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Cross sections of transitions between Tm excited states on collisions with Ne and Xe atoms

Evgenii B. Aleksandrov, В. И. Попов, V. K. Prilipko, L. Yu. Khryashchev

Published May 1, 1986• 0 citations
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Collisional redistribution in transitions between excited states

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AIP conference proceedings•Jan 1, 1990•0 citations

Inelastic collisions between selectively excited rubidium 6D2 -state atoms and noble-gas atoms: Fine-structure-state mixing

Byron George Zollars, Hans A. Schuessler, Joel Wm. Parker +1 more

Inelastic collisional processes in fine-structure-state mixing have been studied by selective stepwise excitation and observation of the resulting fluorescence during collisions of excited rubidium $6^{2}D_{\frac{5}{2}}$ state atoms with various noble-gas atoms. It is shown that for intermediately excited rubidium atoms the fine-structure-state mixing cross sections are generally increasing from helium to xexon. The cross sections for the process $\mathrm{Rb}(6^{2}D_{\frac{5}{2}})+A(n^{1}S_{0})\ensuremath{\rightarrow}\mathrm{Rb}(6^{2}D_{\frac{3}{2}})+A(n^{1}S_{0})+\ensuremath{\Delta}E$ have the values ${\ensuremath{\sigma}}_{\mathrm{fs}}^{*}=2.4\ifmmode\pm\else\textpm\fi{}0.9, 3.1\ifmmode\pm\else\textpm\fi{}1.2, 2.6\ifmmode\pm\else\textpm\fi{}1.0, 5.8\ifmmode\pm\else\textpm\fi{}2.2, \mathrm{and} 9.3\ifmmode\pm\else\textpm\fi{}5.6$ in units of ${10}^{\ensuremath{-}14}$ ${\mathrm{cm}}^{2}$, where $A$ denotes in sequence any one of the noble gas atoms He, Ne, Ar, Kr, and Xe, respectively. Transfer cross sections for the transfer of excited Rb$6^{2}D$-state atoms out of the doublet were also determined and are about an order of magnitude smaller than the fine-structure-mixing cross sections.

Physical Review A•Sep 1, 1983•9 citations

Deexcitation of Rydberg states of He by He, Ne, Ar, Kr, and Xe

A. Hitachi, Christopher Davies, Terence A. King +2 more

The total quenching cross sections for $\mathrm{He}({n}^{1,3}S)(2\ensuremath{\le}n\ensuremath{\le}11)$ states by thermal collisions [600(+ 200, - 100) K] with He, Ne, Ar, Kr, and Xe have been measured. The main quenching mechanism is attributed to Penning ionization for lower $n$, and collisional angular-momentum transfer for highly excited states. Measured cross sections are of the order of ${10}^{\ensuremath{-}15}$ to ${10}^{\ensuremath{-}14}$, ${\mathrm{cm}}^{2}$. The values for higher $n$ states are much smaller than the geometrical cross section; this is explained by a relatively large energy spread between the $S$ state and $l\ensuremath{\ge}1$ states.

Physical Review A•Sep 1, 1980•24 citations

Energy transfer in collisions between excited atoms

A. Kopystyńska, L. Moi

Physics Reports•Dec 1, 1982•59 citations

Collisions of Highly Excited Atoms

R. F. Stebbings

Advances in atomic and molecular physics•Jan 1, 1979•8 citations

Fine-structure mixing in the 9D state of caesium induced in collisions with noble-gas atoms

M. Łukaszewski, I. Jackowska

Cross sections for the transfer of excitation between fine-structure sublevels of the 9D state of caesium due to collisions with noble-gas atoms are measured. The experimental method employs stepwise excitation with a pulsed dye laser in the second step (6 2 P 3/2 to 9 2 D 5/2 ) and time-resolved detection of sensitised fluorescence 9 2 D 3/2 to 6 2 P 1/2 . The cross sections for the process Cs(9 2 D 3/2 )+A to Cs(9 2 D 5/2 )+A are (in units of 10 -14 cm 2 ) 7.6(1.5), 2.5(5), 2.7(5), 3.0(6) and 3.2(6) for A=He, Ne, Ar, Kr and Xe, respectively. For all the noble gases except helium the experimental cross sections are a few times smaller than the ones obtained in a recent semiclassical calculation.

Journal of Physics B Atomic Molecular and Optical Physics•Nov 14, 1988•5 citations
Inelastic collisional processes in fine-structure-state mixing have been studied by selective stepwise excitation and observation of the resulting fluorescence during collisions of excited rubidium 62D526^{2}D_{\frac{5}{2}}62D25​​ state atoms with various noble-gas atoms. It is shown that for intermediately excited rubidium atoms the fine-structure-state mixing cross sections are generally increasing from helium to xexon. The cross sections for the process $\mathrm{Rb}(6^{2}D_{\frac{5}{2}})+A(n^{1}S_{0})\ensuremath{\rightarrow}\mathrm{Rb}(6^{2}D_{\frac{3}{2}})+A(n^{1}S_{0})+\ensuremath{\Delta}E$ have the values ${\ensuremath{\sigma}}_{\mathrm{fs}}^{*}=2.4\ifmmode\pm\else\textpm\fi{}0.9, 3.1\ifmmode\pm\else\textpm\fi{}1.2, 2.6\ifmmode\pm\else\textpm\fi{}1.0, 5.8\ifmmode\pm\else\textpm\fi{}2.2, \mathrm{and} 9.3\ifmmode\pm\else\textpm\fi{}5.6$ in units of ${10}^{\ensuremath{-}14}$ cm2{\mathrm{cm}}^{2}cm2, where AAA denotes in sequence any one of the noble gas atoms He, Ne, Ar, Kr, and Xe, respectively. Transfer cross sections for the transfer of excited Rb62D6^{2}D62D-state atoms out of the doublet were also determined and are about an order of magnitude smaller than the fine-structure-mixing cross sections.
The total quenching cross sections for $\mathrm{He}({n}^{1,3}S)(2\ensuremath{\le}n\ensuremath{\le}11)$ states by thermal collisions [600(+ 200, - 100) K] with He, Ne, Ar, Kr, and Xe have been measured. The main quenching mechanism is attributed to Penning ionization for lower nnn, and collisional angular-momentum transfer for highly excited states. Measured cross sections are of the order of ${10}^{\ensuremath{-}15}$ to ${10}^{\ensuremath{-}14}$, cm2{\mathrm{cm}}^{2}cm2. The values for higher nnn states are much smaller than the geometrical cross section; this is explained by a relatively large energy spread between the SSS state and $l\ensuremath{\ge}1$ states.
Cross sections for the transfer of excitation between fine-structure sublevels of the 9D state of caesium due to collisions with noble-gas atoms are measured. The experimental method employs stepwise excitation with a pulsed dye laser in the second step (6 2 P 3/2 to 9 2 D 5/2 ) and time-resolved detection of sensitised fluorescence 9 2 D 3/2 to 6 2 P 1/2 . The cross sections for the process Cs(9 2 D 3/2 )+A to Cs(9 2 D 5/2 )+A are (in units of 10 -14 cm 2 ) 7.6(1.5), 2.5(5), 2.7(5), 3.0(6) and 3.2(6) for A=He, Ne, Ar, Kr and Xe, respectively. For all the noble gases except helium the experimental cross sections are a few times smaller than the ones obtained in a recent semiclassical calculation.