LABORATORY STUDY OF RATE COEFFICIENTS FOR H{sub 2}O:He INELASTIC COLLISIONS BETWEEN 20 AND 120 K
Abstract
Statetostate rate coefficients for orthoH{sub 2}O:He and paraH{sub 2}O:He inelastic collisions in the 20120 K thermal range are investigated by means of an improved experimental procedure. This procedure is based on the use of a kinetic master equation (MEQ) which describes the evolution of populations of H{sub 2}O rotational levels along a supersonic jet of H{sub 2}O highly diluted in helium. The MEQ is expressed in terms of experimental observables and rate coefficients for H{sub 2}O:He inelastic collisions. The primary experimental observables are the local number density and the populations of the rotational energy levels of H{sub 2}O, quantities which are determined along the jet with unprecedented accuracy by means of Raman spectroscopy with high space resolution. Sets of rate coefficients from the literature and from present closecoupling calculations using two different potential energy surfaces (PESs) have been tested against the experiment. The Green et al. rate coefficients are up to 50% too low compared to the experiment, while most rates calculated here from the Hodges et al. PES and the Patkowski et al. PES are much closer to the experimental values. Experimental rates with an estimated accuracy on the order of 10% have been obtained for orthoH{sub 2}O:He and paraH{sub 2}O:He inelasticmore »
 Authors:
 Laboratory of Molecular Fluid Dynamics, Instituto de Estructura de la Materia, CSIC Serrano 121, E28006 Madrid (Spain)
 Instituto de Física Fundamental, CSIC Serrano 123, E28006 Madrid (Spain)
 Publication Date:
 OSTI Identifier:
 22340122
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Astrophysical Journal, Supplement Series; Journal Volume: 216; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 74 ATOMIC AND MOLECULAR PHYSICS; 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ACCURACY; DENSITY; ENERGY LEVELS; HELIUM; KINETIC EQUATIONS; MOLECULE COLLISIONS; POTENTIAL ENERGY; RAMAN SPECTROSCOPY; ROTATIONAL STATES; SPATIAL RESOLUTION; WATER
Citation Formats
Tejeda, G., Moreno, E., Fernández, J. M., Montero, S., CarmonaNovillo, E., and Hernández, M. I., Email: emsalvador@iem.cfmac.csic.es. LABORATORY STUDY OF RATE COEFFICIENTS FOR H{sub 2}O:He INELASTIC COLLISIONS BETWEEN 20 AND 120 K. United States: N. p., 2015.
Web. doi:10.1088/00670049/216/1/3.
Tejeda, G., Moreno, E., Fernández, J. M., Montero, S., CarmonaNovillo, E., & Hernández, M. I., Email: emsalvador@iem.cfmac.csic.es. LABORATORY STUDY OF RATE COEFFICIENTS FOR H{sub 2}O:He INELASTIC COLLISIONS BETWEEN 20 AND 120 K. United States. doi:10.1088/00670049/216/1/3.
Tejeda, G., Moreno, E., Fernández, J. M., Montero, S., CarmonaNovillo, E., and Hernández, M. I., Email: emsalvador@iem.cfmac.csic.es. 2015.
"LABORATORY STUDY OF RATE COEFFICIENTS FOR H{sub 2}O:He INELASTIC COLLISIONS BETWEEN 20 AND 120 K". United States.
doi:10.1088/00670049/216/1/3.
@article{osti_22340122,
title = {LABORATORY STUDY OF RATE COEFFICIENTS FOR H{sub 2}O:He INELASTIC COLLISIONS BETWEEN 20 AND 120 K},
author = {Tejeda, G. and Moreno, E. and Fernández, J. M. and Montero, S. and CarmonaNovillo, E. and Hernández, M. I., Email: emsalvador@iem.cfmac.csic.es},
abstractNote = {Statetostate rate coefficients for orthoH{sub 2}O:He and paraH{sub 2}O:He inelastic collisions in the 20120 K thermal range are investigated by means of an improved experimental procedure. This procedure is based on the use of a kinetic master equation (MEQ) which describes the evolution of populations of H{sub 2}O rotational levels along a supersonic jet of H{sub 2}O highly diluted in helium. The MEQ is expressed in terms of experimental observables and rate coefficients for H{sub 2}O:He inelastic collisions. The primary experimental observables are the local number density and the populations of the rotational energy levels of H{sub 2}O, quantities which are determined along the jet with unprecedented accuracy by means of Raman spectroscopy with high space resolution. Sets of rate coefficients from the literature and from present closecoupling calculations using two different potential energy surfaces (PESs) have been tested against the experiment. The Green et al. rate coefficients are up to 50% too low compared to the experiment, while most rates calculated here from the Hodges et al. PES and the Patkowski et al. PES are much closer to the experimental values. Experimental rates with an estimated accuracy on the order of 10% have been obtained for orthoH{sub 2}O:He and paraH{sub 2}O:He inelastic collisions between 20 and 120 K by scaling and averaging the theoretical rates to the experiment.},
doi = {10.1088/00670049/216/1/3},
journal = {Astrophysical Journal, Supplement Series},
number = 1,
volume = 216,
place = {United States},
year = 2015,
month = 1
}

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