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Title: Superconductivity in the Nb-Ru-Ge σ phase

Journal Article · · Physical Review Materials
 [1];  [2];  [3];  [1];  [3];  [1]
  1. Princeton Univ., Princeton, NJ (United States)
  2. Louisiana State Univ., Baton Rouge, LA (United States)
  3. Gdansk Univ. of Technology, Gdansk (Poland)

Here, we show that the previously unreported ternary σ-phase material Nb20.4Ru5.7Ge3.9 (Nb0.68Ru0.19Ge0.13) is a superconductor with a critical temperature of 2.2 K. Temperature-dependent magnetic susceptibility, resistance, and specific heat measurements were used to characterize the superconducting transition. The Sommerfeld constant γ for Nb20.4Ru5.7Ge3.9 is 91 mJ mol-f.u.-1K-2 (~3 mJ mol-atom-1K-2) and the specific heat anomaly at the superconducting transition, ΔC/γTc, is approximately 1.38. The zero-temperature upper critical field (µ0Hc2(0)) was estimated to be 2 T by resistance data. Field-dependent magnetization data analysis estimated µ0Hc1(0) to be 5.5 mT. Thus, the characterization shows Nb20.4Ru5.7Ge3.9 to be a type II BCS superconductor. This material appears to be the first reported ternary phase in the Nb-Ru-Ge system, and the fact that there are no previously reported binary Nb-Ru, Nb-Ge, or Ru-Ge σ-phases shows that all three elements are necessary to stabilize the material. An analogous σ-phase in the Ta-Ru-Ge system did not display superconductivity above 1.7 K, which suggests that electron count cannot govern the superconductivity observed. Preliminary characterization of a possible superconducting σ-phase in the Nb-Ru-Ga system is also reported.

Research Organization:
Princeton Univ., NJ (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Basic Energy Sciences (BES)
Grant/Contract Number:
FG02-98ER45706
OSTI ID:
1411888
Alternate ID(s):
OSTI ID: 1411803
Journal Information:
Physical Review Materials, Vol. 1, Issue 7; ISSN 2475-9953
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 2 works
Citation information provided by
Web of Science

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