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...
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2016-01-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/201611302002 |
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doaj-dc2d3f2b42774fb58f4bf0ad274b2e552021-08-02T03:11:23ZengEDP SciencesEPJ Web of Conferences2100-014X2016-01-011130200210.1051/epjconf/201611302002epjconf_fb2016_02002HD + ortho-/para-H2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 KSultanov Renat A.0Guster Dennis1Department of Information Systems, BCRL & Integrated Science and Engineering Laboratory Facility (ISELF) at St. Cloud State UniversityDepartment of Information Systems, BCRL & Integrated Science and Engineering Laboratory Facility (ISELF) at St. Cloud State UniversityState-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.http://dx.doi.org/10.1051/epjconf/201611302002 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Sultanov Renat A. Guster Dennis |
spellingShingle |
Sultanov Renat A. Guster Dennis HD + ortho-/para-H2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K EPJ Web of Conferences |
author_facet |
Sultanov Renat A. Guster Dennis |
author_sort |
Sultanov Renat A. |
title |
HD + ortho-/para-H2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K |
title_short |
HD + ortho-/para-H2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K |
title_full |
HD + ortho-/para-H2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K |
title_fullStr |
HD + ortho-/para-H2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K |
title_full_unstemmed |
HD + ortho-/para-H2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 K ≲ T ≲ 300 K |
title_sort |
hd + ortho-/para-h2 rotational energy transfer non-reactive scattering at low astrophysical temperatures: 2 k ≲ t ≲ 300 k |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2016-01-01 |
description |
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. |
url |
http://dx.doi.org/10.1051/epjconf/201611302002 |
work_keys_str_mv |
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1721243499571970048 |