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DC Field | Value | Language |
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dc.contributor.author | Chhabra, S. | - |
dc.contributor.author | Kushwaha, A. | - |
dc.contributor.author | Kumar, T.J.D. | - |
dc.date.accessioned | 2018-12-28T04:46:08Z | - |
dc.date.available | 2018-12-28T04:46:08Z | - |
dc.date.issued | 2018-12-28 | - |
dc.identifier.uri | http://localhost:8080/xmlui/handle/123456789/1095 | - |
dc.description.abstract | Quantum dynamics of the molecule cyanogen (NCCN) and its collision with helium taking place in the interstellar medium has been studied. An ab initio potential energy surface of NCCN−−He, a van der Waals complex, is generated using the high-level single reference coupled-cluster with single and double and perturbative triple excitation method and aug-cc-pVQZ basis sets. Using the multipole expansion, Legendre coefficients have been calculated and utilized in determining collisional cross sections. Close-coupling calculations have been performed to study rotational excitations for He collision with NCCN. Due to nuclear spin statistics, collision induced transitions have even ∆j, while odd ∆j transitions are forbidden. The presence of resonances arising from rapid oscillation of cross sections in the low energy region is the result of quasi-bound states in the NCCN−−He van der Waals complex. Among all the transitions, ∆j = 2 are found to be predominant for excitation. Thereafter, for each transition, the rate coefficients have been calculated which decrease with increasing values of j and ∆j. The result of this work will be helpful to accurately model the abundance of cyanogen in stellar atmospheres and interstellar gas. Published by AIP Publishing. | en_US |
dc.language.iso | en_US | en_US |
dc.title | Quantum dynamics study of rotational transitions of NCCN induced by he collision | en_US |
dc.type | Article | en_US |
Appears in Collections: | Year-2018 |
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Full Text.pdf | 1.83 MB | Adobe PDF | View/Open Request a copy |
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