Literature DB >> 19586103

A five-dimensional potential-energy surface for the rotational excitation of SO2 by H2 at low temperatures.

A Spielfiedel1, M-L Senent, F Dayou, C Balança, L Cressiot-Vincent, A Faure, L Wiesenfeld, N Feautrier.   

Abstract

The SO(2) molecule is detected in a large variety of astronomical objects, notably molecular clouds and star-forming regions. An accurate modeling of the observations needs a very good knowledge of the collisional excitation rates with H(2) because of competition between collisional and radiative processes that excite and quench the different rotational levels of SO(2). We report here a five-dimensional, rigid-body, interaction potential for SO(2)-H(2). As a first application, we present rate constants for excitation/de-excitation of the 31 first levels of SO(2) by para-H(2) at low temperatures. Propensity rules are discussed.

Entities:  

Year:  2009        PMID: 19586103     DOI: 10.1063/1.3158357

Source DB:  PubMed          Journal:  J Chem Phys        ISSN: 0021-9606            Impact factor:   3.488


  1 in total

1.  The millimeter IRAM-30 m line survey toward IK Tau.

Authors:  L Velilla Prieto; C Sánchez Contreras; J Cernicharo; M Agúndez; G Quintana-Lacaci; V Bujarrabal; J Alcolea; C Balança; F Herpin; K M Menten; F Wyrowski
Journal:  Astron Astrophys       Date:  2016-12-19       Impact factor: 5.802

  1 in total

北京卡尤迪生物科技股份有限公司 © 2022-2023.