1990
DOI: 10.1007/bf01437526
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The state dependence of the interaction of metastable rare gas atoms Rg*(ms3 P 2,3 P 0) (Rg=Ne, Ar, Kr, Xe) with ground state sodium atoms

Abstract: The state dependence of the interaction of metastable rare gas atoms Rg* (ms 3P2, 3P0) (Rg = Ne, Ar, Kr, Xe) with ground state sodium atoms Schohl, S.; Müller, M.W.; Meijer, H.A.J.; Ruf, M.-W.; Hotop, H.; Morgner, H. Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Schohl, S., Müller, M. W., Meijer, H. A. J., Ruf, M-W., Hotop, H., & Morgner, H. (1990). The state dependence of the interaction of metastable rare gas atoms Rg* (ms 3P2, 3P0) (Rg = Ne, Ar, … Show more

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Cited by 19 publications
(20 citation statements)
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“…which is a direct, simple and useful prescription to estimate well depths for Penning ionizing quasi-molecules, as exploited, e.g., for He (2 3S, 2 1S) + alkali atoms [34] and for Rg* + Na (3s) [44] (Rg* = metastable 3P 2 and 3P 0 of Ne, Ar, Kr, Xe) For triatomic Penning ionization systems, as discussed here, the potential surfaces depend on two variables, i.e. on the distance R (taken to be the distance between the center of the metastable rare gas atom Rg* and the midpoint of the diatomic target molecule) and on the angle O between the vector R and the molecular axis r (we choose O = 0 ° to correspond to the coil±near conformation Rg* -H -F, while O = 180 ° describes coil±near Rg* approach towards the F-end).…”
Section: Resultsmentioning
confidence: 99%
“…which is a direct, simple and useful prescription to estimate well depths for Penning ionizing quasi-molecules, as exploited, e.g., for He (2 3S, 2 1S) + alkali atoms [34] and for Rg* + Na (3s) [44] (Rg* = metastable 3P 2 and 3P 0 of Ne, Ar, Kr, Xe) For triatomic Penning ionization systems, as discussed here, the potential surfaces depend on two variables, i.e. on the distance R (taken to be the distance between the center of the metastable rare gas atom Rg* and the midpoint of the diatomic target molecule) and on the angle O between the vector R and the molecular axis r (we choose O = 0 ° to correspond to the coil±near conformation Rg* -H -F, while O = 180 ° describes coil±near Rg* approach towards the F-end).…”
Section: Resultsmentioning
confidence: 99%
“…The metastable neon atoms are produced in a differentially pumped cold cathode dc discharge. The metastable beam contains neon atoms in the 3P 2-and 3Po-state, favouring the 3P2 species (j(3~)/j(3Po)~ 5/1 [23,27]). Since, in addition, the cross section a2 for Ne*(3P2)+ H collisions is considerably larger than the corresponding cross section ao for Ne*(3Po) + H, i.e.…”
Section: Methodsmentioning
confidence: 99%
“…In particular, rather detailed information exists for the basic processes He*(2 3S, 21S)+H/D [10,13,[18][19][20], which may be regarded as prototype systems for autoionizing collision complexes at thermal energies, while less effort was devoted to the investigation of heavier metastable noble gases [21][22][23][24][25].…”
Section: Introductionmentioning
confidence: 99%
“…The metastable atom beam was collimated by a 2mm wide and 1 mm high slit at a distance of 348 mm from the source exit hole (solid angle 1.7.10-Ssr). Table 6 summarizes the relevant quantities needed in the procedure Present results of the total, photon-corrected detector currents for fresh graphite surface and comparable source gas densities b Flux into a solid angle of 1.7-10 -5 sr ° [201 a [13,19,20] o Evaluated for the region of laser photoionization (distance from source 348 ram); average velodties as given in (7) and the determined fluxes F 2 and densities n 2. Interestingly, almost equal densities are found for Ne*, At*, and Kr*.…”
Section: Absolute Metastable Atom Fluxes and Densitiesmentioning
confidence: 99%
“…Reactions of metastable rare gas atoms Rg* with photons, electrons, atoms, molecules, and surfaces are ac-* Dedicated to Prof. Dr. Wilhelm Hanle on the occasion of his 90th birthday "~" Present address: Fysisk Laboratorium, H.C. Orsted Institutet, DK-2100 Copenhagen, Denmark *'~ Permanent address: Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, 80309-0440, USA tively studied by molecular beam techniques [1][2][3][4][5][6][7][8][9][10][11][12][13][14][15][16].…”
Section: Introductionmentioning
confidence: 99%