NASA NTRS · 19960025067
Modification of Einstein A Coefficient in Dissipative Gas Medium
Abstract
Spontaneous radiation in dissipative gas medium such as plasmas is investigated by Langevin equations and the modified Weisskopf-Wigner approximation. Since the refractive index of gas medium is expected to be nearly unity, we shall first neglect the medium polarization effect. We show that absorption in plasmas may in certain case modify the Einstein A coefficient significantly and cause a pit in the A coefficient-density curves for relatively low temperature plasmas and also a pit in the A coefficient-temperature curves. In the next, the effect of medium polarization is taken into account in addition. To our surprise, its effect in certain case is quite significant. The dispersive curves show different behaviors in different region of parameters.
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Cao, Chang-Qi, Cao, Hui, Qin, Ke-Cheng. 1996-01-01. Modification of Einstein A Coefficient in Dissipative Gas Medium. https://ntrs.nasa.gov/citations/19960025067
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