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dc.contributor.authorChhabra, S.-
dc.contributor.authorKushwaha, A.-
dc.contributor.authorKumar, T.J.D.-
dc.date.accessioned2018-12-28T04:46:08Z-
dc.date.available2018-12-28T04:46:08Z-
dc.date.issued2018-12-28-
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/1095-
dc.description.abstractQuantum 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.isoen_USen_US
dc.titleQuantum dynamics study of rotational transitions of NCCN induced by he collisionen_US
dc.typeArticleen_US
Appears in Collections:Year-2018

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