# Isospin breaking in the yield of heavy meson pairs in e+e- annihilation   near threshold

**Authors:** S. Dubynskiy, A. Le Yaouanc, L. Oliver, J.-C. Raynal, M.B. Voloshin

arXiv: 0704.0293 · 2008-11-26

## TL;DR

This paper investigates how strong and Coulomb interactions influence the ratio of charged to neutral heavy meson pairs produced near threshold energies in electron-positron annihilation, considering isospin effects and mass differences.

## Contribution

It introduces a realistic model incorporating resonant and nonresonant scattering in different isospin channels to analyze yield ratios near thresholds.

## Key findings

- Yield ratio depends smoothly on scattering phase in I=1 channel.
- Coulomb effects are sensitive to scattering phases in both isoscalar and isovector channels.
- Strong scattering modifies the pure kinematic effect of meson mass differences.

## Abstract

We revisit the problem of interplay between the strong and the Coulomb interaction in the charged-to-neutral yield ratio for $B {\bar B}$ and $D {\bar D}$ pairs near their respective thresholds in $e^+e^-$ annihilation. We consider here a realistic situation with a resonant interaction in the isospin I=0 channel and a nonresonant strong scattering amplitude in the I=1 state. We find that the yield ratio has a smooth behavior depending on the scattering phase in the I=1 channel. The same approach is also applicable to the $K {\bar K}$ production at the $\phi(1020)$ resonance, where the Coulomb effect in the charged-to-neutral yield ratio is generally sensitive to the scattering phases in both the isoscalar and the isovector channels. Furthermore, we apply the same approach to the treatment of the effect of the isotopic mass difference between the charged and neutral mesons and argue that the strong-scattering effects generally result in a modification to the pure kinematical effect of this mass difference.

## Full text

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## Figures

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## References

13 references — full list in the complete paper: https://tomesphere.com/paper/0704.0293/full.md

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Source: https://tomesphere.com/paper/0704.0293