Charm production in nonresonante+e−annihilations at√s =10.55 GeV

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ID: 270648
1988
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Abstract
We report results on the differential and total cross sections for inclusive production of the charmed particles D*+, D*0, D0, D+, Ds, and Λc in e+e− annihilations at √s=10.55 GeV. Widely used quark fragmentation models are discussed and compared with the measured charmed-particle momentum distributions. This comparison, as well as that with measurements at other center-of-mass energies, shows the need to take QCD corrections into account and their importance for a correct interpretation of the model parameters. The observed rate of D0 and D+ production is compared to the expected total charm production cross section. We measure the probability of a charmed meson being produced as a vector meson and the D*+ decay branching fraction into D0π+.
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Authors D. Bortoletto,M. Goldberg,R. Holmes,N. Horwitz,A. Jawahery,P. Lubrano,G. C. Moneti,V. Sharma,I. P. J. Shipsey,P. Thoma,S. E. Csorna,T. Letson,M. D. Mestayer,R. S. Panvini,G. B. Word,Alice Bean,G. J. Bobbink,I. C. Brock,T. Ferguson,R. W. Kraemer,H. Vogel,C. Bebek,K. Berkelman,E. Blucher,D. G. Cassel,T. Copie,R. DeSalvo,J. W. DeWire,R. Ehrlich,R. S. Galik,M. G. D. Gilchriese,B. Gittelman,S. W. Gray,A. M. Halling,D. L. Hartill,B. K. Heltsley,S. Holzner,J. Kandaswamy,Robert Kowalewski,D. L. Kreinick,Y. Kubota,N. B. Mistry,James Mueller,R. Namjoshi,E. Nordberg,D. Perticone,D. Peterson,M. Pisharody,Kenneth Read,D. Riley,A. Silverman,Sheldon Stone,A. J. Sadoff,P. Avery,D. Besson,L. Garren,Themistocles Bowcock,K. Kinoshita,F. M. Pipkin,M. Procario,Richard Wilson,J. Wolinski,D. Xiao,P. Haas,M. Hempstead,T. Jensen,D. R. Johnson,H. Kagan,R. Kass,P. Baringer,R. L. McIlwain,D. H. Miller,E. I. Shibata,S. Behrends,Jan M. Guida,Joan A. Guida,F. Morrow,Ronald Poling,E. H. Thorndike,P. Tipton,M. S. Alam,N. Katayama,I. J. Kim,W. C. Li,X. C. Lou,C. R. Sun,V. Tanikella;D. Bortoletto;M. Goldberg;R. Holmes;N. Horwitz;A. Jawahery;P. Lubrano;G. C. Moneti;V. Sharma;I. P. J. Shipsey;P. Thoma;S. E. Csorna;T. Letson;M. D. Mestayer;R. S. Panvini;G. B. Word;Alice Bean;G. J. Bobbink;I. C. Brock;T. Ferguson;R. W. Kraemer;H. Vogel;C. Bebek;K. Berkelman;E. Blucher;D. G. Cassel;T. Copie;R. DeSalvo;J. W. DeWire;R. Ehrlich;R. S. Galik;M. G. D. Gilchriese;B. Gittelman;S. W. Gray;A. M. Halling;D. L. Hartill;B. K. Heltsley;S. Holzner;J. Kandaswamy;Robert Kowalewski;D. L. Kreinick;Y. Kubota;N. B. Mistry;James Mueller;R. Namjoshi;E. Nordberg;D. Perticone;D. Peterson;M. Pisharody;Kenneth Read;D. Riley;A. Silverman;Sheldon Stone;A. J. Sadoff;P. Avery;D. Besson;L. Garren;Themistocles Bowcock;K. Kinoshita;F. M. Pipkin;M. Procario;Richard Wilson;J. Wolinski;D. Xiao;P. Haas;M. Hempstead;T. Jensen;D. R. Johnson;H. Kagan;R. Kass;P. Baringer;R. L. McIlwain;D. H. Miller;E. I. Shibata;S. Behrends;Jan M. Guida;Joan A. Guida;F. Morrow;Ronald Poling;E. H. Thorndike;P. Tipton;M. S. Alam;N. Katayama;I. J. Kim;W. C. Li;X. C. Lou;C. R. Sun;V. Tanikella;
Journal physical review d
Year 1988
DOI
10.1103/physrevd.37.1719
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