in the case of a ferromagnetic structure. The calculated moments on the two sites of the Ce atoms are in agreement with the experimental value (0.93 μ B /Ce). The calculations predict that the studied compound has a pseudogap in the DOS curve. Analysis of the partial DOS suggests some differences in hybridization strengths between the Ce-Bi and Ce-Cu orbitals.
ISSN:1478-6435
1478-6443
DOI:10.1080/14786430701607004