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Phys. Rev. B 77, 134520 (2008) [6 pages]

Direct observation of a Fermi surface and superconducting gap in LuNi2B2C

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P. Starowicz1,2, C. Liu1, R. Khasanov1,3, T. Kondo1, G. Samolyuk1, D. Gardenghi1,4, Y. Lee1, T. Ohta5, B. Harmon1, P. Canfield1, S. Bud’ko1, E. Rotenberg5, and A. Kaminski1
1Ames Laboratory and Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA
2M. Smoluchowski Institute of Physics, Jagiellonian University, Reymonta 4, 30-059 Kraków, Poland
3Physik-Institut der Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland
4Bob Jones University, Greenville, South Carolina 29614, USA
5Advanced Light Source, Berkeley National Laboratory, Berkeley, California 94720, USA

Received 29 January 2008; published 30 April 2008

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 μ, which originates from thermally excited electrons above the energy of 2Δ. This feature was not previously observed in the Lu-based material.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.77.134520
DOI:
10.1103/PhysRevB.77.134520
PACS:
74.70.Dd, 71.18.+y, 71.20.−b