The role of Ni vacancies on the physical properties of CeNixBi2-y single crystals

International Conference on Strongly Correlated Electron Systems 2014

Rosa, P.F.S.^1,2 ; Jesus, C.B.R.^1 ; Adriano, C.^1 ; Fisk, Z.^2 ; Pagliuso, P.G.^1

Instituto de Física gleb Wataghin, UNICAMP, Campinas-SP

13083-859, Brazil^1

University of California, Irvine

CA

92697-4574, United States^2

关键词: Antiferromagnetic transition temperature;    Conduction electrons;    Crystal fields;    Energy dispersive x-ray spectroscopy analysis;    Exciting field;    Low temperatures;    Magnetic frustrations;    New superconductor;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/592/1/012063/pdf
DOI  :  10.1088/1742-6596/592/1/012063

来源: IOP

【 摘 要 】

The search for new superconductors (SC) represents an exciting field in condensed matter physics. Recently, CeNi0.8Bi2has been reported as a new bulk SC (Tc∼ 4.2 K) in which Ni vacancies play an essential role for the emergence of superconductivity. Here we report experiments of magnetic susceptibility and heat capacity combined with energy dispersive X- ray spectroscopy analysis on CeNixBi2-y(x 0.62, 0.70, 0.74, 0.78) single crystals. Our data show a systematic enhancement of the antiferromagnetic transition temperature (TN) with x, as well as the low temperature Ce3+magnetic anisotropy. In particular, we find that the crystal- field ground state doublet becomes more isolated from the excited states as one approaches the Ni-rich end. As a consequence of such subtle crystal-field evolution, our analyses suggest that both the magnetic frustration and the hybridization between Ce3+4f and conduction electrons are decreasing along the series. In addition, SC transitions are observed in both La and Ce members with no bulk signature, strongly indicating the presence of impurity SC phases.