Growing LaAlO3/SrTiO3 interfaces by sputter deposition
Source abstract
Abstract
Sputter deposition of oxide materials in a high-pressure oxygen atmosphere is a well-known technique to produce thin films of perovskite oxides in particular. Also interfaces can be fabricated, which we demonstrated recently by growing LaAlO3 on SrTiO3 substrates and showing that the interface showed the same high degree of epitaxy and atomic order as is made by pulsed laser deposition. However, the high pressure sputtering of oxides is not trivial and number of parameters are needed to be optimized for epitaxial growth. Here we elaborate on the earlier work to show that only a relatively small parameter window exists with respect to oxygen pressure, growth temperature, radiofrequency power supply and target to substrate distance. In particular the sensitivity to oxygen pressure makes it more difficult to vary the oxygen stoichiometry at the interface, yielding it insulating rather than conducting.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Electronic and Structural Properties of Oxides · Magnetic and transport properties of perovskites and related materials · Semiconductor materials and devices
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Leiden University 1 Kamerlingh Onnes Laboratorium, , The Netherlands
Delft Technical University 2 National Center for High Resolution Microscopy, Kavli Institute for Nanoscience, , Lorentzweg 1, 2628 CJ Delft, The Netherlands
University of Twente 3 Faculty of Science and Technology and MESA+ Institute for Nanotechnology, , 7500 AE Enschede, The Netherlands
Leiden University 4 Huygens - Kamerlingh Onnes Laboratorium, , The Netherlands
References (25)
Show source-provided references
1. Nature · 2004 · 427 · 42310.1038/nature02308 ↗
2. J. Phys. Cond. Matt. · 2014 · 26 · 14320110.1088/0953-8984/26/14/143201 ↗
3. Nature Materials · 2006 · 5 · 20410.1038/nmat1569 ↗
4. Science · 2006 · 313 · 194210.1126/science.1131091 ↗
5. Phys. Rev. B · 2007 · 75 · 121404(R)10.1103/PhysRevB.75.121404 ↗
6. Nature Mat. · 2007 · 6 · 49310.1038/nmat1931 ↗
7. Adv. Mat. · 2009 · 21 · 166510.1002/adma.200801448 ↗
8. Europhys. Lett. · 2011 · 93 · 3700110.1209/0295-5075/93/37001 ↗
9. Europhys. Lett. · 2010 · 91 · 1700410.1209/0295-5075/91/17004 ↗
10. Bulletin of the APS · 2010 · 55
11. Nat. Commum. · 2013 · 4 · 235110.1038/ncomms3351 ↗
12. e-JSSNT · 2012 · 10 · 110.1380/ejssnt.2012.1 ↗
13. Appl. Phys. Lett. · 2013 · 102 · 12160110.1063/1.4798828 ↗
14. Phys. Rev. Lett. · 2013 · 110 · 19680410.1103/PhysRevLett.110.196804 ↗
15. Appl. Phys. Lett. · 2010 · 97 · 12410510.1063/1.3487778 ↗
16. Appl. Phys. Lett. · 2012 · 101 · 13160110.1063/1.4754112 ↗
17. Appl. Phys. Lett. · 2013 · 102 · 25160210.1063/1.4812353 ↗
18. Appl. Phys. Lett. · 2013 · 103 · 07160410.1063/1.4817921 ↗
19. Zeitsch. Physik B · 1989 · 74 · 1310.1007/BF01307235 ↗
20. Science · 1994 · 266 · 154010.1126/science.266.5190.1540 ↗
21. Appl. Phys. Lett. · 1998 · 73 · 292010.1063/1.122630 ↗
22. Phys. Rev. B · 2011 · 83 · 08540810.1103/PhysRevB.83.085408 ↗
23. Appl. Surf. Science · 2012 · 258 · 924210.1016/j.apsusc.2012.01.117 ↗
24. Appl. Phys. Lett. · 2014 · 104 · 05160910.1063/1.4864186 ↗
25. Bulletin of the APS · 2011 · 56