Determination of the evaporation coefficient of D<sub>2</sub>O

The evaporation rate of D<sub>2</sub>O has been determined by Raman thermometry of a droplet train (12–15 μm diameter) injected into vacuum (~10<sup>-5</sup> torr). The cooling rate measured as a function of time in vacuum was fit to a model that accounts for temperature grad...

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Main Authors: R. C. Cohen, R. J. Saykally, J. D. Smith, C. D. Cappa, W. S. Drisdell
Format: Article
Language:English
Published: Copernicus Publications 2008-11-01
Series:Atmospheric Chemistry and Physics
Online Access:http://www.atmos-chem-phys.net/8/6699/2008/acp-8-6699-2008.pdf
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spelling doaj-2214addea9594ed09a96410d1b97056a2020-11-24T20:56:13ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242008-11-0182266996706Determination of the evaporation coefficient of D<sub>2</sub>OR. C. CohenR. J. SaykallyJ. D. SmithC. D. CappaW. S. DrisdellThe evaporation rate of D<sub>2</sub>O has been determined by Raman thermometry of a droplet train (12–15 μm diameter) injected into vacuum (~10<sup>-5</sup> torr). The cooling rate measured as a function of time in vacuum was fit to a model that accounts for temperature gradients between the surface and the core of the droplets, yielding an evaporation coefficient (&gamma;<sub>e</sub>) of 0.57&plusmn;0.06. This is nearly identical to that found for H<sub>2</sub>O (0.62&plusmn;0.09) using the same experimental method and model, and indicates the existence of a kinetic barrier to evaporation. The application of a recently developed transition-state theory (TST) model suggests that the kinetic barrier is due to librational and hindered translational motions at the liquid surface, and that the lack of an isotope effect is due to competing energetic and entropic factors. The implications of these results for cloud and aerosol particles in the atmosphere are discussed. http://www.atmos-chem-phys.net/8/6699/2008/acp-8-6699-2008.pdf
collection DOAJ
language English
format Article
sources DOAJ
author R. C. Cohen
R. J. Saykally
J. D. Smith
C. D. Cappa
W. S. Drisdell
spellingShingle R. C. Cohen
R. J. Saykally
J. D. Smith
C. D. Cappa
W. S. Drisdell
Determination of the evaporation coefficient of D<sub>2</sub>O
Atmospheric Chemistry and Physics
author_facet R. C. Cohen
R. J. Saykally
J. D. Smith
C. D. Cappa
W. S. Drisdell
author_sort R. C. Cohen
title Determination of the evaporation coefficient of D<sub>2</sub>O
title_short Determination of the evaporation coefficient of D<sub>2</sub>O
title_full Determination of the evaporation coefficient of D<sub>2</sub>O
title_fullStr Determination of the evaporation coefficient of D<sub>2</sub>O
title_full_unstemmed Determination of the evaporation coefficient of D<sub>2</sub>O
title_sort determination of the evaporation coefficient of d<sub>2</sub>o
publisher Copernicus Publications
series Atmospheric Chemistry and Physics
issn 1680-7316
1680-7324
publishDate 2008-11-01
description The evaporation rate of D<sub>2</sub>O has been determined by Raman thermometry of a droplet train (12–15 μm diameter) injected into vacuum (~10<sup>-5</sup> torr). The cooling rate measured as a function of time in vacuum was fit to a model that accounts for temperature gradients between the surface and the core of the droplets, yielding an evaporation coefficient (&gamma;<sub>e</sub>) of 0.57&plusmn;0.06. This is nearly identical to that found for H<sub>2</sub>O (0.62&plusmn;0.09) using the same experimental method and model, and indicates the existence of a kinetic barrier to evaporation. The application of a recently developed transition-state theory (TST) model suggests that the kinetic barrier is due to librational and hindered translational motions at the liquid surface, and that the lack of an isotope effect is due to competing energetic and entropic factors. The implications of these results for cloud and aerosol particles in the atmosphere are discussed.
url http://www.atmos-chem-phys.net/8/6699/2008/acp-8-6699-2008.pdf
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