How to Measure the Mass of the W

dc.creatorAustern, Matthew H.
dc.creatorCahn, Robert N.
dc.date1993-04-29
dc.date.accessioned2026-07-07T03:56:02Z
dc.date.available2026-07-07T03:56:02Z
dc.descriptionWe perform a numerical calculation of the total cross section $σ(e^+e^- \rightarrow W^+W^-)$ as a function of energy, taking into account the finite width of the $W$ and the most important radiative corrections. We present these results, in tabular form, for several values of $M_W$. Using these results, we investigate running strategies for integrated luminosities that might be available at LEP~200 and estimate the accuracy to which it will be possible to determine the mass of the $W$ by measuring this cross section near threshold. With an integrated luminosity of $100\ {\rm pb}^{-1}$ it should be possible to achieve a precision of $100\ {\rm MeV}$, and with an integrated luminosity of $500\ {\rm pb}^{-1}$, a precision of $60\ {\rm MeV}$.
dc.description16 pages (8 figures, appended at end), LBL-33780
dc.identifierhttps://arxiv.org/abs/hep-ph/9304317
dc.identifierhttp://arxiv.org/abs/hep-ph/9304317
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44790
dc.subjectHigh Energy Physics - Phenomenology
dc.titleHow to Measure the Mass of the W
dc.typetext

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