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

doi:10.1016/0370-2693(90)90447-e

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

1990

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;
Schellman, H;
Schmidke, WB;
Schwarz, AS;
Seiden, A;
Sheldon, PD;
Smith, JG;
Snyder, A;
Soderstrom, E;
Stoker, DP;
Stroynowski, R;
Thun, R;
Trilling, GH;
Tschirhart, R;
Van Kooten, R;
Veltman, H;
Voruganti, P;
Wagner, SR;
Weber, P;
Weinstein, AJ;
Weisz, S;
White, SL;
Wicklund, E;
Wood, DR;
Wu, DY;
Yelton, JM
et al.

Published Web Location

https://doi.org/10.1016/0370-2693(90)90447-e

Creative Commons 'BY' version 4.0 license

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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UC Irvine

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

Published Web Location