Abstract
The quaternary intermetallic compound superconductor YC with transition temperature K has been investigated by and nuclear magnetic resonance (NMR) and by magnetic susceptibility measurements both in the normal and the superconducting states. The NMR and relaxation measurements have been performed in a powder sample and single crystals. () NMR spectra display patterns typical for an axially symmetric field gradient with quadrupole coupling frequency kHz and () data show spectra typical for a large anisotropic Knight shift, , with axial symmetry (). In the normal state, the increases with decreasing temperature while decreases. The temperature dependences of both the isotropic () and anisotropic () components of the and Knight shifts are presented together with dc magnetic susceptibility () measurements obtained from magnetization measurements and are explained by the sharp features of the density of states near the Fermi level in the system. The analysis of the NMR and data when combined with the theoretical calculation of the Van Vleck contribution to allows the determination of the hyperfine coupling constants for both nuclei investigated and permits the separation of the different contributions to the total measured . The nuclear spin-lattice relaxation rate (NSLR) () results for show an enhancement of when lowering the temperature, consistent with previous results. It is shown that the enhancement of the NSLR is not due to the effects of antiferromagnetic fluctuations of Ni magnetic moments but simply due to the increase of the -band spin susceptibility with decreasing temperature as reflected in the temperature dependence of the Knight shift. Contrary to the case of , the NSLR displays a which is independent of temperature, indicating that the dominant contribution is from a large temperature-independent orbital Knight shift. In the superconducting state, the NSLR drops rapidly without a coherence peak and is found to fit BCS behavior with a superconducting gap parameter at given by .
- Received 20 May 1996
DOI:https://doi.org/10.1103/PhysRevB.54.15341
©1996 American Physical Society