# Decay ${\mathit{D} \to} {{\mathit K}^{(*)}}{{\mathit \ell}^{+}}{{\mathit   \nu}_{{{{\mathit \ell}}}}}$ in covariant quark model

**Authors:** N. R. Soni, J. N. Pandya

arXiv: 1706.01190 · 2017-08-02

## TL;DR

This paper calculates form factors and decay rates for D-meson leptonic and semileptonic decays using a covariant quark model with infrared confinement, providing results consistent with isospin symmetry and experiments.

## Contribution

It introduces a covariant quark model with infrared confinement to compute form factors across the full kinematic range for D-meson decays, enhancing theoretical predictions.

## Key findings

- Form factors computed across entire kinematic range.
- Branching ratios consistent with experimental data.
- Ratios of partial widths close to isospin invariance expectations.

## Abstract

We study the leptonic and semileptonic $D$-meson decays (${{\mathit D} \to} {{\mathit \ell}^{+}}{{\mathit \nu}_{{{{\mathit \ell}}}}}$ and ${\mathit{D} \to} {{\mathit K}^{(*)}}{{\mathit \ell}^{+}}{{\mathit \nu}_{{{{\mathit \ell}}}}}$) in the framework of covariant quark model with built-in infrared confinement. We compute the required form factors in the entire kinematical momentum transfer region. The calculated form factors are used to evaluate the branching fractions of these transitions. We determine the following ratios of the partial widths: $\Gamma ({{\mathit D}^{0}} \rightarrow {{\mathit K}^{-}}{{\mathit e}^{+}}{{\mathit \nu}_{{e}}})/\Gamma({{\mathit D}^{+}} \rightarrow {{\overline{\mathit K}}^{0}}{{\mathit e}^{+}}{{\mathit \nu}_{{e}}}) = 1.02$, $\Gamma({{\mathit D}^{0}} \rightarrow {{\mathit K}^{-}}{{\mathit \mu}^{+}}{{\mathit \nu}_{{\mu}}})/\Gamma({{\mathit D}^{+}} \rightarrow {{\overline{\mathit K}}^{0}}{{\mathit \mu}^{+}}{{\mathit \nu}_{{\mu}}}) = 0.99$ and $\Gamma({{\mathit D}^{+}} \rightarrow {{\overline{\mathit K}}^{0}}{{\mathit \mu}^{+}}{{\mathit \nu}_{{\mu}}}) / \Gamma({{\mathit D}^{+}} \rightarrow {{\overline{\mathit K}}^{0}}{{\mathit e}^{+}}{{\mathit \nu}_{{e}}}) = 0.97$ which are in close resemblance with the iso-spin invariance and experimental results.

## Full text

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## Figures

21 figures with captions in the complete paper: https://tomesphere.com/paper/1706.01190/full.md

## References

73 references — full list in the complete paper: https://tomesphere.com/paper/1706.01190/full.md

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Source: https://tomesphere.com/paper/1706.01190