dc.contributor.author |
Christofilos, D |
en |
dc.contributor.author |
Papagelis, K |
en |
dc.contributor.author |
Ves, S |
en |
dc.contributor.author |
Kourouklis, GA |
en |
dc.contributor.author |
Raptis, C |
en |
dc.date.accessioned |
2014-03-01T01:17:58Z |
|
dc.date.available |
2014-03-01T01:17:58Z |
|
dc.date.issued |
2002 |
en |
dc.identifier.issn |
0953-8984 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/14726 |
|
dc.subject |
High Pressure |
en |
dc.subject |
Lattice Dynamics |
en |
dc.subject.classification |
Physics, Condensed Matter |
en |
dc.subject.other |
Crystal lattices |
en |
dc.subject.other |
Eigenvalues and eigenfunctions |
en |
dc.subject.other |
High pressure effects |
en |
dc.subject.other |
Phase transitions |
en |
dc.subject.other |
Raman spectroscopy |
en |
dc.subject.other |
Monoclinic structure |
en |
dc.subject.other |
Strontium compounds |
en |
dc.title |
High-pressure Raman study and lattice dynamical calculations for SrWO4 |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1088/0953-8984/14/47/334 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1088/0953-8984/14/47/334 |
en |
heal.language |
English |
en |
heal.publicationDate |
2002 |
en |
heal.abstract |
A high-pressure Raman study of SrWO4 reveals a pressure induced phase transition starting at 11.5 GPa. Several Raman lines exhibit a nonlinear behaviour in the pressure range of 11.5-15 GPa, which can be attributed to either stabilization of the high-pressure phase or an intermediate phase. Using a theoretical lattice dynamical calculation, based on an empirical potential model, we have obtained the Raman active mode eigenvectors giving us an insight into the phase transition mechanism. The lowest-frequency mode exhibits a negative pressure slope in the scheelite phase and involves a motion of the WO4 tetrahedron as a whole according to the theoretical results. The experimental evidence suggests that the structure of the high-pressure phase is closely related to the scheelite structure, being formed by closely lying distorted WO4 tetrahedra rather than involving an octahedrally coordinated W ion. |
en |
heal.publisher |
IOP PUBLISHING LTD |
en |
heal.journalName |
Journal of Physics Condensed Matter |
en |
dc.identifier.doi |
10.1088/0953-8984/14/47/334 |
en |
dc.identifier.isi |
ISI:000180323900038 |
en |
dc.identifier.volume |
14 |
en |
dc.identifier.issue |
47 |
en |
dc.identifier.spage |
12641 |
en |
dc.identifier.epage |
12650 |
en |