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Epitaxial La0.67(Sr,Ca)0.33MnO3 Films on Si for IR Bolometer Applications

Published online by Cambridge University Press:  17 March 2011

A.M. Grishin
Affiliation:
Department of Condensed Matter Physics, Royal Institute of Technology, SE-164 40 Stockholm-Kista, SWEDEN
S.I. Khartsev
Affiliation:
Department of Condensed Matter Physics, Royal Institute of Technology, SE-164 40 Stockholm-Kista, SWEDEN
J.-H. Kim
Affiliation:
Department of Condensed Matter Physics, Royal Institute of Technology, SE-164 40 Stockholm-Kista, SWEDEN
Jun Lu
Affiliation:
Ångström Microstructure Laboratory, Uppsala University, SE-751 21 Uppsala, SWEDEN
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Abstract

We report on processing and properties of La0.67(Sr,Ca)0.33MnO3(LSCMO) films grown by pulsed laser deposition technique on Si(001) substrates buffered with Bi4Ti3O12/CeO2/YSZ heteroepitaxial layers. X-ray diffraction shows cube-on-cube growth of epitaxial Bi4Ti3O12/CeO2/YSZ/Si heterostructure whereas the LSCMO layer grows in the “diagonal-on-side” manner onto the Bi4Ti3O12 (BTO) template. High resolution TEM images demonstrate sharp interfaces between the buffer layers and LSCMO film as well as rare misfit dislocations on the CeO2/YSZ interface. LSCMO film processing conditions have been optimized to get maximum temperature coefficient of resistivity TCR = 4.4%K-1 and colossal magnetoresistance(CMR) ‘Delta;ρ/ρ ∼ 2.9%kOe-1 @ 294K. Almost ultimate CMR performance at room temperature has been achieved due to successive improvement of c-axisorientation of layers: full widths at half-maximum (FWHM) 0.65, 0.58, 0.65, 1.13 and 0.18 degrees in LSCMO/BTO/CeO2/YSZ/Si stack, respectively. Characterization of electrical noise in CMR film yields noise equivalent temperature difference (NETD) as low as 1.2 ‘mu;K/√Hz @ 30Hz and 294K.

Type
Research Article
Copyright
Copyright © Materials Research Society 2004

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References

REFERENCES

1 Lisauskas, Alvydas, Khartsev, S. I., Grishin, Alex, Appl. Phys. Lett. 77, 756 (2000); ibid 77, 3302 (2000).Google Scholar
2 Trajanovic, Z., Kwon, C., Robson, M.C., Kim, K. C., Rajeswari, M., Ramesh, R., Venkatesan, T., Appl. Phys. Lett. 69,1005 (1996).Google Scholar
3 Gu, J. Y., Kwon, C., Robson, M.C., Trajanovic, Z., Ghosh, K., Sharma, R. P., Shreekala, R., Rajeswari, M.. Venkatesan, T., and Ramesh, R., Appl. Phys. Lett, 70, 1763 (1997).Google Scholar
4 Wong, K. H., Leung, Y.S., Thin Solid Films, 354, 55 (1999).Google Scholar
5 Rubi, D., Duhalde, S., Terzzoli, M. C., Leyva, G., Polla, G., Levy, P., Parisi, F., Urbano, R.R., Physica B, 320, 86 (2002).Google Scholar
6 Kung, Pang-Jen, Fenner, D. B., Potrepka, Daniel M., Budnick, Joseph I., Appl. Phys. Lett, 69,427 (1996).Google Scholar
7 Khartsev, S. I. and Grishin, A. M., Mater. Res. Soc. Symp. Proc. 666, F7.12 (2001).Google Scholar
8 Lisauskas, A., Khartsev, S. I., Grishin, A.M., Proc. SPIE 4318, 235 (2001).Google Scholar
9 Unewisse, M. H., Craig, B. I., Watson, R. J., Reinhold, O., and Liddiard, K.C., Proc. SPIE 2554, 43 (1995).Google Scholar