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Temperature dependence of xenon excimer formations using two-photon absorption laser-induced fluorescence
Frédéric Marchal, Neermalsing Sewraj, G Jabbour, Peyo Rodriguez Akerreta, Gerald Ledru

Temperature dependence of xenon excimer formations using two-photon absorption laser-induced fluorescence

Science & Mathematics Published 2010 Verification Pending

Overview & Synopsis

The temporal dependence of VUV emissions of the first continuum of xenon at around 150 nm are investigated for pressures ranging from 10 to 100 Torr and for temperatures ranging from 200 to 300 K, after briefly and selectively populating exclusively the resonant or the metastable atomic states of the 5p 5 6s configuration. A kinetic and spectroscopic study was performed by analyzing the VUV post luminescence decay of xenon operating with such excitation conditions. Our results clearly show the temperature effects on the rate constants α 31 and α 32 of formation of excimers correlated respectively to the first resonant and the first metastable states by three-body collisions. The resulting reaction rates are obtained as a function of temperature T: α 31 = 3.90 × 10 −27 T −1.78 cm −6 s −1, α 32 = 1.34 × 10 −27 T −1.70 cm −6 s −1. For the whole pressure range, low temperatures favour the formation of xenon excimers and the efficiency of the three-body collisions in forming stabilized excimers increases with decreasing temperature

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Document Information

Document Title Temperature dependence of xenon excimer formations using two-photon absorption laser-induced fluorescence
Author / Organization Frédéric Marchal, Neermalsing Sewraj, G Jabbour, Peyo Rodriguez Akerreta, Gerald Ledru
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2010
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-125392
Original Source Link Visit Source Page on hal.science »