STATE TO STATE ROTATIONAL ENERGY TRANSFER N THE $\nu_{2}$ = 1 STATE OF AMMONIA*

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1992

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Ohio State University

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Time-resolved infrared double-resonance is used to study state-resolved rational energy transfer in ammonia 14NH3) self-collisions and between ammonia and foreign gases. NH3 molecules are prepared in selected rovibrational stales of the v2=1 level using coincidences between CO2 laser lines and v2 fundamental transitions. Measurements of both the total depopulation rate and the rates of transfer into specific final rovibrational sates (v,J,K) have been carried out. For NH3NH3 collisions, total depopulations rates and ground-state recovery rates are found to be three and eight times larger, respectively, than the Lennard-Jones collision rate, in accord with theoretical expectations for polar molecules. A kinetic master equation analysis of time-resolved level populations yields state to state rate constants and propensity rules for NH3NH3 and NH3Ar collisions. Individual rotational energy transfer rates in v2=1 are slower than in the vibrational ground state. but still comparable to the Lennard-Jones collision frequency. Our experiments show that rotational energy transfer in v2=1 is not governed by simple ``dipole like” selection rules. They show fast rotational energy transfer, which can be related to long range interaction potentials, but at the same time considerable amounts of ΔJ= 2,3 and ΔK = 3 transitions, which may be attributed to higher order terms in the multipole expansion of the intermolecular potential. No pronounced symmetry-state correlation and no preferred pathways were found except the preference for relaxation within a K-stack and expected separate relaxation of different nuclear spin species. Rates of collision induced symmetry change (a<−>s) in this region are on the order of $k_{as}= 4 $ μs−1 torr,−1 smaller than kas in the ground state, but over an order of magnitude larger than that recently reported the literature for v2=1. Depopulation rates for other collision partners (Ar, H2, N2, and He) can be understood in terms of the intermolecular potentials. Comparisons are made between the relaxation rates measured in this work and infrared pressure-broadening coefficients reported in the literature.

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*Work supported by NASA Grants NAGW-1667 and NAGW-2387 and N.S.F. Grant CHE89-14953 to the G.R. Harrison Spectroscopy Laboratory.


Author Institution: Institut f""{u}r Physikalische Chemie, Universit'{a}t G""{o}ttingen; Department of Chemistry, G.R. Harrison Spectroscopy Laboratory

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