Theoretical study of the electronically excited radical cations of naphthalene and anthracene as archetypal models for astrophysical observations. Part II. Dynamics consequences

dc.contributor.author Ghanta, S.
dc.contributor.author Sivaranjana Reddy, V.
dc.contributor.author Mahapatra, S.
dc.date.accessioned 2022-03-27T00:15:44Z
dc.date.available 2022-03-27T00:15:44Z
dc.date.issued 2011-08-28
dc.description.abstract Nuclear dynamics is investigated theoretically from first principles by employing the ab initio vibronic models of the prototypical naphthalene and anthracene radical cations developed in Part I. This Part is primarily aimed at corroborating a large amount of available experimental data with a specific final goal to establish an unambiguous link with the current observations in astrophysics and astronomy. The detailed analyses presented here perhaps establish that these two prototypical polycyclic aromatic hydrocarbon radical cations are indeed potential carriers of the observed diffuse interstellar bands. © the Owner Societies 2011.
dc.identifier.citation Physical Chemistry Chemical Physics. v.13(32)
dc.identifier.issn 14639076
dc.identifier.uri 10.1039/c1cp21084j
dc.identifier.uri http://xlink.rsc.org/?DOI=c1cp21084j
dc.identifier.uri https://dspace.uohyd.ac.in/handle/1/2961
dc.title Theoretical study of the electronically excited radical cations of naphthalene and anthracene as archetypal models for astrophysical observations. Part II. Dynamics consequences
dc.type Journal. Article
dspace.entity.type
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