On the Validity of Collider-Mass Scaling for Molecular Rotational Excitation
Kyle M. Walker, B. H. Yang, P. C. Stancil, N. Balakrishnan, R. C., Forrey

TL;DR
This paper critically examines the common practice of using reduced-mass scaling to estimate molecular rotational excitation rates, demonstrating its limitations and proposing the need for explicit calculations or measurements for accuracy.
Contribution
The study shows that standard reduced-mass scaling is invalid for estimating collisional rate coefficients, advocating for explicit calculations or alternative scaling methods.
Findings
Reduced-mass scaling is unreliable for collisional rate estimates.
Explicit calculations are preferred over scaling methods.
Interaction potential strength influences inelastic cross sections.
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 H, 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, He, and He 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…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
