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Full-dimensional quantum dynamics of water in collisions with H

POSTER

Abstract

Modeling of molecular emission spectra from the interstellar medium requires the

calculation of rate coefficients for excitation by collisions with abundant species.

Water is an abundant molecule in a variety of astrophysical environments,

and has been the focus of countless theoretical astrophysical studies and observations.

In this work we report full-dimensional state-to-state and total quenching cross sections

and rate coefficients from some selected rotational J Ka,Kc states in vibrational states of

(v1,v2,v3)=(010) and (100) for both para- and ortho-H2O in collisions with H,

v1, v2, v3 are quantum numbers for the fundamental vibrational modes of water.

The high level ab initio potential energy surface (PES)

used in the scattering calculations were fitted using a two-component invariant polynomial method.

Our total vibrational quenching cross sections

are also compared with the results of Cabrera-Gonzalez et al., which were calculated on

a 4D PES with the Rigid-bender close-coupling method.

Presenters

  • Benhui Yang

    University of Georgia

Authors

  • Benhui Yang

    University of Georgia

  • Chen Qu

    Emory Univeristy

  • Phillip Stancil

    University of Georgia

  • Joel Bowman

    Emory University

  • Dongzheng Yang

    University of New Mexico

  • Hua Guo

    University of New Mexico

  • Robert Forrey

    Penn State University, Berks Campus, Penn State Berks

  • Balakrishnan Naduvalath

    University of Nevada, Las Vegas, University of Nevada - Las Vegas