Grain orientations and grain boundary networks of YBa2Cu3O7−δ films deposited by metalorganic and pulsed laser deposition on biaxially textured Ni–W substrates
Source abstract
Abstract
We report a detailed study of the grain orientations and grain boundary (GB) networks in YBa2Cu3O7-δ (YBCO) films ∼0.8 μm thick grown by both the in situ pulsed laser deposition (PLD) process and the ex situ metalorganic deposition (MOD) process on rolling-assisted biaxially textured substrates (RABiTS). The PLD and MOD growth processes result in columnar and laminar YBCO grain structures, respectively. In the MOD-processed sample [full-width critical current density Jc(0 T, 77 K) = 3.4 MA/cm2], electron back-scatter diffraction (EBSD) revealed an improvement in both the in-plane and out-of-plane alignment of the YBCO relative to the template that resulted in a significant reduction of the total grain boundary misorientation angles. A YBCO grain structure observed above individual template grains was strongly correlated to larger out-of-plane tilts of the template grains. YBCO GBs meandered extensively about their corresponding template GBs and through the thickness of the film. In contrast, the PLD-processed film [full width Jc(0 T, 77 K) = 0.9 MA/cm2] exhibited nearly perfect epitaxy, replicating the template grain orientations. No GB meandering was observed in the PLD-processed film with EBSD. Direct transport measurement of the intra-grain Jc(0 T, 77 K) values of PLD and MOD-processed films on RABiTS revealed values up to 4.5 and 5.1 MA/cm2, respectively. As the intra-grain Jc values were similar, the significantly higher full-width Jc for the MOD-processed sample is believed to be due to the improved grain alignment and extensive GB meandering.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · ZnO doping and properties · Copper-based nanomaterials and applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (36)
Show source-provided references
1. 10.1063/1.142595210.1063/1.1425952 ↗
2. 10.1557/JMR.2000.015810.1557/JMR.2000.0158 ↗
3. 10.1103/RevModPhys.74.48510.1103/RevModPhys.74.485 ↗
4. 10.1016/S0968-4328(99)00047-510.1016/S0968-4328(99)00047-5 ↗
5. 10.1109/77.91978310.1109/77.919783 ↗
6. 10.1103/PhysRevB.41.403810.1103/PhysRevB.41.4038 ↗
7. 10.1109/77.91964910.1109/77.919649 ↗
8. 10.1063/1.131563110.1063/1.1315631 ↗
9. 10.1063/1.12615710.1063/1.126157 ↗
10. 10.1063/1.185541410.1063/1.1855414 ↗
11. 10.1063/1.9975210.1063/1.99752 ↗
12. 10.1016/S0921-4534(03)00803-710.1016/S0921-4534(03)00803-7 ↗
13. 10.1557/JMR.2005.026210.1557/JMR.2005.0262 ↗
14. 10.1016/j.physc.2005.03.08410.1016/j.physc.2005.03.084 ↗
15. 10.1063/1.162510310.1063/1.1625103 ↗
16. 10.1109/TASC.2003.81182010.1109/TASC.2003.811820 ↗
17. 10.1557/mrs2004.16310.1557/mrs2004.163 ↗
18. 10.1016/j.physc.2004.02.20210.1016/j.physc.2004.02.202 ↗
19. 10.1016/0921-4534(91)91104-C10.1016/0921-4534(91)91104-C ↗
20. 10.1063/1.11455910.1063/1.114559 ↗
21. 10.1557/mrs2004.16010.1557/mrs2004.160 ↗
22. 10.1557/mrs2004.16110.1557/mrs2004.161 ↗
23. 10.1063/1.136023010.1063/1.1360230 ↗
24. 10.1109/77.91988510.1109/77.919885 ↗
25. Holesinger · 2004
26. 10.1103/PhysRevB.71.10450110.1103/PhysRevB.71.104501 ↗
27. 10.1016/j.scriptamat.2004.05.01610.1016/j.scriptamat.2004.05.016 ↗
28. 10.1038/nmat91610.1038/nmat916 ↗
29. 10.1103/PhysRevLett.90.24700610.1103/PhysRevLett.90.247006 ↗
30. 10.1557/JMR.2005.015010.1557/JMR.2005.0150 ↗
31. 10.1063/1.210602110.1063/1.2106021 ↗
32. 10.1063/1.34623310.1063/1.346233 ↗
33. 10.1103/PhysRevB.60.140910.1103/PhysRevB.60.1409 ↗
34. 10.1063/1.11748910.1063/1.117489 ↗
35. 10.1088/0953-2048/16/5/10110.1088/0953-2048/16/5/101 ↗
36. 10.1088/0953-2048/17/1/01110.1088/0953-2048/17/1/011 ↗