1. Temperature and density dependence of Kr L-shell spectrum in hot dense plasmas.
- Author
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Gallardo-Diaz, E., Mancini, R. C., Carpenter, K. R., Adrian, P., Frenje, J., and Florido, R.
- Subjects
HIGH temperature plasmas ,X-ray spectroscopy ,ACTION spectrum ,SPECTRAL lines ,ELECTRON temperature ,INERTIAL confinement fusion ,DENSE plasmas - Abstract
Kr L-shell spectroscopy modeling results are discussed in this paper, focusing on the n = 4 to n = 2 line transitions of Be- and Li-like Kr ions. Collisional radiative atomic kinetic and Stark-broadened spectral line shape calculations show electron temperature T e and density n e sensitivity in the spectrum. The combination of the T e dependence due to the relative intensity of Be-like to Li-like line emissions in the range from 1.5 to 3 keV and the n e sensitivity from the Stark broadening effect on the line shapes in the range from 5 × 10 23 to 2 × 10 24 / cc results in a spectrum that can be employed to diagnose T e and n e . Two different collisional radiative atomic kinetic models i.e., Prismspect [J. J. MacFarlane, et al., Int. Fusion Sci. Appl. Conf. Proc. 457 (2003)] and ABAKO [Florido, et al., PRE, 80, 056402 (2009)] produce similar results in level populations and spectra. In x-ray spectroscopy of implosion cores, this Kr L-shell spectrum may prove useful in an intermediate T e range in which Ar is too ionized for its K-shell to be of diagnostic value and Kr is not ionized enough for its K-shell emission to be useful. [ABSTRACT FROM AUTHOR]
- Published
- 2024
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