1995
DOI: 10.1088/0022-3727/28/7/015
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Characterization of imprisoned Xe resonant photons in He-Xe and Ne-Xe mixtures

Abstract: The Holstein's theory of the imprisonment of resonance radiation for pressure-broadened Lorentzian profiles is extended to the Xe-based binary gas mixtures which are widely employed in practical discharge devices. In the binary mixtures, collisions between radiating and buffer atoms modify the emission and absorption spectrum profiles, affecting the imprisonment characteristics. It is found that the imprisonment time Tp is independent of total or partial pressures, provided that the Xe mixture ratio m and disc… Show more

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Cited by 34 publications
(22 citation statements)
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“…The intensity of the 147-nm resonance line saturates with respect to the discharge current due to electronic de-excitation of the excited Xe atoms. 9 This so-called plasma saturation causes luminous-efficiency deterioration. An increase of the drive frequency enhances the saturation since the excited Xe atoms are more likely to be destroyed by the discharge current in the following sustain pulse.…”
Section: Luminous Efficiency and Luminance Vs Xe Content And Frequencymentioning
confidence: 99%
“…The intensity of the 147-nm resonance line saturates with respect to the discharge current due to electronic de-excitation of the excited Xe atoms. 9 This so-called plasma saturation causes luminous-efficiency deterioration. An increase of the drive frequency enhances the saturation since the excited Xe atoms are more likely to be destroyed by the discharge current in the following sustain pulse.…”
Section: Luminous Efficiency and Luminance Vs Xe Content And Frequencymentioning
confidence: 99%
“…The same approach has been applied to the other resonance line, 185 nm, which is also reabsorbed. 53,64,74,75 In the general case, the effective transition probability can be estimated using the formulas of Igarashi et al 76 for a mixture of gases or the analytical formulas derived by Curry and Lawler. 77,78 The pressure broadening due to Ar atoms is accounted for through the parameter ␥ ϭvn Ar /2, where is the interaction cross section, v is the relative velocity, and n Ar is the argon density.…”
Section: Atomic Datamentioning
confidence: 99%
“…The escape factors provide effective lifetimes for the radiative transitions and depend on the lower state density, the gas temperature, and the bulb dimensions. The general formulas for the escape factors are taken from [45].…”
Section: A Model Componentsmentioning
confidence: 99%