Hauptseite > Publikationsdatenbank > Ferroelectricity in nonstoichiometric SrTiO3 films studied by ultraviolet Raman spectroscopy > print |
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024 | 7 | _ | |a 10.1063/1.3499273 |2 DOI |
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084 | _ | _ | |2 WoS |a Physics, Applied |
100 | 1 | _ | |0 P:(DE-HGF)0 |a Tenne, D.A. |b 0 |
245 | _ | _ | |a Ferroelectricity in nonstoichiometric SrTiO3 films studied by ultraviolet Raman spectroscopy |
260 | _ | _ | |a Melville, NY |b American Institute of Physics |c 2010 |
300 | _ | _ | |a 142901 |
336 | 7 | _ | |a Journal Article |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |
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440 | _ | 0 | |0 562 |a Applied Physics Letters |v 97 |x 0003-6951 |y 14 |
500 | _ | _ | |a This work was supported in part by the NSF through Grant Nos. DMR-0705127 (D.A.T.), DMR-0507146 (D.G.S.), ECCS-0708759 (C.B.E.), and DMR-0906443 (C.B.E.) and through the MRSEC program by Grant No. DMR-0820404 (C.M.B), DOE EPSCoR Grant No. DE-FG02-04ER46142 (D.A.T.), and Research Corporation for Science Advancement Grant No. 7134 (D.A.T.). |
520 | _ | _ | |a Homoepitaxial Sr1+xTiO3+delta films with -0.2 <= x <= 0.25 grown by reactive molecular-beam epitaxy on SrTiO3 (001) substrates have been studied by ultraviolet Raman spectroscopy. Nonstoichiometry for strontium-deficient compositions leads to the appearance of strong first-order Raman scattering at low temperatures, which decreases with increasing temperature and disappears at about 350 K. This indicates the appearance of a spontaneous polarization with a paraelectric-to-ferroelectric transition temperature above room temperature. Strontium-rich samples also show a strong first-order Raman signal, but the peaks are significantly broader and exhibit a less pronounced temperature dependence, indicating a stronger contribution of the disorder-activated mechanism in Raman scattering. (C) 2010 American Institute of Physics. [doi:10.1063/1.3499273] |
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700 | 1 | _ | |0 P:(DE-HGF)0 |a Heeg, T. |b 3 |
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773 | _ | _ | |0 PERI:(DE-600)1469436-0 |a 10.1063/1.3499273 |g Vol. 97, p. 142901 |p 142901 |q 97<142901 |t Applied physics letters |v 97 |x 0003-6951 |y 2010 |
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