Direct observation of a Fermi surface and superconducting gap in LuNi2B2C

被引:13
作者
Starowicz, P. [1 ,2 ,3 ]
Liu, C. [1 ,2 ]
Khasanov, R. [1 ,2 ,4 ]
Kondo, T. [1 ,2 ]
Samolyuk, G. [1 ,2 ]
Gardenghi, D. [1 ,2 ,5 ]
Lee, Y. [1 ,2 ]
Ohta, T. [6 ]
Harmon, B. [1 ,2 ]
Canfield, P. [1 ,2 ]
Bud'ko, S. [1 ,2 ]
Rotenberg, E.
Kaminski, A. [1 ,2 ]
机构
[1] Iowa State Univ, Ames Lab, Ames, IA 50011 USA
[2] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA
[3] Jagiellonian Univ, M Smoluchowski Inst Phys, PL-30059 Krakow, Poland
[4] Univ Zurich, Inst Phys, CH-8057 Zurich, Switzerland
[5] Bob Jones Univ, Greenville, SC 29614 USA
[6] Berkeley Natl Lab, Berkeley, CA 94720 USA
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevB.77.134520
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
We measured the Fermi surface (FS), band dispersion, and superconducting gap in LuNi2B2C using angle resolved photoemission spectroscopy. Experimental data were compared to the tight-binding version of the linear muffin-tin orbital (LMTO) method and linearized augmented plane-wave (LAPW) calculations. We found reasonable agreement between the two calculations and experimental data. The measured FS exhibits large parallel regions with a nesting vector that agrees with a previous positron annihilation study and calculations of the generalized susceptibility. The measured dispersion curves also agree reasonably well with the TB-LMTO calculations, although with some differences in the strength of the hybridization. In addition, the spectrum in the superconducting state revealed a 2 meV superconducting gap. The data also clearly show the presence of a coherent peak above the chemical potential mu, which originates from thermally excited electrons above the energy of 2 Delta. This feature was not previously observed in the Lu-based material.
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页数:6
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