| Numéro |
J. Phys. Colloques
Volume 48, Numéro C9, Décembre 1987
X-Ray and Inner-Shell ProcessesVol. 1 |
|
|---|---|---|
| Page(s) | C9-609 - C9-612 | |
| DOI | https://doi.org/10.1051/jphyscol:19879101 | |
X-Ray and Inner-Shell Processes
Vol. 1
J. Phys. Colloques 48 (1987) C9-609-C9-612
DOI: 10.1051/jphyscol:19879101
Departamento de Fisica and Centro de Fisica Atomica da Universidade de Lisboa (INIC), Avenida Pr. Gama Pinto 2, P-1699 Lisboa Codex, Portugal
Vol. 1
J. Phys. Colloques 48 (1987) C9-609-C9-612
DOI: 10.1051/jphyscol:19879101
ORIGIN OF THE OBSERVED Lβ2, SATELLITE X-RAYS OF TUNGSTEN NOT PREDICTED BY THEORY
L. SALGUEIRO, M.L. CARVALHO and F. PARENTEDepartamento de Fisica and Centro de Fisica Atomica da Universidade de Lisboa (INIC), Avenida Pr. Gama Pinto 2, P-1699 Lisboa Codex, Portugal
Résumé
Au cours de l'étude experimentale de la raie Lβ2 du tungstène, nous avons observé des radiations dont l'énergie est d'accord avec des transitions de Coster- Kronig L1→L3M, non prévues par la théorie.
Abstract
We observed satellite X-rays in the Lβ2 spectrum of tungsten with energies which show that they originate from atoms with a second hole in the M level. We conclude that this extra hole was created by Coster-Kronig L1→L3M transitions which existing calculations do not predict.