Abstract

It is shown that, in the bound state picture, the ${\ensuremath{\Lambda}}_{c}(2593)\ensuremath{\rightarrow}{\ensuremath{\Lambda}}_{c}\ensuremath{\gamma}$ and ${\ensuremath{\Lambda}}_{c}(2625)\ensuremath{\rightarrow}{\ensuremath{\Lambda}}_{c}\ensuremath{\gamma}$ decays are severely suppressed. On the other hand, for their bottom counterparts, which are predicted to have masses of 5900 and 5926 MeV, respectively, they may have significant radiative branching ratios. The ${\ensuremath{\Lambda}}_{b}(5926)\ensuremath{\rightarrow}{\ensuremath{\Lambda}}_{b}\ensuremath{\gamma}$ mode possibly dominates over the strong decay mode, while the ${\ensuremath{\Lambda}}_{b}(5900)$ resonance lies below the strong decay threshold and can only decay radiatively. The isospin allowed ${\ensuremath{\Lambda}}_{Q}^{**}\ensuremath{\rightarrow}{\ensuremath{\Sigma}}_{Q}\ensuremath{\gamma}$ mode is expected to be small.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

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.