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New physics in sto d semileptonic transitions: rare hyperon vs. kaon decays

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arxiv 2112.11979 v2 pith:BBNALBJN submitted 2021-12-22 hep-ph hep-ex

New physics in sto d semileptonic transitions: rare hyperon vs. kaon decays

classification hep-ph hep-ex
keywords gammadecayskaonphysicshyperontheorycontextcontributions
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We investigate the potential of rare hyperon decays to probe the short distance structure in the $s\to d\nu\bar\nu$ and $s\to d\ell^+\ell^-$ transitions. Hyperon decays into neutrinos ($B_1\to B_2\nu\bar\nu$) can be reliably predicted by using form factors determined in baryon chiral perturbation theory. Their decay rates are sensitive to different short-distance operators, as compared to their kaon counterparts, and the corresponding branching fractions are in the range of $10^{-14}\sim10^{-13}$ in the standard model. In the context of the low-energy effective theory, we find that the anticipated BESIII measurements of the $B_1\to B_2\nu\bar\nu$ decays would lead to constraints on new physics in the purely axial vector $\bar d \gamma_\mu\gamma_5 s$ current that are stronger than the present limits from their kaon siblings $K\to \pi\pi\nu\bar\nu$. On the other hand, although hyperon decays into charged leptons are dominated by long-distance hadronic contributions, angular observable such as the leptonic forward-backward asymmetry is sensitive to the interference between long- and short-distance contributions. We discuss the sensitivity to new physics of a potential measurement of this observable in comparison with observables in the kaon decays $K_L\to\mu^+\mu^-$ and $K^+\to\pi^+\mu^+\mu^-$. We conclude that the current kaon bounds are a few orders of magnitude better than those that could be obtained from $\Sigma^+\to p\mu^+\mu^-$ except for two scenarios with new physics in the $(\bar d \gamma^\mu s)(\bar\ell\gamma_\mu\gamma_5\ell)$ and $(\bar d \gamma^\mu \gamma_5s)(\bar\ell\gamma_\mu\ell)$ currents. Finally, we point out that the loop effects from renormalization group evolution are important in this context, when relating the low-energy effective field theory to new physics models in the UV.

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