Potential observation of the transitions at Belle II
arXiv:1804.01017 · doi:10.1103/PhysRevD.97.094018
Abstract
We perform the investigation of two-body hidden-bottom transitions of the , which include decays. For estimating the branching ratios of these processes, we consider contributions from the triangle hadronic loops composed of S-wave and mesons, which are a bridge to connect the and final states. Our results show that both of the branching ratios of these decays can reach . Due to such considerable potential to observe these two-body hidden-bottom transitions of the , we suggest the forthcoming Belle II experiment to explore them.
7 pages, 3 figures and 1 table
References in corpus (11)
- Observation of anomalous Upsilon(1S)pi+pi- and Upsilon(2S)pi+pi- production near the Upsilon(5S) resonance
- Scalar Resonance Contributions to the Dipion Transition Rates of in the re-scattering model
- Study on contributions of hadronic loops to decays of vector pseudoscalar mesons
- The puzzle of excessive non- component of the inclusive decay and the long-distant contribution
- Observation of and search for at GeV
- Peak shifts due to rescattering in dipion transitions
- transitions in the rescattering model and the new BaBar measurement
- Bottomonium dipion transitions
- Explaining the anomalous decays through the hadronic loop effect
- Prediction of anomalous transitions
- Exploring the and hidden-bottom hadronic transitions
Cited by in corpus (10)
- Spectroscopic survey of higher-lying states of meson family
- Predicted and decay modes of the charmoniumlike
- Proposal of searching for the hadronic decays into plus
- Hidden-bottom hadronic transitions of
- How higher charmonia shape the puzzling data of the cross section
- Production of charmonium plus one meson by annihilation
- Higher strangeonium decays into light flavor baryon pairs like , , and
- Charmonium decays into pair governed by the hadronic loop mechanism
- Non- Decays into Light Meson Pairs of the -Wave Charmonium
- Hidden-bottom hadronic decays of with a or emission