HD + ortho-/para-H2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K
State-resolved integral cross sections and corresponding thermal rate coefficients are computed for the HD + ortho-/para-H2 rotational energy transfer collision at low temperatures of astrophysical interest: 2 K ≲ T ≲ 300 K. A recent original full-dimensional H2-H2 potential energy surface (PES) was...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
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EDP Sciences
2016-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/201611302002 |
| Summary: | State-resolved integral cross sections and corresponding thermal rate coefficients are computed for the HD + ortho-/para-H2 rotational energy transfer collision at low temperatures of astrophysical interest: 2 K ≲ T ≲ 300 K. A recent original full-dimensional H2-H2 potential energy surface (PES) was adopted and appropriately modified for the current non-symmetrical four-atomic system. |
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| ISSN: | 2100-014X |