dc.contributor.author |
Antonakos, A |
en |
dc.contributor.author |
Liarokapis, E |
en |
dc.contributor.author |
Filippi, M |
en |
dc.contributor.author |
Prellier, W |
en |
dc.contributor.author |
Aydogdu, GH |
en |
dc.contributor.author |
Habermeier, H-U |
en |
dc.date.accessioned |
2014-03-01T02:46:12Z |
|
dc.date.available |
2014-03-01T02:46:12Z |
|
dc.date.issued |
2009 |
en |
dc.identifier.issn |
1557-1939 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/32601 |
|
dc.subject |
Infrared |
en |
dc.subject |
Manganites |
en |
dc.subject |
Thin films |
en |
dc.subject.classification |
Physics, Applied |
en |
dc.subject.classification |
Physics, Condensed Matter |
en |
dc.subject.other |
Different substrates |
en |
dc.subject.other |
Infrared |
en |
dc.subject.other |
Infrared active modes |
en |
dc.subject.other |
Infrared reflectivity spectrums |
en |
dc.subject.other |
Insulating gaps |
en |
dc.subject.other |
Manganite thin films |
en |
dc.subject.other |
Thickness dependences |
en |
dc.subject.other |
Calcium |
en |
dc.subject.other |
Gallium alloys |
en |
dc.subject.other |
Infrared spectroscopy |
en |
dc.subject.other |
Manganese compounds |
en |
dc.subject.other |
Manganites |
en |
dc.subject.other |
Oxide minerals |
en |
dc.subject.other |
Reflection |
en |
dc.subject.other |
Solids |
en |
dc.subject.other |
Thin films |
en |
dc.subject.other |
Substrates |
en |
dc.title |
Infrared reflectivity spectra of manganite thin films grown on different substrates |
en |
heal.type |
conferenceItem |
en |
heal.identifier.primary |
10.1007/s10948-008-0399-8 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1007/s10948-008-0399-8 |
en |
heal.language |
English |
en |
heal.publicationDate |
2009 |
en |
heal.abstract |
We have measured the reflectivity infrared (IR) spectra of R1-x Ca (x) MnO3 (R = La, Pr) manganite thin films grown on different substrates (SrTiO3 (STO), LaAlO3 (LAO) and SrLaGaO4 (SLGO)) manganites over a wide frequency (50-5000 cm(-1)) range. In the Far IR (FIR) region the substrates dominate over the manganite spectrum. However, the previously observed infrared active modes or mode pairs could be identified. In the mid-IR (MIR) region, a characteristic insulating gap at 700 cm(-1) is always present for all thin film studied, which shows substrate and thickness dependence. |
en |
heal.publisher |
SPRINGER |
en |
heal.journalName |
Journal of Superconductivity and Novel Magnetism |
en |
dc.identifier.doi |
10.1007/s10948-008-0399-8 |
en |
dc.identifier.isi |
ISI:000262315900004 |
en |
dc.identifier.volume |
22 |
en |
dc.identifier.issue |
2 |
en |
dc.identifier.spage |
109 |
en |
dc.identifier.epage |
113 |
en |