Phys. Rev. A 54, 1372 - 1384 (1996)

Energy-pooling collisions in cesium: 6PJ+6PJ→6S+(nl=7P,6D,8S,4F)

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Z. J. Jabbour, R. K. Namiotka, and J. Huennekens
Department of Physics, Lehigh University, 16 Memorial Drive East, Bethlehem, Pennsylvania 18015

M. Allegrini, S. Milošević, and F. de Tomasi
Unità INFM, Dipartimento di Fisica, Università di Pisa, Piazza Torricelli 2, 56126 Pisa, Italy

Received 25 September 1995

We report experimental rate coefficients for the energy-pooling collisions Cs(6P1/2)+Cs(6P1/2)→Cs(6S1/2)+Cs(nlJ) and Cs(6P3/2)+Cs(6P3/2)→Cs(6S1/2)+Cs(nlJ) where nlJ=7P1/2, 7P3/2, 6D3/2, 6D5/2, 8S1/2, 4F5/2, or 4F7/2. Atoms were excited to either the 6P1/2 or 6P3/2 state using a single-mode Ti:sapphire laser. The excited-atom density and spatial distribution were mapped by monitoring the absorption of a counterpropagating single-mode ring dye laser beam, tuned to either the 6P1/2→8S1/2 or 6P3/2→7D3/2,5/2 transitions, which could be translated parallel to the pump beam. Transmission factors, which describe the average probability that photons emitted within the fluorescence detection region can pass through the optically thick vapor without being absorbed, were calculated for all relevant transitions. Effective lifetimes of levels populated by energy-pooling collisions are modified by radiation trapping, and these factors were calculated using the Molisch theory. These calculated quantities have been combined with the measured excited-atom densities and fluorescence ratios to yield absolute energy-pooling rate coefficients. It was found that the rate for production, in all cases, is greatest for 6D, but that 1/2-1/2 collisions are significantly more efficient than 3/2-3/2 collisions for populating 7P. It was also found that 7P1/2 is populated two to three times more efficiently than 7P3/2 in 1/2-1/2 collisions, but that the 7P fine-structure levels are approximately equally populated in 3/2-3/2 collisions. © 1996 The American Physical Society.


©1996 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevA.54.1372
DOI: 10.1103/PhysRevA.54.1372
PACS: 34.50.Rk, 34.90.+q

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