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Constraints on the charged scalar effects using the forward-backward asymmetry on $B\to D^{(*)}\tau\bar{\nu_{\tau}}$

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arxiv 1205.4908 v3 pith:BA4OSN7M submitted 2012-05-22 hep-ph hep-ex

classification hep-phhep-ex
keywords effectschargedforward-backwardasymmetriesscalarasymmetrybranchingconstraints
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

The decay modes $\bar{B}\to D^{(*)}\tau\bar{\nu}_{\tau}$ are sensitive to charged scalar effects, such as the charged Higgs effects. In this paper we suggest a method to determine their effects by using the ratio of branching fractions and forward-backward asymmetries. In particular, forward-backward asymmetries on $\bar{B}\to D^{(*)}\tau(\to \pi\nu_{\tau})\bar{\nu}_{\tau}$, $\bar{B}\to D^{(*)}\tau(\to \rho\nu_{\tau})\bar{\nu}_{\tau}$, and $\bar{B}\to D^{(*)}\tau(\to a_1\nu_{\tau})\bar{\nu}_{\tau}$ play an important role, which discriminate the Standard Model from other New Physics scenarios.

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  1. The effects of polarization on the observables in the decay $\Xi_{cc}^{++} \rightarrow \Xi_{c}^{+} \bar{\ell}\nu_{\ell}$

    hep-ph 2026-03 accept novelty 5.5 of 10

    Polarization of the parent baryon, daughter baryon, and muon strongly reshapes branching ratios, forward-backward asymmetries, and newly defined polarization ratios in Ξ_cc++ → Ξ_c+ ℓ ν, while the μ/e LFU ratio stays ...

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