On the validity of collider-mass scaling for molecular rotational excitation

Kyle M. Walker, B. H. Yang, P. C. Stancil, N. Balakrishnan, Robert C. Forrey

Research output: Contribution to journalArticle

20 Citations (Scopus)

Abstract

Rate coefficients for collisional processes such as rotational and vibrational excitation are essential inputs in many astrophysical models. When rate coefficients are unknown, they are often estimated using known values from other systems. The most common example is to use He-collider rate coefficients to estimate values for other colliders, typically H2, using scaling arguments based on the reduced mass of the collision system. This procedure is often justified by the assumption that the inelastic cross section is independent of the collider. Here we explore the validity of this approach focusing on rotational inelastic transitions for collisions of H, para-H 2, 3He, and 4He with CO in its vibrational ground state. We compare rate coefficients obtained via explicit calculations to those deduced by standard reduced-mass scaling. Not surprisingly, inelastic cross sections and rate coefficients are found to depend sensitively on both the reduced mass and the interaction potential energy surface. We demonstrate that standard reduced-mass scaling is not valid on physical and mathematical grounds, and as a consequence, the common approach of multiplying a rate coefficient for a molecule-He collision system by the constant factor of ∼1.4 to estimate the rate coefficient for para-H2 collisions is deemed unreliable. Furthermore, we test an alternative analytic scaling approach based on the strength of the interaction potential and the reduced mass of the collision systems. Any scaling approach, however, may be problematic when low-energy resonances are present; explicit calculations or measurements of rate coefficients are to be preferred.

Original languageEnglish (US)
Article number96
JournalAstrophysical Journal
Volume790
Issue number2
DOIs
StatePublished - Aug 1 2014

Fingerprint

scaling
coefficients
collision
excitation
collisions
cross section
rate
cross sections
estimates
potential energy
astrophysics
interactions
ground state
energy
molecules
calculation

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Walker, Kyle M. ; Yang, B. H. ; Stancil, P. C. ; Balakrishnan, N. ; Forrey, Robert C. / On the validity of collider-mass scaling for molecular rotational excitation. In: Astrophysical Journal. 2014 ; Vol. 790, No. 2.
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On the validity of collider-mass scaling for molecular rotational excitation. / Walker, Kyle M.; Yang, B. H.; Stancil, P. C.; Balakrishnan, N.; Forrey, Robert C.

In: Astrophysical Journal, Vol. 790, No. 2, 96, 01.08.2014.

Research output: Contribution to journalArticle

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