Calculation of the ratios and absolute rates of the $\Xi_b^- \to \pi^- (D_s^- ) \ \Xi_c^0 (2790) \left(\Xi_c^0 (2815) \right)$ and $\Xi_b^- \to \bar{\nu}_l l \ \Xi_c^0 (2790) \left(\Xi_c^0 (2815) \right)$ decays
R. Pavao, W-H Liang, J. Nieves, E. Oset

TL;DR
This paper calculates decay rate ratios of $ ext{Xi}_b$ baryons into $ ext{Xi}_c$ resonances using a chiral meson-baryon interaction model, providing predictions consistent across relativistic and nonrelativistic approaches.
Contribution
It introduces a method to compute decay rate ratios involving $ ext{Xi}_b$ and $ ext{Xi}_c$ resonances using a dynamically generated resonance model with chiral WT interactions, including relativistic and nonrelativistic calculations.
Findings
Ratios of decay rates are similar (~1% difference) in both relativistic and nonrelativistic calculations.
Calculated decay rate ratios agree with experimental data when normalized to related $ ext{Lambda}_b$ decays.
The approach effectively predicts decay ratios involving dynamically generated $ ext{Xi}_c$ resonances.
Abstract
In this work we calculate the ratios of rates of the nonleptonic and semileptonic decays into the (2790) and (2815) () resonances. These resonances are dynamically generated from the pseudoscalar-baryon and vector-baryon interactions, whose mixing is done using the chiral Weinberg-Tomozawa (WT) meson-baryon interaction extended to four flavors. The first part of the decay is a weak decay that we analyze through their quark constituents where it is noted that only the heavy quarks ( and ) participate in the interaction, leaving the light pair () as spectators. This first decay then produces a meson-baryon pair that creates the through the WT interaction. We then proceed to calculate the decay rates to (2790) and (2815) for both the nonleptonic and semileptonic cases and then calculate the ratios between them. We do this…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Quantum Chromodynamics and Particle Interactions · Black Holes and Theoretical Physics
