Superconductivity in a low carrier density system: A single crystal study of cubic Y3Ru4Ge13

•Y3Ru4Ge13 is a low carrier density (1020/cm3) semimetal and exhibits bulk superconductivity.•The superconductivity arises due to inter-valley electron-phonon interactions.•Hall coefficient has unusual temperature dependence similar to both High-Tc and layered compounds like MgB2.•These classes of m...

Full description

Saved in:
Bibliographic Details
Published in:Physica. C, Superconductivity Vol. 492; pp. 90 - 95
Main Authors: Prakash, Om, Thamizhavel, A., Nigam, A.K., Ramakrishnan, S.
Format: Journal Article
Language:English
Published: Amsterdam Elsevier B.V 01-09-2013
Elsevier
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:•Y3Ru4Ge13 is a low carrier density (1020/cm3) semimetal and exhibits bulk superconductivity.•The superconductivity arises due to inter-valley electron-phonon interactions.•Hall coefficient has unusual temperature dependence similar to both High-Tc and layered compounds like MgB2.•These classes of materials have good thermoelectric properties.•We need good data on single crystals for further understanding of thermoelectric properties. We have successfully grown the single crystal of a low carrier density system Y3Ru4Ge13 which crystallises in the cubic crystal structure with the space group Pm3n. Y3Ru4Ge13 exhibits superconductivity below 2.85K as determined from the electrical resistivity, magnetic susceptibility and heat capacity measurements. The bulk measurements indicate multi-band superconductivity in this low carrier system. Hall effect measurements show that the Hall coefficient RH is positive and it decreases rapidly with temperature which is highly unusual. The simple estimation of the carrier concentration gives a value (1020/cm3) which is 2–3 orders of magnitude lower than that of a conventional metal like Cu which seems to suggest that Y3Ru4Ge13 is a semimetal that display multiband superconductivity.
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
ISSN:0921-4534
1873-2143
DOI:10.1016/j.physc.2013.05.014