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Structure, magnetic and electrical properties of CeIrSb and its hydride CeIrSbH0.8
Etienne Gaudin, Bernard Chevalier, Wilfried Hermes, Ute Ch. Rodewald, Rainer Pöttgen

Structure, magnetic and electrical properties of CeIrSb and its hydride CeIrSbH0.8

Science & Mathematics Published 2009 Verification Pending

Overview & Synopsis

The ternary antimonide CeIrSb absorbs hydrogen under moderate temperature and pressure conditions (4 MPa and 573 K), leading to the hydride CeIrSbH0.8. The crystal structures of both compounds have been investigated by X-ray diffraction on powders and single crystals: TiNiSi type, space group Pnma, a=735.07(7), b=456.93(4), c=792.8(1) pm, R1/wR2=0.0206/0.0395, 601 F2 values for CeIrSb and a=728.16(14), b=460.35(6), c=825.87(2) pm, R1/wR2=0.0322/0.0735, 528 F2 values for CeIrSbH0.8 with 20 variables per refinement. Hydrogenation induces both an increase of the cell volume V (+4%) and a strongly anisotropic expansion of the unit cell with a maximum of 4.3% in the c direction, leading to a significant increase of the Ce–Ir and Ce–Ce distances in this direction. The H-insertion into CeIrSb leads to a magnetic transition from intermediate valence to antiferromagnetic behavior (TN=7.0 K) evidenced by magnetization, electrical resistivity and specific heat measurements. This transition can be explained on the basis of the Doniach diagram considering the Jcf interaction between the 4f(Ce) and conduction electrons.

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Document Information

Document Title Structure, magnetic and electrical properties of CeIrSb and its hydride CeIrSbH0.8
Author / Organization Etienne Gaudin, Bernard Chevalier, Wilfried Hermes, Ute Ch. Rodewald, Rainer Pöttgen
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2009
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-182647
Original Source Link Visit Source Page on hal.science »