X-ray-absorption fine-structure study of the A15 superconductors Nb3(Sn,Sb)

J. B. Boyce, F. Bridges, T. Claeson, T. H. Geballe, G. W. Hull, N. Kitamura, and F. Weiss
Phys. Rev. B 37, 54 – Published 1 January 1988
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Abstract

X-ray-absorption fine-structure measurements at the Sn and Sb K edges were made on Nb3Sn, Nb3Sb, and Nb3Sn1xSbx alloys. No temperature-dependent anomalies were noted for the Sn-Nb and Sb-Nb distances or for the broadening in these distances for temperatures from 4.2 K to well above the transition temperatures. The temperature dependence of the broadenings fits an Einstein oscillator model well, with Einstein temperatures of 237 K for Nb3Sn and 254 K for Nb3Sb. These results also agree with recent theoretical calculations. The Debye-Wallertype broadening in the Sn-Nb and Sb-Nb distances for the alloys are not equal to one another, but instead are nearly equal to those of the binary end-point compounds, i.e., to Nb3Sn and Nb3Sb, respectively.

  • Received 6 July 1987

DOI:https://doi.org/10.1103/PhysRevB.37.54

©1988 American Physical Society

Authors & Affiliations

J. B. Boyce

  • Xerox Corporation, Palo Alto Research Center, Palo Alto, California 94304

F. Bridges

  • Physics Department, University of CaliforniaSanta Cruz, Santa Cruz, California 95064

T. Claeson

  • Physics Department, Chalmers University of Technology, S-412 96 Göteborg, Sweden

T. H. Geballe

  • Applied Physics Department, Stanford University, Stanford, California 94305

G. W. Hull

  • Bell Communications Research, Red Bank, New Jersey 07701-7020

N. Kitamura

  • Aoyama Gakuin University, 6-16-1 Chitosedai, Setagaya-ku, Tokyo 157, Japan

F. Weiss

  • Laboratoire des Matériaux et du Génie Physique, 38402 Saint-Martin-d’Hères, France

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Vol. 37, Iss. 1 — 1 January 1988

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