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NLO prediction for the decays $\tau \to \ell \ell'\ell' \nu \bar \nu$ and $\mu \to e e e \nu \bar\nu$
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These proceedings review the differential decay rates and the
branching ratios of the tau and muon decays
\tau \to \ell \ell' \ell' \nu \bar\nuτ→ℓℓ′ℓ′νν‾
(with \ell,\ell'=\mu,eℓ,ℓ′=μ,e)
and \mu \to e e e \nu \bar \nuμ→eeeνν‾
in the Standard Model at NLO. These five-body leptonic decays are a tool
to study the Lorentz structure of weak interactions and to test lepton
flavour universality. They are also a source of SM background to
searches for the lepton-flavour-violating decays
\mu \to e e eμ→eee
and \tau \to \ell \ell' \ell'τ→ℓℓ′ℓ′.Even if the shift in the branching ratios induced by radiative
corrections turns out to be small and of order 1% — mainly due to a
running effect of the fine structure constant — locally in the phase
space these corrections can reach the 5 - 10% level, depending on the
applied cuts. We found for instance that in the phase space region where
the neutrino energies are small, and the momenta of the three charged
leptons have a similar signature as in \mu \to eeeμ→eee
and \tau \to \ell \ell'\ell'τ→ℓℓ′ℓ′,
the NLO corrections decrease the leading-order prediction by about 10 -
20%.
Title: NLO prediction for the decays $\tau \to \ell \ell'\ell' \nu \bar \nu$ and $\mu \to e e e \nu \bar\nu$
Description:
These proceedings review the differential decay rates and the
branching ratios of the tau and muon decays
\tau \to \ell \ell' \ell' \nu \bar\nuτ→ℓℓ′ℓ′νν‾
(with \ell,\ell'=\mu,eℓ,ℓ′=μ,e)
and \mu \to e e e \nu \bar \nuμ→eeeνν‾
in the Standard Model at NLO.
These five-body leptonic decays are a tool
to study the Lorentz structure of weak interactions and to test lepton
flavour universality.
They are also a source of SM background to
searches for the lepton-flavour-violating decays
\mu \to e e eμ→eee
and \tau \to \ell \ell' \ell'τ→ℓℓ′ℓ′.
Even if the shift in the branching ratios induced by radiative
corrections turns out to be small and of order 1% — mainly due to a
running effect of the fine structure constant — locally in the phase
space these corrections can reach the 5 - 10% level, depending on the
applied cuts.
We found for instance that in the phase space region where
the neutrino energies are small, and the momenta of the three charged
leptons have a similar signature as in \mu \to eeeμ→eee
and \tau \to \ell \ell'\ell'τ→ℓℓ′ℓ′,
the NLO corrections decrease the leading-order prediction by about 10 -
20%.
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