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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Main Authors: Sultanov Renat A., Guster Dennis
Format: Article
Language:English
Published: EDP Sciences 2016-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201611302002
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spelling 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
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