Abstract The excitation energy and the oscillator strength values have been computed for the 1 s 2 – 1 s 2 p , 1 s 2 s – 1 s… Click to show full abstract
Abstract The excitation energy and the oscillator strength values have been computed for the 1 s 2 – 1 s 2 p , 1 s 2 s – 1 s 2 p , 1 s 2 s – 1 s 3 p transitions in the helium isoelectronic sequence ( Z = 2 through Z = 116 ). The importance of the Breit interaction and radiative corrections to the oscillator strength as well as transition energies have been studied. The method of calculations was based on the relativistic hydrogen-like (with non-integer nuclear number) wavefunctions.
               
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