K-Shell Photoionization of the Oxygen Isonuclear Sequence

29th International Conference on Photonic, Electronic, and Atomic Collisions

Gharaibeh, M.F.^1,2 ; Bizau, J.M.^3 ; Cubaynes, D.^3 ; Guilbaud, S.^3 ; Al Shorman, M.M.^3 ; Ababneh, I.Q.^2 ; Sakho, I.^4 ; Blancard, C.^5 ; McLaughlin, B.M.^6,7

Department of Mathematics, Statistics and Physics, Qatar University, P. O. Box 2713, Doha, Qatar^1

Department of Physics, Jordan University of Sciences and Technology, Irbid

22110, Jordan^2

Institut des Sciences Moieculaires DOrsay (ISMO), CNRS UMR 8214, Universite Paris-Sud, Bat. 350, Orsay Cedex

F-91405, France^3

Department of Physics, UFR of Sciences and Technologies, University Assane Seck of Ziguinchor, Ziguinchor, Senegal^4

CEA-DAM-DIF, Bruyeres-le-Chatel, Arpajon Cedex

F-91297, France^5

Centre for Theoretical Atomic and Molecular Physics (CTAMOP), School of Mathematics and Physics, Queen's University of Belfast, Belfast

BT7 1NN, United Kingdom^6

Institute for Theoretical Atomic and Molecular Physics (ITAMP), Harvard Smithsonian Center for Astrophysics, MS-14, Cambridge

MA

02138, United States^7

关键词: Isonuclear sequence;    K-shell photoionization;    R-matrix calculation;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/635/9/092074/pdf
DOI  :  10.1088/1742-6596/635/9/092074

来源: IOP

【 摘 要 】

K-shell photoionization cross-section measurements for the oxygen isonuclear sequence from N-like to Li-like made at the SOLEIL Light Source are compared with SUNC, MCDF and R-matrix calculations.