TY - DATA T1 - The Z4 scaled radiative transition probabilities Adi (s−1) for the 2snp 1, 3P1 → 2s22p6 1S0 (6 ≤ n ≤ 13) transition and Auger branch ratios Ba of different states of Fe16+, Kr26+ and Xe44+, as a function of the principal number n PY - 2013/08/07 AU - L C Gao AU - D H Zhang AU - L Y Xie AU - J G Wang AU - Y L Shi AU - C Z Dong UR - https://iop.figshare.com/articles/figure/_The_em_Z_em_sup_4_sup_scaled_radiative_transition_probabilities_em_A_sub_di_sub_em_em_s_em_sup_1_su/1012617 DO - 10.6084/m9.figshare.1012617.v1 L4 - https://ndownloader.figshare.com/files/1480440 KW - 2 2 KW - number n KW - Abstract Photoionization KW - Z 4 KW - Auger branch ratios Ba KW - xe KW - kr KW - fe KW - ground state 1 KW - 2 2 p 61 S 0 KW - radiative transition probabilities Adi KW - method KW - section KW - systematical calculations KW - pi KW - dirac KW - resonance strengths KW - ar KW - Atomic Physics KW - Molecular Physics N2 - Figure 3. The Z4 scaled radiative transition probabilities Adi (s−1) for the 2snp 1, 3P1 → 2s22p6 1S0 (6 ≤ n ≤ 13) transition and Auger branch ratios Ba of different states of Fe16+, Kr26+ and Xe44+, as a function of the principal number n. Abstract Photoionization (PI) cross sections of the ground state 1s2 2s2 2p61 S0 of Ne-like Ar8+, Fe16+, Kr26+ and Xe44+ ions are calculated by using the Dirac atomic R-matrix code based on a fully relativistic R-matrix method. To analyze the detailed resonant structure, systematical calculations based on the multiconfiguration Dirac–Fock method are performed for the dominant 2s → np resonant transitions, and the resonant energies, strengths and total natural widths are presented. The resonant structures and characteristics of the PI cross sections and resonance strengths along the Ne-like sequence are discussed with emphasis on the influence of relativistic effects. For the Ar8+ ion, good agreement is found between the present results and available theoretical calculations and experimental data. ER -