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Oblique Corrections To The W Width

High Energy Physics - Phenomenology 2009-10-22 v1

Abstract

The lowest-order expression for the partial WW width to eν, Γ(Weν)=GμMW3/(6π2)e \nu ,~\Gamma (W \to e \nu) = G_\mu M_W^3 /(6 \pi \sqrt{2}), has no oblique radiative corrections from new physics if the measured WW mass is used. Here Gμ=(1.16639±0.00002)×105G_\mu = (1.16639 \pm 0.00002) \times 10^{-5} GeV/c2c^2 is the muon decay constant. For the present value of MW=(80.14±0.27)M_W = (80.14 \pm 0.27) GeV/c2c^2, and with mt=140m_t = 140 GeV/c2/c^2, one expects Γ(Weν)=(224.4±2.3)\Gamma (W \to e \nu) = (224.4 \pm 2.3) MeV. The total width Γtot(W)\Gamma_{\rm tot}(W) is also expected to lack oblique corrections from new physics, so that Γtot(W)/Γ(Weν)=3+6[1+{αs(MW)/π}]\Gamma_{\rm tot} (W)/ \Gamma (W \to e \nu) = 3 + 6 [1 + \{\alpha_s (M_W)/\pi \}]. Present data are consistent with this prediction.

Cite

@article{arxiv.hep-ph/9309307,
  title  = {Oblique Corrections To The W Width},
  author = {Jonathan L. Rosner and Mihir P. Worah and Tatsu Takeuchi},
  journal= {arXiv preprint arXiv:hep-ph/9309307},
  year   = {2009}
}

Comments

15 pages (LaTeX), one PostScript figure not included (available upon request)

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