Abstract
The variation of electronic transition moment with internuclear distance in the case of (A 2 Π -X 2 Σ +) and and (B 2 Σ + -X 2 Σ +) transitions of astrophysically significant BO molecule been reinvestigated. On the basis of the results it is concluded that the conventional Morse potential is not appropriate to yield meaningful information about the electronic transition moments. The preferential superiority of the RKRV potential over Morse potential in such studies has been critically discussed.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.