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Quenching of 6s6d and 6s7d Hg atoms by Hg*-Hg,Hg*-Ar and Hg*-N2 collisions
Institution:1. Department of Earth and Environmental Sciences and Williamson Research Centre for Molecular Environmental Science, University of Manchester, Manchester M13 9PL, UK;2. Departamento de Geología, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Santiago, Chile;3. Centro de Excelencia en Geotermia de Los Andes (CEGA), Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Santiago, Chile;4. Scottish Universities Environmental Research Centre, East Kilbride G75 0QF, UK
Abstract:The radiative decays and collisional quenching of Hg 61D2, 63D2, 71D2 and 73D2 atoms were investigated by time-resolved methods. Hg vapour, pure or mixed with a buffer gas in a fluorescence cell, was irradiated with u.v. light pulses from a frequency-doubled N2 laser-pumped dye laser, populating selectively each state in turn by 2-photon absorption from the 61S0 ground state. Fluorescent components arising from the decays to the 61P1 or 63S0 state were resolved with a spectrometer and their time evolutions recorded with a transient digitizer or time-to-amplitude converter and pulse-height analyzer, yielding the respective decay rates. The quenching cross sections were obtained from variations of measured decay rates with Hg or buffer-gas density.
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