Machine learning prediction of state-to-state rate constants for astrochemistry

Author:

Bossion DuncanORCID,Nyman Gunnar,Scribano Yohann

Funder

Knut and Alice Wallenberg Foundation

Publisher

Elsevier BV

Reference37 articles.

1. Vibrational level population of H2 and H2+ in the early universe;Coppola;Astrophys. J. Suppl. Ser.,2011

2. Temperature and density dependent cooling function for H2 with updated H2/H collisional rates;Coppola;Mon. Not. R. Astron. Soc.,2019

3. Collisional excitation of H2 molecules by H atoms;Mandy;Astrophys. J. Suppl. Ser.,1993

4. Ortho?para-H2 conversion processes in astrophysical media;Lique;Int. Rev. Phys. Chem.,2014

5. Revisited study of the ro-vibrational excitation of H2 by H: towards a revision of the cooling of astrophysical media;Lique;Mon. Not. R. Astron. Soc.,2015

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