Date: Wed, 5 Dec 2001 10:16:30 +0900 (JST) From: seki@neutrino.kek.jp To: Hiroshi Toki <toki@rcnp.osaka-u.ac.jp>, Kuniharu Kubodera <kubodera@nuc003.psc.sc.edu>, MILLER@nucthy.phys.washington.edu, "Stephen A. Wood" <saw@jlab.org>, Vijay Pandharipande <vijay@bethe.physics.uiuc.edu>, "E.A. Paschos" <paschos@physik.uni-dortmund.de>, Giampaolo Co <Giampaolo.Co@le.infn.it>, Jacques Marteau <marteau@in2p3.fr>, martinez@quasar.physik.unibas.ch, Hiroki Nakamura <naka@barbara.hep.phys.waseda.ac.jp>, paolo lipari <Paolo.Lipari@roma1.infn.it>, "S.K. Singh" <sk_singh@bharatmail.com> cc: opc.nuint01@neutrino.kek.jp Subject: NuTev result Message-ID: <Pine.LNX.3.95LJ1.1b3.1011205100136.3710D-100000@neutrino.kek.jp> Dear the panel discussion leaders and the theory benchmarkers, The NuTeV collaboration has recently reported (hep-ex/0110059) the EW parameter \sin^2 \theta_W found to be 3 sd above the standard model prediction. Some have raised a question, whether this could have a nuclear physics origin. We are trying to see whether we could arrange a time for discussion of this issue during NuInt01 workshop. As expertise of various issues in neutrino-nucleus or related physics, I thought you may find this interesting or may wish to contribute comments to it, and thus I should inform you just in the case that you should not be aware of it. Will see you at KEK next week. Best wishes, Seki
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