Multiply-excited states and their contribution to opacity in CO2 laser-driven tin-plasma conditions
J. Phys. B: At. Mol. Opt. Phys. , Volume 54 - Issue 3 p. 035002: 1- 11
A recent study [Nat. Commun. 11, 2334 (2020)] has found that transitions between multiply-excited configurations in open 4d-subshell tin ions are the dominant contributors to intense EUV emission from dense, Nd:YAG-driven (laser wavelength = 1.064 micrometres) tin plasmas. In the present study, we employ the Los Alamos Atomic code to investigate the spectral contribution from these transitions under industrially-relevant, CO2 laser-driven (laser wavelength = 10.6 micrometres) tin plasma conditions. First, we employ Busquet's ionisation temperature method to match the average charge state <Z> of a non-local- thermodynamic equilibrium (non-LTE) plasma with an LTE one. This is done by varying the temperature of the LTE calculations until a so-called ionisation temperature T_Z is established. Importantly, this approach generates LTE-computed configuration populations in excellent agreement with the non-LTE populations. A corollary of this observation is that the non-LTE populations are well-described by Boltzmann-type exponential distributions having effective temperatures T_eff approximately equal to T_Z. In the second part of this work, we perform extensive level-resolved LTE opacity calculations at T_Z. It is found that 66% of the opacity in the industrially-relevant 2% bandwidth centered at 13.5 nm arises from transitions between multiply-excited states. These results reinforce the need for the consideration of complex, multiply-excited states in modelling the radiative properties of laser-driven plasma sources of EUV light.
|ERC , NWO|
|J. Phys. B: At. Mol. Opt. Phys.|
|Organisation||EUV Plasma Processes|
Sheil, J, Versolato, O.O, Neukirch, A.J, & Colgan, J. (2021). Multiply-excited states and their contribution to opacity in CO2 laser-driven tin-plasma conditions. J. Phys. B: At. Mol. Opt. Phys., 54(3), 035002: 1–035002:11. doi:10.1088/1361-6455/abcedf