1997
DOI: 10.1016/s0022-4073(97)00095-2
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Resonance radiation transfer in dense dispersive media

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Cited by 5 publications
(2 citation statements)
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“…The self-absorbed 396.15 nm resonant line exhibits a peak at its central wavelength. Such a feature has been already reported 24,27 in the case of sodium resonant transitions in a high pressure ͑0.7-2.9 bars͒ lamp discharge. However, the populating processes and spectral broadening mechanisms are strongly different from ours: the temperature is about 1000 K, the atomic density ranges from 10 24 to 10 25 m −3 , and the electron density from 10 21 to 10 22 m −3 .…”
Section: Introductionsupporting
confidence: 74%
“…The self-absorbed 396.15 nm resonant line exhibits a peak at its central wavelength. Such a feature has been already reported 24,27 in the case of sodium resonant transitions in a high pressure ͑0.7-2.9 bars͒ lamp discharge. However, the populating processes and spectral broadening mechanisms are strongly different from ours: the temperature is about 1000 K, the atomic density ranges from 10 24 to 10 25 m −3 , and the electron density from 10 21 to 10 22 m −3 .…”
Section: Introductionsupporting
confidence: 74%
“…In the broad range of conditions in plasmas and gases, where the complete redistribution (CRD) in photon frequency within the resonance line shape is applicable, the radiative transfer is described by the Biberman-Holstein equation for the density of excited atoms [9,10] and characterized by the infinite mean-squared displacement of the initial perturbation [11] and, respectively, by the irreducibility of the integral equation, in space variables, to a differential one. This makes the respective radiative transfer a nonlocal (superdiffusive) one [12,13] (for the deviation from the CRD and the limits of its applicability see, e.g., [14][15][16]). …”
Section: Introductionmentioning
confidence: 99%