HD +ortho-/para-H2rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K

Renat A. Sultanov, Dennis Guster, C. Elster, D.R. Phillips, C.D. Roberts
2016 EPJ Web of Conferences  
State-resolved integral cross sections and corresponding thermal rate coefficients are computed for the HD + ortho-/para-H 2 rotational energy transfer collision at low temperatures of astrophysical interest: 2 K T 300 K. A recent original fulldimensional H 2 -H 2 potential energy surface (PES) was adopted and appropriately modified for the current non-symmetrical four-atomic system.
doi:10.1051/epjconf/201611302002 fatcat:zacovs2llrgopovrlxali4djxm