Calculation of scalar nuclear spin-spin coupling in a noble-gas mixture
Author(s): Vaara, Juha; Romalis, Michael V
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Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Vaara, Juha | - |
dc.contributor.author | Romalis, Michael V | - |
dc.date.accessioned | 2024-03-11T22:27:31Z | - |
dc.date.available | 2024-03-11T22:27:31Z | - |
dc.date.issued | 2019-06-12 | en_US |
dc.identifier.citation | Vaara, Juha, Romalis, Michael V. (Calculation of scalar nuclear spin-spin coupling in a noble-gas mixture. Physical Review A, 99 (6), 10.1103/physreva.99.060501 | en_US |
dc.identifier.issn | 2469-9926 | - |
dc.identifier.uri | http://arks.princeton.edu/ark:/88435/pr1nc5sc7r | - |
dc.description.abstract | Indirect spin-spin interactions between nuclei bound in a molecule are well known in nuclear magnetic resonance, but such interactions between unbound atoms are less well studied and are often assumed to be zero. We present a precision calculation of this interaction between 129Xe and 3He nuclei in a gas. Relativistic, state-of-the-art electronic structure theory is used to compute the scalar coupling constant J (R) and the interatomic potential energy function V (R) as functions of the Xe-He internuclear distance R. Using virial expansion we find the nuclear spin enhancement factor κ = −0.0105 ± 0.0015, in excellent agreement with recent experiments. This interaction is particularly important for precision measurements using nuclear spin comagnetometers. | en_US |
dc.language | en | en_US |
dc.language.iso | en_US | en_US |
dc.relation.ispartof | Physical Review A | en_US |
dc.rights | Author's manuscript | en_US |
dc.title | Calculation of scalar nuclear spin-spin coupling in a noble-gas mixture | en_US |
dc.type | Journal Article | en_US |
dc.identifier.doi | doi:10.1103/physreva.99.060501 | - |
dc.identifier.eissn | 2469-9934 | - |
pu.type.symplectic | http://www.symplectic.co.uk/publications/atom-terms/1.0/journal-article | en_US |
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1811.08678.pdf | 2.31 MB | Adobe PDF | View/Download |
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