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New Strategies for New Physics Search with $\Lambda_b \to \Lambda \nu \bar\nu$ Decays

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arxiv 2501.10652 v2 pith:BMUTYSNR submitted 2025-01-18 hep-ph

classification hep-ph
keywords lambdaphysicsasymmetrydecaysforward-backwardfuturetextuparrow
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We examine the new physics sensitivity of the rare decay $\Lambda_b \to \Lambda \nu\bar\nu$ which can be accessible at future $Z$-pole machines like FCC-ee and CEPC. We find that the longitudinal polarization of $\Lambda_b$ baryons produced in $Z$ decays introduces a novel observable, the forward-backward asymmetry $A_\text{FB}^\uparrow$ in the angle between the outgoing $\Lambda$ momentum and the $\Lambda_b$ spin. We provide Standard Model predictions for the $\Lambda_b \to \Lambda \nu\bar\nu$ branching ratio and $A_\text{FB}^\uparrow$, and show that future precision measurements of these observables are complementary and probe new physics scales comparable to other $b \to s \nu\bar\nu$ and $b \to s \ell^+ \ell^-$ processes. We also show that the zero crossing of the forward-backward asymmetry offers a robust test of form factor calculations independent of new physics.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A Unified Dark Matter Explanation for $\boldsymbol{B^+ \!\to K^+\nu\bar{\nu}}$ and the Super-Kamiokande Antineutrino Excess

    hep-ph 2026-07 conditional novelty 5.0 of 10

    A UV-complete complex scalar DM model under gauged U(1)Lμ−Lτ accommodates the SK antineutrino excess, the Belle II B+→K+νν̄ excess, and the DM relic density with one light dark sector.

  2. $\Lambda_b \to \Lambda^{(\ast)}\nu\bar{\nu}$ decays and the recent Belle-II $B^+\to K^+\nu\bar{\nu}$ data

    hep-ph 2025-07 conditional novelty 5.0 of 10

    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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