A reanalysis of B0-B̄0 mixing in e+e− annihilation at 29 GeV
Clicks: 106
ID: 272038
1990
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 |
URL | |
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