2004
DOI: 10.1016/j.jms.2004.08.015
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Nuclear spin selection rules in chemical reactions by angular momentum algebra

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Cited by 105 publications
(138 citation statements)
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References 16 publications
(27 reference statements)
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“…A careful theoretical study was necessary to explain all the results. Indeed, although the use of nuclear-spin selection rules (Oka 2004), leads to the reproduction of most of the observed OPR values below three at reasonable temperatures (Le Gal et al 2014a,b), it was necessary to identify a mechaArticle number, page 1 of 12 arXiv:1708.08980v2 [astro-ph.GA] 1 Oct 2017 A&A proofs: manuscript no. H2CL+_manuscript_accepted_2columns nism able to at least partially thermalize the OPR at the very low temperatures where the thermal OPR exceeds three and goes to infinity as the temperature goes to 0 K. This need led Persson et al (2016) to consider a process previously omitted in models: the poorly studied H + NH 2 H-atom exchange reaction to interconvert NH 2 between its ortho and para forms, thus increasing the OPR with decreasing temperature.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…A careful theoretical study was necessary to explain all the results. Indeed, although the use of nuclear-spin selection rules (Oka 2004), leads to the reproduction of most of the observed OPR values below three at reasonable temperatures (Le Gal et al 2014a,b), it was necessary to identify a mechaArticle number, page 1 of 12 arXiv:1708.08980v2 [astro-ph.GA] 1 Oct 2017 A&A proofs: manuscript no. H2CL+_manuscript_accepted_2columns nism able to at least partially thermalize the OPR at the very low temperatures where the thermal OPR exceeds three and goes to infinity as the temperature goes to 0 K. This need led Persson et al (2016) to consider a process previously omitted in models: the poorly studied H + NH 2 H-atom exchange reaction to interconvert NH 2 between its ortho and para forms, thus increasing the OPR with decreasing temperature.…”
Section: Introductionmentioning
confidence: 99%
“…Indeed, even an understanding of what appear to be thermal values under interstellar conditions can require a detailed analysis. Once well understood, OPRs can afford new powerful astrophysical diagnostics on the chemical and physical conditions of their environments, and in particular can trace their history, provided that the memory of a chemical process can be propagated and preserved in the molecular level population distributions (Oka 2004;Faure et al 2013;Le Gal et al 2014a). …”
Section: Introductionmentioning
confidence: 99%
“…This ranges from the astronomical importance of the ortho-para ratio [1][2][3][4][5] , to studies of nuclear-spin conversion [6,7] , selection rules and reactive collisions [8][9][10] or symmetry breaking [11] . Spin-enriched samples furthermore would allow for hypersensitized NMR experiments via polarization transfer reactions [12][13][14] .…”
mentioning
confidence: 99%
“…60 We will assume a general reaction H 3 + + X → HX + + H 2 whose mechanism is a direct proton hop (i.e., no complex is formed that can result in proton scrambling prior to dissociation). When the reaction involves o-H 3 + , application of Oka's angular momentum algebra 37 quickly shows that only o-H 2 can be formed as formation of p-H 2 would violate conservation of total nuclear spin angular momentum. Although the angular momentum algebra only gives proper branching ratios in the high-temperature limit, this selection rule for the chemical reaction also applies at the low temperatures relevant for cold interstellar clouds.…”
Section: Discussionmentioning
confidence: 99%
“…From a chemical physics standpoint, this reaction exhibits selection rules based on the symmetries of the reactants' rovibronic and nuclear spin state, 36 or alternatively, the selection rules can be derived in terms of nuclear spin angular momentum algebra. 37 Because of the weakness of the nuclear magnetic interaction, the two nuclear spin modifications (o-H 3 + , angular momentum I = (3/2), symmetry Γ ns = A 1 ; p-H 3 + , I = (1/2), Γ ns = E) can be regarded as separate chemical species; interconversion can only take place by means of reactive collisions or by interaction with a strong inhomogeneous magnetic field. As such, the H 3 + + H 2 → H 2 + H 3 + reaction has seen considerable theoretical treatment, especially in recent years, 38−41 and the effects of the nuclear spin selection rules have been experimentally studied by highresolution spectroscopy of H 3 + in hydrogenic plasmas.…”
Section: Introductionmentioning
confidence: 99%