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Title: Rate constants for the formation of CS by radiative association

Abstract

Rate constants for the formation of carbon monosulfide (CS) by radiative association are calculated using accurate molecular data. The rate constants include both direct and indirect formation processes. The indirect processes (inverse rotational and electronic predissociation) are evaluated for conditions of local thermodynamic equilibrium (LTE) and also in the non-LTE limit of zero radiation temperature and atomic density. Phenomenological rate constants for CS formation in realistic astrophysical environments are expected to lie in-between these limiting cases. An analytic formula is used to fit the rate constants for convenient use in astrophysical models. The impact of the results on various astrophysical environments is briefly discussed.

Authors:
 [1]; ORCiD logo [2];  [3];  [4]
  1. Pennsylvania State Univ., Reading, PA (United States)
  2. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  3. Univ. of Georgia, Athens, GA (United States)
  4. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Queen's Univ., Belfast, Northern Ireland (United Kingdom)
Publication Date:
Research Org.:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Org.:
USDOE
OSTI Identifier:
1543963
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 479; Journal Issue: 4; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics

Citation Formats

Forrey, R. C., Babb, J. F., Stancil, P. C., and McLaughlin, B. M. Rate constants for the formation of CS by radiative association. United States: N. p., 2018. Web. doi:10.1093/mnras/sty1739.
Forrey, R. C., Babb, J. F., Stancil, P. C., & McLaughlin, B. M. Rate constants for the formation of CS by radiative association. United States. https://doi.org/10.1093/mnras/sty1739
Forrey, R. C., Babb, J. F., Stancil, P. C., and McLaughlin, B. M. Sat . "Rate constants for the formation of CS by radiative association". United States. https://doi.org/10.1093/mnras/sty1739. https://www.osti.gov/servlets/purl/1543963.
@article{osti_1543963,
title = {Rate constants for the formation of CS by radiative association},
author = {Forrey, R. C. and Babb, J. F. and Stancil, P. C. and McLaughlin, B. M.},
abstractNote = {Rate constants for the formation of carbon monosulfide (CS) by radiative association are calculated using accurate molecular data. The rate constants include both direct and indirect formation processes. The indirect processes (inverse rotational and electronic predissociation) are evaluated for conditions of local thermodynamic equilibrium (LTE) and also in the non-LTE limit of zero radiation temperature and atomic density. Phenomenological rate constants for CS formation in realistic astrophysical environments are expected to lie in-between these limiting cases. An analytic formula is used to fit the rate constants for convenient use in astrophysical models. The impact of the results on various astrophysical environments is briefly discussed.},
doi = {10.1093/mnras/sty1739},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 479,
place = {United States},
year = {Sat Jun 30 00:00:00 EDT 2018},
month = {Sat Jun 30 00:00:00 EDT 2018}
}

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Cited by: 11 works
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Works referencing / citing this record:

Semiclassical methods for calculating radiative association rate constants for different thermodynamic conditions: Application to formation of CO, CN, and SiN
journal, June 2019

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Rovibrational transition properties of the X 1 Σ + and A 1 Π states of carbon monosulfide
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Dicarbon Formation in Collisions of Two Carbon Atoms
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Dicarbon formation in collisions of two carbon atoms
text, January 2019