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Anharmonic effects and Faust-Henry coefficient of CdTe in the vicinity of the energy gap

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dc.contributor.author Stergiou, VC en
dc.contributor.author Kontos, AG en
dc.contributor.author Raptis, YS en
dc.date.accessioned 2014-03-01T01:27:56Z
dc.date.available 2014-03-01T01:27:56Z
dc.date.issued 2008 en
dc.identifier.issn 1098-0121 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/18641
dc.subject Energy Gap en
dc.subject.classification Physics, Condensed Matter en
dc.subject.other WAVELENGTH OPTICAL PHONONS en
dc.subject.other RAMAN-SCATTERING en
dc.subject.other TEMPERATURE-DEPENDENCE en
dc.subject.other THERMAL-EXPANSION en
dc.subject.other PRESSURE-DEPENDENCE en
dc.subject.other IONIC CRYSTALS en
dc.subject.other DISPERSION en
dc.subject.other SPECTRA en
dc.subject.other SEMICONDUCTORS en
dc.subject.other DETECTORS en
dc.title Anharmonic effects and Faust-Henry coefficient of CdTe in the vicinity of the energy gap en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevB.77.235201 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevB.77.235201 en
heal.identifier.secondary 235201 en
heal.language English en
heal.publicationDate 2008 en
heal.abstract Crystallodynamic properties of CdTe are studied, by Raman spectroscopy, as a function of the temperature and excitation energy. The temperature dependence (in the range of 20-300 K) of the peak frequency and the full width at half maximum of the Raman scattering bands, which were obtained from the ≈0 optical (LO and TO) lattice vibrations, are mainly attributed to the anharmonic effects due to the phonon decay toward the ≠0 points of the Brillouin zone. The intensity ratio (LO/TO) of the phonons is also studied as a function of the temperature and excitation energy, leading to a Faust-Henry coefficient that is nearly constant over the energy range investigated (1.49-1.54 eV). © 2008 The American Physical Society. en
heal.publisher AMER PHYSICAL SOC en
heal.journalName Physical Review B - Condensed Matter and Materials Physics en
dc.identifier.doi 10.1103/PhysRevB.77.235201 en
dc.identifier.isi ISI:000257289500051 en
dc.identifier.volume 77 en
dc.identifier.issue 23 en


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