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$R^\nu_{K^{(*)}}$ and non-standard neutrino interactions
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abstract
We discuss the modes $B\to K^{(*)}\nu\bar\nu$ in the context of non-standard neutrino interactions that add incoherently to the SM rates. We consider two scenarios: an additional light neutrino; and neutrino lepton flavour violation. We find that an additional light neutrino that interacts with SM fields via a non-universal $Z^\prime$ can increase $R^\nu_{K^{(*)}}$ by up to a factor of two without conflicting with $B_s-\bar B_s$ mixing. This model then predicts rates for $B_s\to \tau^+\tau^-$ up to six times larger than the SM. In the context of neutrino lepton flavour violation mediated by leptoquarks we find that the current experimental upper bounds on $R^\nu_{K^{(*)}}$ are already more constraining than direct bounds from $B_s\to \tau \ell$ and $B\to K^{(*)}\tau \ell$ modes for $\ell=e,\mu$.
Forward citations
Cited by 2 Pith papers
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Radiative generation of chiral vector operators in $b\to s \nu\bar{\nu}$ transition
Minimal one-loop models that generate both chiral vector operators for b→sνν̄ are systematically classified but cannot quantitatively explain the Belle II anomaly.
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$\Lambda_b \to \Lambda^{(\ast)}\nu\bar{\nu}$ decays and the recent Belle-II $B^+\to K^+\nu\bar{\nu}$ data
Belle-II's B+ -> K+ nu nubar excess, if due to new physics, constrains the branching ratios and angular observables of Lambda_b -> Lambda(*) nu nubar decays, with the hadronic forward-backward asymmetry the best discr...
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