| Автор | J Jauhiainen |
| Автор | H Aksela |
| Автор | S Aksela |
| Автор | A Kivimaki |
| Автор | O -P Sairanen |
| Автор | E Nommiste |
| Автор | J Vegh |
| Дата выпуска | 1995-09-14 |
| dc.description | Correlation satellite lines originating from the strong mixing between 5s<sup>1</sup>5p<sup>5</sup>, 5s<sup>2</sup>5p<sup>3</sup>nd (n=5, 6, 7, ...) and 5s<sup>2</sup>5p<sup>3</sup>ms (m=6, 7, 8, ...) configurations in the final state of the N<sub>4,5</sub>-O<sub>1</sub>O<sub>2,3</sub> Auger decay of Xe and between 4s<sup>1</sup>4p<sup>5</sup>, 4s<sup>2</sup>4p<sup>3</sup>nd (n=4, 5, 6, ...) and 4s<sup>2</sup>4p<sup>3</sup>ms (m=5, 6, 7, ...) final-state configurations in the M<sub>4,5</sub>-N<sub>1</sub>N<sub>2,3</sub> Auger decay of Kr have been studied by means of synchrotron-radiation excited electron spectroscopy and relativistic multiconfigurational Dirac-Fock calculations. Improvements in experimental and computational methods have made it possible, for the first time, to resolve and to assign most of the satellite lines with high accuracy. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Correlation satellites in the Xe N<sub>4,5</sub>-OO and Kr M<sub>4,5</sub>-NN Auger spectra |
| Тип | paper |
| DOI | 10.1088/0953-4075/28/17/020 |
| Electronic ISSN | 1361-6455 |
| Print ISSN | 0953-4075 |
| Журнал | Journal of Physics B: Atomic, Molecular and Optical Physics |
| Том | 28 |
| Первая страница | 3831 |
| Последняя страница | 3843 |
| Аффилиация | J Jauhiainen; Dept. of Phys., Oulu Univ., Finland |
| Аффилиация | H Aksela; Dept. of Phys., Oulu Univ., Finland |
| Аффилиация | S Aksela; Dept. of Phys., Oulu Univ., Finland |
| Аффилиация | A Kivimaki; Dept. of Phys., Oulu Univ., Finland |
| Аффилиация | O -P Sairanen; Dept. of Phys., Oulu Univ., Finland |
| Аффилиация | E Nommiste; Dept. of Phys., Oulu Univ., Finland |
| Аффилиация | J Vegh; Dept. of Phys., Oulu Univ., Finland |
| Выпуск | 17 |
