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Molecular collisions : State-of-the-art calculations of inelastic collisions

Published online by Cambridge University Press:  01 February 2008

Laurent Wiesenfeld
Affiliation:
Laboratoire d'Astrophysique de Grenoble, UMR CNRS 5571, Université Joseph-Fourier Grenoble, France email: laurent.wiesenfeld@obs.ujf-grenoble.fr
Alexandre Faure
Affiliation:
Laboratoire d'Astrophysique de Grenoble, UMR CNRS 5571, Université Joseph-Fourier Grenoble, France email: laurent.wiesenfeld@obs.ujf-grenoble.fr
Nicolas Troscompt
Affiliation:
Laboratoire d'Astrophysique de Grenoble, UMR CNRS 5571, Université Joseph-Fourier Grenoble, France email: laurent.wiesenfeld@obs.ujf-grenoble.fr
Michael Wernli
Affiliation:
Laboratoire d'Astrophysique de Grenoble, UMR CNRS 5571, Université Joseph-Fourier Grenoble, France email: laurent.wiesenfeld@obs.ujf-grenoble.fr Dipartimento di Chimica, La Sapienza, University of Rome, P. le A. Moro 5, Italy
Cecilia Ceccarelli
Affiliation:
Laboratoire d'Astrophysique de Grenoble, UMR CNRS 5571, Université Joseph-Fourier Grenoble, France email: laurent.wiesenfeld@obs.ujf-grenoble.fr
Pierre Valiron
Affiliation:
Laboratoire d'Astrophysique de Grenoble, UMR CNRS 5571, Université Joseph-Fourier Grenoble, France email: laurent.wiesenfeld@obs.ujf-grenoble.fr
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Abstract

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We set up a framework for calculating in a precise and controlled way the collisional properties of several molecules of astrophysical meaning. The quantities that are relevant for astrophysics are rotational and vibrational quenching/excitation rates by means of collisions of H2 with water and some organic molecules (HC3N, H2CO). We calculate those rates by means of successively determining a intermolecular potential energy surface and calculating inelastic cross sections and rates classically and/or quantum mechanically. These calculations are part of the European Union FP6 Molecular Universe program.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Dubernet, M.-L., et al. 2006, A&A, 460, 323Google Scholar
Faure, A., Crimier, N., Ceccarelli, C., Valiron, P., Wiesenfeld, L., & Dubernet, M. L. 2007, A&A, 472, 1029Google Scholar
Faure, A., Valiron, P., Wernli, M.Wiesenfeld, L., Rist, C., Noga, J., & Tennyson, J. 2005, J. Chem. Phys., 122, 221102CrossRefGoogle Scholar
Green, S. 1991, ApJS, 76, 979CrossRefGoogle Scholar
Troscompt, N., Faure, A., Wiesenfeld, L., Ceccarelli, C., & Valiron, P. 2008, A&A, submittedGoogle Scholar
Valiron, P., Wernli, M., Faure, A., Wiesenfeld, L., Rist, C., Kedžuch, S., & Noga, J. 2008, J. Chem. Phys., submittedGoogle Scholar
Wiesenfeld, L., Faure, A., Wernli, M., Valiron, P., Daniel, F., Dubernet, M. L., Grosjean, A., & Tennyson, J. 2006, AIP Conf. Proc. 855: Astrochemistry - From Laboratory Studies to Astronomical Observations, 855, 245CrossRefGoogle Scholar