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A reanalysis of B0-B̄0 mixing in e+e- annihilation at 29 GeV

  • Author(s): Weir, AJ;
  • Abrams, G;
  • Adolphsen, CE;
  • Alexander, JP;
  • Alvarez, M;
  • Amidei, D;
  • Baden, AR;
  • Barish, BC;
  • Barklow, T;
  • Barnett, BA;
  • Bartelt, I;
  • Blockus, D;
  • Bonvicini, G;
  • Boyarski, A;
  • Boyer, J;
  • Brabson, B;
  • Breakstone, A;
  • Brom, JM;
  • Bulos, F;
  • Burchat, PR;
  • Burke, DL;
  • Butler, F;
  • Calvino, F;
  • Cence, RJ;
  • Chapman, J;
  • Cords, D;
  • Coupal, DP;
  • Destaebler, HC;
  • Dorfan, DE;
  • Dorfan, JM;
  • Drell, PS;
  • Feldman, GJ;
  • Fernandez, E;
  • Field, RC;
  • Ford, WT;
  • Fordham, C;
  • Frey, R;
  • Fujino, D;
  • Gan, KK;
  • Gidal, G;
  • Gladney, L;
  • Glanzman, T;
  • Gold, MS;
  • Goldhaber, G;
  • Green, A;
  • Grosse-Wiesmann, P;
  • Haggerty, J;
  • Hanson, G;
  • Harr, R;
  • Harris, FA;
  • Hawkes, CM;
  • Hayes, K;
  • Herrup, D;
  • Heusch, CA;
  • Himel, T;
  • Hollebeek, RJ;
  • Hutchinson, D;
  • Hylef, J;
  • Innes, WR;
  • Jaffre, M;
  • Jaros, JA;
  • Juricic, I;
  • Kadyk, JA;
  • Karlen, D;
  • Kent, J;
  • Klein, SR;
  • Koska, W;
  • Kozanecki, W;
  • Lankford, AJ;
  • Larsen, RR;
  • LeClaire, BW;
  • Levi, ME;
  • Litke, AM;
  • Lockyer, NS;
  • Lüth, V;
  • Matthews, JAJ;
  • Meyer, DI;
  • Milliken, BD;
  • Moffeit, KC;
  • Müller, L;
  • Nash, J;
  • Nelson, ME;
  • Nitz, D;
  • Ogren, H;
  • Ong, RA;
  • O'Shaughnessy, KF;
  • Parker, SI;
  • Peck, C;
  • Perl, ML;
  • Petersen, A;
  • Petradza, M;
  • Porter, FC;
  • Rankin, P;
  • Richter, B;
  • Riles, K;
  • Rowson, PC;
  • Rust, DR;
  • Sadrozinski, HFW;
  • Schaad, T;
  • Schalk, TL
  • et al.
Abstract

Data taken by the Mark II detector at the PEP storage ring was used to measure the rate of dilepton production in multihadronic events produced by e+e- annihilation at √s=29 GeV. We determine the probability that a hadron initially containing a b (b̄) quark decays to a positive (negative) lepton to be 0.17-0.08+0.15, with 90% confidence level limits of 0.06 and 0.38. © 1990.

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