Use of preceramic polymers for magnesium diboride composites

► We used polysiloxane copolymers for improving transport properties of MgB2. ► Polysiloxane-co-vinyl-ferrocene was used to insert magnetic nanoparticles. ► Cyclic polysiloxane-co-styrene leads to the best critical properties. ► Magnetic pinning is visible at high temperatures in samples with ferroc...

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Published inPhysica. C, Superconductivity Vol. 480; pp. 102 - 107
Main Authors Sandu, V., Cimpoiasu, E., Aldica, G., Popa, S., Sandu, E., St. Vasile, B., Hurduc, N., Nor, I.
Format Journal Article
LanguageEnglish
Published Amsterdam Elsevier B.V 01.10.2012
Elsevier
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Summary:► We used polysiloxane copolymers for improving transport properties of MgB2. ► Polysiloxane-co-vinyl-ferrocene was used to insert magnetic nanoparticles. ► Cyclic polysiloxane-co-styrene leads to the best critical properties. ► Magnetic pinning is visible at high temperatures in samples with ferrocene. We used preceramic polysiloxane polymers to fabricate superconducting MgB2 composites that are doped with carbon and nanosized inclusions to improve the pinning properties. The polysiloxanes were prepared by atom transfer radical polymerization and the composites were fabricated by the short time spark plasma sintering method. We found that the superconducting critical temperatures were higher than expected from the carbon content found from the X-ray diffraction analysis of the (110) peak of MgB2. To explain this finding we propose that the grains are unevenly doped, with a core–shell distribution. We also found that both, the upper critical fields and the critical current densities are higher in the preceramic-doped samples than in pure MgB2, in agreement with the carbon doping level. When ferrocene-grafted polysiloxane is used, the upper critical field is the largest, while the critical current density is the lowest. We attribute this fact to the fact that the polymer pyrolysis results in iron-based nanostructures which have a pair breaking effect.
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
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ISSN:0921-4534
1873-2143
DOI:10.1016/j.physc.2012.03.052