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

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ID: 272038
1990
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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.
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Authors A.J. Weir,G. Abrams,C.E. Adolphsen,J.P. Alexander,M. Alvarez,D. Amidei,A.R. Baden,B.C. Barish,T. Barklow,B.A. Barnett,I. Bartelt,D. Blockus,G. Bonvicini,A. Boyarski,J. Boyer,B. Brabson,A. Breakstone,J.M. Brom,F. Bulos,P.R. Burchat,D.L. Burke,F. Butler,Francisco Calvino,R.J. Cence,J. Chapman,D. Cords,D.P. Coupal,H.C. Destaebler,D.E. Dorfan,J.M. Dorfan,P.S. Drell,G.J. Feldman,E. Fernandez,R.C. Field,W.T. Ford,C. Fordham,Raymond Frey,D. Fujino,K.K. Gan,G. Gidal,L. Gladney,T. Glanzman,M.S. Gold,G. Goldhaber,A. Green,P. Grosse-Wiesmann,J. Haggerty,G. Hanson,R. Harr,F.A. Harris,C.M. Hawkes,K. Hayes,D. Herrup,C.A. Heusch,T. Himel,R.J. Hollebeek,D. Hutchinson,J. Hylef,W.R. Innes,M. Jaffre,J.A. Jaros,I. Juricic,J.A. Kadyk,Dean Karlen,J. Kent,Spencer Klein,W. Koska,W. Kozanecki,A.J. Lankford,R.R. Larsen,B.W. LeClaire,M.E. Levi,A.M. Litke,N.S. Lockyer,V. Lüth,J.A.J. Matthews,D.I. Meyer,B.D. Milliken,K.C. Moffeit,L. Müller,Jordan Nash,M.E. Nelson,D. Nitz,H. Ogren,R.A. Ong,K.F. O'Shaughnessy,S.I. Parker,C. Peck,M.L. Perl,A. Petersen,M. Petradza,F.C. Porter,P. Rankin,B. Richter,K. Riles,P.C. Rowson,D.R. Rust,Hartmut Sadrozinski,T. Schaad,T.L. Schalk,H. Schellman,W.B. Schmidke,A.S. Schwarz,A. Seiden,P.D. Sheldon,J.G. Smith,A. Snyder,E. Soderstrom,D.P. Stoker,R. Stroynowski,R. Thun,G.H. Trilling,R. Tschirhart,R. Van Kooten,H. Veltman,P. Voruganti,S.R. Wagner,P. Weber,A.J. Weinstein,S. Weisz,S.L. White,E. Wicklund,D.R. Wood,D.Y. Wu,J.M. Yelton;A.J. Weir;G. Abrams;C.E. Adolphsen;J.P. Alexander;M. Alvarez;D. Amidei;A.R. Baden;B.C. Barish;T. Barklow;B.A. Barnett;I. Bartelt;D. Blockus;G. Bonvicini;A. Boyarski;J. Boyer;B. Brabson;A. Breakstone;J.M. Brom;F. Bulos;P.R. Burchat;D.L. Burke;F. Butler;Francisco Calvino;R.J. Cence;J. Chapman;D. Cords;D.P. Coupal;H.C. Destaebler;D.E. Dorfan;J.M. Dorfan;P.S. Drell;G.J. Feldman;E. Fernandez;R.C. Field;W.T. Ford;C. Fordham;Raymond Frey;D. Fujino;K.K. Gan;G. Gidal;L. Gladney;T. Glanzman;M.S. Gold;G. Goldhaber;A. Green;P. Grosse-Wiesmann;J. Haggerty;G. Hanson;R. Harr;F.A. Harris;C.M. Hawkes;K. Hayes;D. Herrup;C.A. Heusch;T. Himel;R.J. Hollebeek;D. Hutchinson;J. Hylef;W.R. Innes;M. Jaffre;J.A. Jaros;I. Juricic;J.A. Kadyk;Dean Karlen;J. Kent;Spencer Klein;W. Koska;W. Kozanecki;A.J. Lankford;R.R. Larsen;B.W. LeClaire;M.E. Levi;A.M. Litke;N.S. Lockyer;V. Lüth;J.A.J. Matthews;D.I. Meyer;B.D. Milliken;K.C. Moffeit;L. Müller;Jordan Nash;M.E. Nelson;D. Nitz;H. Ogren;R.A. Ong;K.F. O'Shaughnessy;S.I. Parker;C. Peck;M.L. Perl;A. Petersen;M. Petradza;F.C. Porter;P. Rankin;B. Richter;K. Riles;P.C. Rowson;D.R. Rust;Hartmut Sadrozinski;T. Schaad;T.L. Schalk;H. Schellman;W.B. Schmidke;A.S. Schwarz;A. Seiden;P.D. Sheldon;J.G. Smith;A. Snyder;E. Soderstrom;D.P. Stoker;R. Stroynowski;R. Thun;G.H. Trilling;R. Tschirhart;R. Van Kooten;H. Veltman;P. Voruganti;S.R. Wagner;P. Weber;A.J. Weinstein;S. Weisz;S.L. White;E. Wicklund;D.R. Wood;D.Y. Wu;J.M. Yelton;
Journal physics letters b
Year 1990
DOI
10.1016/0370-2693(90)90447-e
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