DC Field | Value | Language |
dc.contributor.author | Dunina, E. V. | - |
dc.contributor.author | Kornienko, A. A. | - |
dc.contributor.author | Fomicheva, L. A. | - |
dc.date.accessioned | 2016-05-24T12:58:28Z | - |
dc.date.accessioned | 2017-07-27T12:00:34Z | - |
dc.date.available | 2016-05-24T12:58:28Z | - |
dc.date.available | 2017-07-27T12:00:34Z | - |
dc.date.issued | 2008 | - |
dc.identifier.citation | Dunina, E. B. Modified theory of f-f transition intensities and crystal field for systems with anomalously strong configuration interaction / E. V. Dunina, A. A. Kornienko, L. A. Fomicheva // Cent. Eur. J. Phys. – 2008. – Vol. 6, № 3. – P. 407 – 414. | ru_RU |
dc.identifier.uri | https://libeldoc.bsuir.by/handle/123456789/6973 | - |
dc.description.abstract | A new theory explaining the intensity of f-f transitions and the crystal field using an approximation of a strong configuration interaction is proposed. The theory enables the anomalous influence of excited configurations with charge transfer on some multiplets of the f shell to be taken into account. With the help of this theory, a satisfactory description of the absorption transitions and luminescence branching ratios from 1 D 2 and 3 P 0 multiplets for the Pr3+ ion in double molybdates has been achieved for the first time. For further validation the theory, was used to provide a description of Stark splitting of Pr3+ — multiplets in elpasolites and determine the covalence parameters; these parameters were found to be in good agreement with values obtained by the other methods. | ru_RU |
dc.language.iso | en | ru_RU |
dc.subject | публикации ученых | ru_RU |
dc.subject | lanthanide ions | ru_RU |
dc.subject | modified Judd-Ofelt theory | ru_RU |
dc.subject | modified theory of crystal field | ru_RU |
dc.subject | optical spectroscopy | ru_RU |
dc.title | Влияние возбужденных конфигураций на силы линий абсорбционных переходов иона тербия в оксидных кристаллах | ru_RU |
dc.type | Article | ru_RU |
Appears in Collections: | Публикации в зарубежных изданиях
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