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A theoretical study of the conversion of gas phase methanediol to formaldehyde

Kent, David R., IV and Widicus, Susanna L. and Blake, Geoffrey A. (2003) A theoretical study of the conversion of gas phase methanediol to formaldehyde. Journal of Chemical Physics, 119 (10). Art. No. 5117. ISSN 0021-9606. http://resolver.caltech.edu/CaltechAUTHORS:20120919-115917235

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Abstract

Methanediol, or methylene glycol, is a product of the liquid phase reaction of water and formaldehyde and is a predicted interstellar grain surface species. Detection of this molecule in a hot core environment would advance the understanding of complex organic chemistry in the interstellar medium, but its laboratory spectroscopic characterization is a prerequisite for such observational searches. This theoretical study investigates the unimolecular decomposition of methanediol, specifically the thermodynamic and kinetic stability of the molecule under typical laboratory and interstellar conditions. Methanediol was found to be thermodynamically stable at temperatures of <100 K, which is the characteristic temperature range for interstellar grain mantles. The infinite-pressure RRKM unimolecular decomposition rate was found to be <10^(−18) s^(−1) at 300 K, indicating gas phase kinetic stability for typical laboratory and hot core temperatures. Therefore, both laboratory studies of and observational searches for this molecule should be feasible.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1063/1.1596392DOIUNSPECIFIED
http://link.aip.org/link/doi/10.1063/1.1596392PublisherUNSPECIFIED
Additional Information:© 2003 American Institute of Physics. Received 28 February 2003; accepted 9 June 2003. D.R.K. is grateful for a graduate fellowship from The Fannie and John Hertz Foundation. S.L.W. and G.A.B. thank the NASA Exobiology and SARA programs, Grant Nos. NAG5-8822 and NAG5-11423. We gratefully acknowledge the support and services rendered by the CIT staff. The computational resources at the MSC were provided by the NSF (CHE-99MRI), IBM (SUR Grant), ARO-DURIP, and ONRDURIP. Other support for the MSC came from NIH, Chevron Texaco, GM, Seiko-Epson, Beckman Institute, Asahi Kasei, Nippon Steel, and DOE ASCI ASAP.
Funders:
Funding AgencyGrant Number
Fannie and John Hertz FoundationUNSPECIFIED
NASA Exobiology programNAG5-8822
NASA SARA ProgramNAG5-11423
NSFCHE-99MRI
IBM SUR grantUNSPECIFIED
ARO-DURIPUNSPECIFIED
ONR-DURIPUNSPECIFIED
NIHUNSPECIFIED
Chevron TexacoUNSPECIFIED
GMUNSPECIFIED
Seiko-EpsonUNSPECIFIED
Caltech Beckman Institute UNSPECIFIED
Asahi KaseiUNSPECIFIED
Nippon SteelUNSPECIFIED
DOE ASCI ASAPUNSPECIFIED
Subject Keywords:organic compounds; interstellar molecules; dissociation
Classification Code:PACS: 82.30.Lp; 98.38.Bn
Record Number:CaltechAUTHORS:20120919-115917235
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20120919-115917235
Official Citation:A theoretical study of the conversion of gas phase methanediol to formaldehyde David R. Kent IV, Susanna L. Widicus, Geoffrey A. Blake, and William A. Goddard III, J. Chem. Phys. 119, 5117 (2003), DOI:10.1063/1.1596392
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34216
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:19 Sep 2012 19:36
Last Modified:26 Dec 2012 16:13

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