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BEYOND THE QUASISTATIC LIMIT FOR IONIC PERTURBERS: HOT AND DENSE PLASMAS AND/OR HYDROGENIC EMITTER


In the case of dense and hot plasmas, interactions with ionic perturbers become a major source of broadening. Due to the linear Stark effect, it is the same situation whether the emitter is an H atom or an hydrogenic ion. The quasistatic approximation used for ionic broadening at low densities is no longer valid and simultaneous strong interactions between the radiator and the surrounding perturbers must be taken into account. Much effort has been devoted to this many body dynamical problem both on the methods and the applications. Important results have been obtained theoretically or experimentally for lines of H (35-37), He (36,38,39), N V (40) and multicharged hydrogenic ions (41). Extensive tables (42) and parametrized formulae (43) are available. Analytic expressions have been obtained for the lines of one electron ions (44), and wing formulae for plasma broadened spectral lines of hydrogenic ions (45). Ion dynamics effects are also studied in He lines (46-49).


Far wings of the Lyman line of H have been studied in a quasi molecular approach in the physical conditions of white dwarfs (50).




Jim Esmond
Wed Oct 30 13:33:17 EST 1996