A computational study of hydrogen dimers in giant-planet infrared spectra
Document identifier: oai:DiVA.org:ltu-76702
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10.1088/1742-6596/1289/1/012010Keyword: Natural Sciences,
Physical Sciences,
Other Physics Topics,
Naturvetenskap,
Fysik,
Annan fysik,
Applied Physics,
Tillämpad fysikPublication year: 2019Relevant Sustainable Development Goals (SDGs):
The SDG label(s) above have been assigned by OSDG.aiAbstract: The absorption due to H2–H2 complexes is investigated theoretically. The potential and dipole surfaces for the complex are taken from the literature. Quantum dynamical calculations of the roto-translational absorption spectrum are performed. Special attention is paid to the fine features due to hydrogen dimers, (H2)2, at the centers of the collision-induced rotational S(0) and S(1) transitions. The computed absorption coefficients are used to analyze the spectra of the four giant planets of our solar system.
Authors
Magnus Gustafsson
Luleå tekniska universitet; Materialvetenskap
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Fletcher Leigh
Department of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK
Other publications
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Glenn Orton
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
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header:
identifier: oai:DiVA.org:ltu-76702
datestamp: 2021-04-19T12:54:10Z
setSpec: SwePub-ltu
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recordCreationDate: 2019-11-14
identifier:
http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-76702
10.1088/1742-6596/1289/1/012010
2-s2.0-85073531216
titleInfo:
@attributes:
lang: eng
title: A computational study of hydrogen dimers in giant-planet infrared spectra
abstract: The absorption due to H2–H2 complexes is investigated theoretically. The potential and dipole surfaces for the complex are taken from the literature. Quantum dynamical calculations of the roto-translational absorption spectrum are performed. Special attention is paid to the fine features due to hydrogen dimers (H2)2 at the centers of the collision-induced rotational S(0) and S(1) transitions. The computed absorption coefficients are used to analyze the spectra of the four giant planets of our solar system.
subject:
@attributes:
lang: eng
authority: uka.se
topic:
Natural Sciences
Physical Sciences
Other Physics Topics
@attributes:
lang: swe
authority: uka.se
topic:
Naturvetenskap
Fysik
Annan fysik
@attributes:
lang: eng
authority: ltu
topic: Applied Physics
genre: Research subject
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lang: swe
authority: ltu
topic: Tillämpad fysik
genre: Research subject
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Published
3
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Gustafsson
Magnus
1969-
role:
roleTerm: aut
affiliation:
Luleå tekniska universitet
Materialvetenskap
nameIdentifier:
maggus
0000-0002-7629-0169
@attributes:
type: personal
namePart:
Leigh
Fletcher
role:
roleTerm: aut
affiliation: Department of Physics and Astronomy University of Leicester University Road Leicester LE1 7RH UK
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type: personal
namePart:
Orton
Glenn
role:
roleTerm: aut
affiliation: Jet Propulsion Laboratory California Institute of Technology 4800 Oak Grove Drive Pasadena CA 91109 USA
originInfo:
dateIssued: 2019
publisher: Institute of Physics (IOP)
relatedItem:
@attributes:
type: host
titleInfo:
title: 24th International Conference on Spectral Lines Shapes 17-22 June 2018 Dublin Ireland
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type: series
titleInfo:
title: Journal of Physics: Conference Series
partNumber: 1289
identifier:
1742-6588
1742-6596
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form: print
typeOfResource: text