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A relativistic version of the time-dependent local density approximation has been developed and is applied to study the photoionisation of mercury above the 5d 3/2 threshold. Partial cross sections and angular distribution asymmetry parameters for the 5d and 6s subshells are determined. Comparisons are made with the relativistic random-phase approximation and with measurements.
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Parpia et al. (1983) studied this question.
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