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WorksPhysics and Astronomy

First search for sidereal and annual modulation of ZZ-pole asymmetries with the recovered SLD data set

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arXiv nonexclusive license
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Published
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Abstract · v1

We report what is, to our knowledge, the first time-resolved analysis of electroweak asymmetries at the ZZ pole, using the public release of the recovered SLD collision data: 6.6×1056.6\times10^5 polarized e+e−→Ze^+e^-\to Z events from the 1996-1998 SLC runs, with 385583 selected hadronic ZZ decays spanning 782 sidereal cycles. The left-right asymmetry ALRA_{LR}, reconstructed with the published SLD selection and per-event signed Compton polarization, shows no sidereal, solar-diurnal, or annual modulation; a simultaneous unbinned likelihood fit bounds the sidereal first-harmonic amplitude at 0.0086 (95% C.L., statistical). The analysis, frozen on the initial partial release, applied unchanged to the 229833 events of the later-released 1998 run confirms the null (amplitude 0.0018, p=0.90). Using the as-built SLC beam azimuth from the release's documentation corpus, we bound the asymmetry's anisotropy tensor in the Sun-centered frame: ρ1≤0.060ρ_1\le0.060, ρ2≤0.18ρ_2\le0.18, and, for vector backgrounds, ρ0≤0.092ρ_0\le0.092 (95% C.L.). A leading-order matching maps these onto minimal Standard-Model-Extension coefficients as 10−210^{-2}-level sensitivities to the two-time-index block of the electroweak gauge-sector coefficient kWk_W (components with no existing laboratory constraint) and to the Higgs-sector coefficient kϕϕk_{ϕϕ}; the insertions split the ZZ pole by polarization, so for the tensor families assessed the resonance saturates the sidereal amplitude near 10−210^{-2} and the Born-model bounds exclude finite coefficient bands rather than set an upper limit. We also derive a previously unpublished ZZ-pole birefringence channel in the helicity-odd azimuthal modulation of the thrust axis, with response enhanced by about 2MZ/ΓZ2M_Z/Γ_Z; a Born-level pilot is null. First sidereal analyses of hadronization and leptonic asymmetries bound instrumental drifts at the 10−410^{-4}-10−310^{-3} fractional level.

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