Estimating the saturation vapor pressures of isoprene oxidation products C<sub>5</sub>H<sub>12</sub>O<sub>6</sub> and C<sub>5</sub>H<sub>10</sub>O<sub>6</sub> using COSMO-RS
<p>We have used COSMO-RS (the conductor-like screening model for real solvents), as implemented in the COSMOtherm program, to compute the saturation vapor pressures at 298 K of two photo-oxidation products of isoprene: the dihydroxy dihydroperoxide <span class="inline-formul...
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doaj-0f04188797a941eaaeeb0da74573faa22020-11-25T02:32:44ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242018-12-0118175891760010.5194/acp-18-17589-2018Estimating the saturation vapor pressures of isoprene oxidation products C<sub>5</sub>H<sub>12</sub>O<sub>6</sub> and C<sub>5</sub>H<sub>10</sub>O<sub>6</sub> using COSMO-RST. Kurtén0N. Hyttinen1E. L. D'Ambro2E. L. D'Ambro3J. Thornton4J. Thornton5N. L. Prisle6University of Helsinki, Department of Chemistry and Institute for Atmospheric and Earth System Research (INAR), P.O. Box 55, 00014 Helsinki, FinlandUniversity of Helsinki, Department of Chemistry and Institute for Atmospheric and Earth System Research (INAR), P.O. Box 55, 00014 Helsinki, FinlandDepartment of Chemistry, University of Washington, Seattle, Washington 98195, USADepartment of Atmospheric Sciences, University of Washington, Seattle, Washington 98195, USADepartment of Chemistry, University of Washington, Seattle, Washington 98195, USADepartment of Atmospheric Sciences, University of Washington, Seattle, Washington 98195, USAUniversity of Oulu, Nano and Molecular Systems Research Unit, P.O. Box 3000, 90014 Oulu, Finland<p>We have used COSMO-RS (the conductor-like screening model for real solvents), as implemented in the COSMOtherm program, to compute the saturation vapor pressures at 298 K of two photo-oxidation products of isoprene: the dihydroxy dihydroperoxide <span class="inline-formula">C<sub>5</sub>H<sub>12</sub>O<sub>6</sub></span>, and the dihydroperoxy hydroxy aldehyde, <span class="inline-formula">C<sub>5</sub>H<sub>10</sub>O<sub>6</sub></span>. The predicted saturation vapor pressures were significantly higher (by up to a factor of 1000) than recent experimental results, very likely due to the overestimation of the effects of intramolecular hydrogen bonds, which tend to increase saturation vapor pressures by stabilizing molecules in the gas phase relative to the liquid. Modifying the hydrogen bond enthalpy parameter used by COSMOtherm can improve the agreement with experimental results – however the optimal parameter value is likely to be system-specific. Alternatively, vapor pressure predictions can be substantially improved (to within a factor of 5 of the experimental values for the two systems studied here) by selecting only conformers with a minimum number of intramolecular hydrogen bonds. The computed saturation vapor pressures were very sensitive to the details of the conformational sampling approach, with the default scheme implemented in the COSMOconf program proving insufficient for the task, for example by predicting significant differences between enantiomers, which should have identical physical properties. Even after exhaustive conformational sampling, COSMOtherm predicts significant differences in saturation vapor pressures between both structural isomers and diastereomers. For <span class="inline-formula">C<sub>5</sub>H<sub>12</sub>O<sub>6</sub></span>, predicted differences in <span class="inline-formula"><i>p</i><sub>sat</sub></span> between structural isomers are up to 2 orders of magnitude, and differences between stereoisomers are up to a factor of 20 – though these differences are very likely exaggerated by the overestimation of the effect of intramolecular H-bonds. For <span class="inline-formula">C<sub>5</sub>H<sub>10</sub>O<sub>6</sub></span>, the maximum predicted differences between the three studied structural isomers and their diastereomer pairs are around a factor of 8 and a factor of 2, respectively, when only conformers lacking intramolecular hydrogen bonds are included in the calculations. In future studies of saturation vapor pressures of polyfunctional atmospheric oxidation products using COSMOtherm, we recommend first performing thorough conformational sampling and subsequently selecting conformers with a minimal number of intramolecular H-bonds.</p>https://www.atmos-chem-phys.net/18/17589/2018/acp-18-17589-2018.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
T. Kurtén N. Hyttinen E. L. D'Ambro E. L. D'Ambro J. Thornton J. Thornton N. L. Prisle |
spellingShingle |
T. Kurtén N. Hyttinen E. L. D'Ambro E. L. D'Ambro J. Thornton J. Thornton N. L. Prisle Estimating the saturation vapor pressures of isoprene oxidation products C<sub>5</sub>H<sub>12</sub>O<sub>6</sub> and C<sub>5</sub>H<sub>10</sub>O<sub>6</sub> using COSMO-RS Atmospheric Chemistry and Physics |
author_facet |
T. Kurtén N. Hyttinen E. L. D'Ambro E. L. D'Ambro J. Thornton J. Thornton N. L. Prisle |
author_sort |
T. Kurtén |
title |
Estimating the saturation vapor pressures of isoprene oxidation products C<sub>5</sub>H<sub>12</sub>O<sub>6</sub> and C<sub>5</sub>H<sub>10</sub>O<sub>6</sub> using COSMO-RS |
title_short |
Estimating the saturation vapor pressures of isoprene oxidation products C<sub>5</sub>H<sub>12</sub>O<sub>6</sub> and C<sub>5</sub>H<sub>10</sub>O<sub>6</sub> using COSMO-RS |
title_full |
Estimating the saturation vapor pressures of isoprene oxidation products C<sub>5</sub>H<sub>12</sub>O<sub>6</sub> and C<sub>5</sub>H<sub>10</sub>O<sub>6</sub> using COSMO-RS |
title_fullStr |
Estimating the saturation vapor pressures of isoprene oxidation products C<sub>5</sub>H<sub>12</sub>O<sub>6</sub> and C<sub>5</sub>H<sub>10</sub>O<sub>6</sub> using COSMO-RS |
title_full_unstemmed |
Estimating the saturation vapor pressures of isoprene oxidation products C<sub>5</sub>H<sub>12</sub>O<sub>6</sub> and C<sub>5</sub>H<sub>10</sub>O<sub>6</sub> using COSMO-RS |
title_sort |
estimating the saturation vapor pressures of isoprene oxidation products c<sub>5</sub>h<sub>12</sub>o<sub>6</sub> and c<sub>5</sub>h<sub>10</sub>o<sub>6</sub> using cosmo-rs |
publisher |
Copernicus Publications |
series |
Atmospheric Chemistry and Physics |
issn |
1680-7316 1680-7324 |
publishDate |
2018-12-01 |
description |
<p>We have used COSMO-RS (the conductor-like screening model for real solvents),
as implemented in the COSMOtherm program, to compute the saturation vapor
pressures at 298 K of two photo-oxidation products of isoprene: the dihydroxy
dihydroperoxide <span class="inline-formula">C<sub>5</sub>H<sub>12</sub>O<sub>6</sub></span>, and the dihydroperoxy hydroxy
aldehyde, <span class="inline-formula">C<sub>5</sub>H<sub>10</sub>O<sub>6</sub></span>. The predicted saturation vapor pressures
were significantly higher (by up to a factor of 1000) than recent
experimental results, very likely due to the overestimation of the effects of
intramolecular hydrogen bonds, which tend to increase saturation vapor
pressures by stabilizing molecules in the gas phase relative to the liquid.
Modifying the hydrogen bond enthalpy parameter used by COSMOtherm can improve
the agreement with experimental results – however the optimal parameter
value is likely to be system-specific. Alternatively, vapor pressure
predictions can be substantially improved (to within a factor of 5 of the
experimental values for the two systems studied here) by selecting only
conformers with a minimum number of intramolecular hydrogen bonds. The
computed saturation vapor pressures were very sensitive to the details of the
conformational sampling approach, with the default scheme implemented in the
COSMOconf program proving insufficient for the task, for example by
predicting significant differences between enantiomers, which should have
identical physical properties. Even after exhaustive conformational sampling,
COSMOtherm predicts significant differences in saturation vapor pressures
between both structural isomers and diastereomers. For
<span class="inline-formula">C<sub>5</sub>H<sub>12</sub>O<sub>6</sub></span>, predicted differences in <span class="inline-formula"><i>p</i><sub>sat</sub></span> between structural
isomers are up to 2 orders of magnitude, and differences between
stereoisomers are up to a factor of 20 – though these differences are very likely
exaggerated by the overestimation of the effect of intramolecular H-bonds.
For <span class="inline-formula">C<sub>5</sub>H<sub>10</sub>O<sub>6</sub></span>, the maximum predicted differences between the
three studied structural isomers and their diastereomer pairs are around a
factor of 8 and a factor of 2, respectively, when only conformers lacking
intramolecular hydrogen bonds are included in the calculations. In future
studies of saturation vapor pressures of polyfunctional atmospheric oxidation
products using COSMOtherm, we recommend first performing thorough
conformational sampling and subsequently selecting conformers with a minimal
number of intramolecular H-bonds.</p> |
url |
https://www.atmos-chem-phys.net/18/17589/2018/acp-18-17589-2018.pdf |
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