Le four to guide us in proper recognition on the states. From our calculations, we located that the inclusion on the triple excitation 4d6 4f3 improves the match involving the present energies and measurements for the greater 4d8 4f levels, even though it deteriorates the agreement for other levels. Thus we’ve got thought of two sets of calculations for Xe9+ , one particular with and the other without such as the CSF 4d6 4f3 . The energies marked with in Table four indicate the inclusion in the CSF 4d6 4f3 . For 4p5 4d10 levels, our power outcomes overestimate the measurements [5] and theoretical final results [15] by practically 2 eV. Except for this transition, in most of the instances our energies show greater agreements together with the experimental final results than the MCDHF calculations [15]. Table 5 presents a comparison on the present energies together with the experimental energies from Churilov et al. [6] and RCI and HFR calculations of Motoumba et al. [14] for Xe10+ . Comparable to Xe9+ , Xe10+ has an open shell structure and therefore, we’ve integrated the wavenumbers Mequinol In Vitro reported in [6] in order that the little spaced levels may be rightly identified. We learnt that adding the CSF 4p4 4d10 improves the energy from the 4d8 levels, though like the CSF 4d5 4f3 with triple excitation improves the power on the larger 4d7 4f levels. The order of some levels from 4d8 , 4d7 5p and 4d7 4f configurations are not as per the order reported in the measurements [6]. Similar cases are also observed within the RCI benefits [14]. Our reported energies show a deviation of practically 2-4 eV for the 4p5 4d9 levels, nonetheless, they are in good agreement using the RCI calculations by Motoumba et al. [14]. The comparison of our calculated wavelengths and transition rates with other theoretical and experimental results is shown via Tables six. For Xe7+ , Table six consists of the measurements from NIST EBIT and Cowan code calculations reported by Fahy et al. [8], compact EBIT benefits from Ali and Nakamura [9] too as HFR calculations of Churilov and Joshi [5]. Though Table six shows a maximum deviation of three.5 for levels of 4d9 5s4f configurations with indices 9 and ten, a great agreement is located involving our reported transition rates plus the calculated results from Cowan code [8]. Wavelengths and transition rates for Xe8+ from the present function are reported and compared in Table 7 together with the measurements and other calculations [5,80,13]. All round, our calculations are in very good agreement with other outcomes. On the other hand, a maximum deviation of 3.4 is identified within the wavelength corresponding to 1 15 (4d10 1 S0 4d9 4f 1 P1 ) transition. This can be because from Table 3 our calculated power on the 4d9 4f 1 P1 level is overestimated by nearly three eV in comparison for the outcome reported by Churilov and Joshi [5]. It can be further noticed for the above transition that our calculated wavelength shows a far better match with that from Ivanova [13] and there is a excellent agreement amongst various values of the transition rate.Table six. Wavelengths and transition rates of Xe7+ for the transitions from 4d10 5s 2 S1/2 state.Index 10 9 8 7 six 5 four 3Jb 3/2 1/2 1/2 3/2 1/2 1/2 3/2 3/2 3/Wavelength (nm) Present 11.9593 11.9713 16.5963 17.0015 17.8218 17.9319 18.1815 18.4659 18.7259 Other Reported 12.32 a , 12.56 b , 12.332 c , 12.3243 d 12.56 b , 12.3265 d 16.668 c a , 17.09 b , 17.087 c 17.09 17.6 a , 17.61 b , 17.603 c 17.73 a , 17.76 b , 17.726 c 17.98 a , 17.92 b , 17.958 c 18.15 a , 18.07 b 18.44 a , 18.31 b , 18.4322 cTransition Price (A) (1010 ) (s-1 ) Present 128.093 122.349 1.934.
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