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- W2016530246 abstract "Detailed calculations on the Kbeta X-ray emission spectrum of atomic argon are reported, using CI wavefunctions based on MCDF-EAL calculations for a number of configurations of varying degrees of excitation and ionisation. Crude approximations to the total widths of states, initial-state populations from shake theory and radiative transition probabilities calculated in a transition orbitals approach were used to obtain line intensities which were synthesised into a predicted spectrum which could be compared with experiment. It is shown that the Rydberg spectator transition (1s)((3p)4p 1S) 2S-(3p2 1D)34p 2P0 contributes substantially to the Kbeta v satellite, altering its shape from that predicted in a simple model which includes only primary hole states, and bringing it into agreement with the experimentally determined shape. It was not possible to identify the major contributions the the Kbeta satellite, but the (1s3s) transitions could be excluded by energy considerations, and the most likely contributions are considered to be the (1s3p2)-(3p3) transitions with or without Rydberg spectator satellites." @default.
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- W2016530246 date "1984-04-14" @default.
- W2016530246 modified "2023-09-24" @default.
- W2016530246 title "The KβX-ray emission spectrum of argon: a theoretical account" @default.
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