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dc.contributor.authorTownsend, P. D.
dc.contributor.authorFinch, A. A.
dc.contributor.authorMaghrabi, M.
dc.contributor.authorRamachandran, V.
dc.contributor.authorVázquez, G. V.
dc.contributor.authorWang, Y.
dc.contributor.authorWhite, D. R.
dc.date.accessioned2018-07-21T23:34:44Z
dc.date.available2018-07-21T23:34:44Z
dc.date.issued2017-12
dc.identifier250562847
dc.identifierbb63c61f-46f7-4339-bafe-a32f2a6c6170
dc.identifier85026377517
dc.identifier000413037400083
dc.identifier.citationTownsend , P D , Finch , A A , Maghrabi , M , Ramachandran , V , Vázquez , G V , Wang , Y & White , D R 2017 , ' Spectral changes and wavelength dependent thermoluminescence of rare earth ions after X-ray irradiation ' , Journal of Luminescence , vol. 192 , pp. 574-581 . https://doi.org/10.1016/j.jlumin.2017.07.041en
dc.identifier.issn0022-2313
dc.identifier.otherRIS: urn:8E0CE07E3D5F35FB091CEFE84572B5EA
dc.identifier.otherORCID: /0000-0002-3689-1517/work/38002304
dc.identifier.urihttps://hdl.handle.net/10023/15623
dc.descriptionY. Wang would like to thank the support of the Fundamental Research Funds for the Central Universities of China, the National Natural Science Foundation of China (No.51472224, No.11205134), and Beijing Higher Education Young Elite Teacher Project (YETP0640).en
dc.description.abstractThe thermoluminescence spectra of rare earth doped materials after X-ray irradiation typically vary with the glow peak temperature. Additionally, there are many examples where, for the same dopant ion, the expected component emission lines peak, but at different temperatures. This unusual behaviour is discussed in terms of changes in proximity of coupling between trapping and recombination sites. Changes in the energy barriers for recombination influence alternative routes for charge transfer to rare earth sites which can involve different higher energy states of the rare earth dopants. Proposed mechanisms include selective tunnelling, or barrier crossing, in addition to normal charge transfer from remote trapping sites. The model successfully describes numerous examples in terms of the energy scheme for the rare earth ions. Whilst the standard emission lines are recorded in the glow curve spectra they do not always occur at the same temperature, and, even for the same rare earth dopant, they can differ by as much as 30 °C. These wavelength dependent variations in peak temperature not only offer information on the proximity of trap and recombination sites, but also introduce issues in conventional activation energy analysis when recording is with polychromatic light. The concepts are relevant for related types of measurement, such as optically stimulated thermoluminescence.
dc.format.extent8
dc.format.extent1028185
dc.language.isoeng
dc.relation.ispartofJournal of Luminescenceen
dc.subjectThermoluminescenceen
dc.subjectModelen
dc.subjectWavelength dependenten
dc.subjectQC Physicsen
dc.subjectGE Environmental Sciencesen
dc.subjectNDASen
dc.subject.lccQCen
dc.subject.lccGEen
dc.titleSpectral changes and wavelength dependent thermoluminescence of rare earth ions after X-ray irradiationen
dc.typeJournal articleen
dc.contributor.sponsorNERCen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. Marine Alliance for Science & Technology Scotlanden
dc.contributor.institutionUniversity of St Andrews. Scottish Oceans Instituteen
dc.contributor.institutionUniversity of St Andrews. St Andrews Isotope Geochemistryen
dc.identifier.doihttps://doi.org/10.1016/j.jlumin.2017.07.041
dc.description.statusPeer revieweden
dc.date.embargoedUntil2018-07-22
dc.identifier.grantnumberNE/H002715/1en


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