2009
DOI: 10.1088/0031-8949/79/04/045302
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Gain coefficient calculation for short wave laser emission from nickel-like Sm

Abstract: The energy levels, transition probabilities and effective collision strengths for the 1s22s22p63s23p63d10 and the 1s22s22p63s23p63d94l (l=s, p, d and f) states of nickel-like Sm are used in the calculation of the reduced population of 55 fine structure levels over a wide range of electron density values (from 1020 to 4×1022) and at various electron plasma temperatures. For those transitions with positive population inversion factor, the gain coefficients are evaluated and plotted against the electron density.

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Cited by 5 publications
(3 citation statements)
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“…This result is in agreement with that of Feldman et al [14,15,19]. See also the data for nickel-like Sm , W, and Eu [20][21][22].At high electron densities ( ), the radiative decay to all the levels will be negligible compared to collisional depopulations and all the level populations become independent of the electron density (see Figures 1-3). The (3d 3/2 4d 3/2 ) 0 level has higher population density from electron density 10 21 to 10 22 cm −3 than the other levels at electron temperature 0.5 KeV, from electron density 10 21 to 2 × 10 22 cm −3 at electron temperature 1 KeV, and from electron density 10 21 to 4 × 10 22 cm −3 at electron temperature 1.5 KeV which mean that the population inversion occur in these ranges.…”
Section: Level Populationsupporting
confidence: 90%
“…This result is in agreement with that of Feldman et al [14,15,19]. See also the data for nickel-like Sm , W, and Eu [20][21][22].At high electron densities ( ), the radiative decay to all the levels will be negligible compared to collisional depopulations and all the level populations become independent of the electron density (see Figures 1-3). The (3d 3/2 4d 3/2 ) 0 level has higher population density from electron density 10 21 to 10 22 cm −3 than the other levels at electron temperature 0.5 KeV, from electron density 10 21 to 2 × 10 22 cm −3 at electron temperature 1 KeV, and from electron density 10 21 to 4 × 10 22 cm −3 at electron temperature 1.5 KeV which mean that the population inversion occur in these ranges.…”
Section: Level Populationsupporting
confidence: 90%
“…[19,20,26]. See also our data for nickel-like Sm and W [27,28]. At high population densities (N e 410 23 ), radiative decay to all levels will be negligible compared to collisional depopulations and all level populations become independent of electron density and are approximately equal.…”
Section: Level Populationmentioning
confidence: 76%
“…We expect that at high densities (N e > 10 20 cm -3 ), radiative decay to all levels will be negligible compared to collisional depopulations and all level population become independent of electron density and are approximately the same (see ref. [16][17][18]). The population inversion is largest when electron collisional de-excitation rate for the upper level is comparable to the radiative decay of this level [10].…”
Section: Level Populationsmentioning
confidence: 99%