Abstract:
It is shown that the 31D–21P transition in helium-like ions is of interest for the amplification of light of wavelengths λ < 50 nm. An analytic formula is derived for the gain due to this transition. An analysis is made of the time dependence of the gain in the model of consecutive recombination during vacuum expansion of an initially completely ionized plasma filament. An allowance is made for the recombination heating of electrons, reabsorption due to the 21P–11S0 radiative transition, and changes in the ion composition of the plasma during its expansion. It is shown that the maximum value of the gain for the C v ion [λ (31D–21P) = 26.7 nm] is ~1 cm–1.