Hetero-Epitaxial Growth of YBCO and MgB 2 Thin Films on Decorated Substrates with Nano-Wires and Nano-Particles
Hetero-Epitaxial Growth of YBCO and MgB 2 Thin Films on Decorated Substrates with Nano-Wires and Nano-Particles
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纳米线和纳米颗粒装饰基底上异质外延生长YBCO和MgB 2 薄膜
DOI:
10.1557/opl.2012.1485
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发表时间:
2012
期刊:
影响因子:
--
通讯作者:
S. Ohshima
中科院分区:
文献类型:
--
作者:
S. Ohshima
Superconducting NMR pickup coils have to have a low surface resistance (Rs) under a high magnetic field. One way of reducing the Rs of superconducting thin films is adding artificial pins to the films. We examined the hetero-epitaxial growth of MgB 2 and YBCO thin films on decorated sapphire and MgO substrates while using nano-wires and nano-particles to add pins to the films. We used ZnO nano-wire to add artificial grain boundary pins to MgB 2 films. The tilted c-plane sapphire substrate with nano-step edges was used for these substrates. The terrace width with one lattice step edge can be controlled by changing the tilt angle. AFM images showed that the tilted c-plane sapphire substrate had straight nano-step edges. ZnO nono-wires were decorated on the nano-step edges by MOCVD, and then deposited on MgB 2 films by sputtering. The Rs of the films was then measured with a sapphire rod resonator. The Rs of MgB 2 thin films fabricated on the tilted c-plane sapphire substrate with ZnO nano-wires was lower than that of MgB 2 thin films on a conventional sapphire substrate under a high magnetic field. We used BaZrO 3 (BZO) nano-particles to add the artificial pins to YBCO thin films. The BZO particles on the MgO substrates were fabricated by laser deposition. The size and density of these particles were controlled with a pulse number of laser shot. YBCO thin films were formed on decorated MgO substrate by laser deposition. The Rs of YBCO thin films on the decorated MgO substrate was lower than that of the YBCO films formed on a conventional MgO substrate under a high magnetic field. We clarified that artificial pins in MgB 2 and YBCO thin films are useful for decreasing the Rs under a high magnetic field.