Abstract
Using the most general form of baryonic interpolating current, the masses and pole residues of the excited 2S and 1P states of the triply-heavy baryons $$\Omega _{\mathrm{{bbc}}}$$ and $$\Omega _{\mathrm{{ccb}}}$$ are calculated within the QCD sum rule approach. The obtained results are compared with the existing theoretical predictions in the literature.
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.