dc.contributor.author | Baringer, Philip S. | |
dc.contributor.author | Bortoletto, D. | |
dc.contributor.author | Goldberg, M. | |
dc.contributor.author | Holmes, R. | |
dc.contributor.author | Horwitz, N. | |
dc.contributor.author | Jawahery, A. | |
dc.contributor.author | Lubrano, P. | |
dc.contributor.author | Moneti, G. C. | |
dc.contributor.author | Sharma, V. | |
dc.contributor.author | Shipsey, I. P. J. | |
dc.contributor.author | Thoma, P. | |
dc.date.accessioned | 2014-10-08T18:06:06Z | |
dc.date.available | 2014-10-08T18:06:06Z | |
dc.date.issued | 1989-04-01 | |
dc.identifier.citation | Baringer, Philip S. et al. (1989). "Charm production in nonresonant e(+)e(-) annihilations at √s =10.55 GeV." Physical Review D, 1988(37):1719. http://dx.doi.org/10.1103/PhysRevD.37.1719 | |
dc.identifier.issn | 1550-7998 | |
dc.identifier.uri | http://hdl.handle.net/1808/15233 | |
dc.description | This is the publisher's version also available electronically from http://journals.aps.org/prd/abstract/10.1103/PhysRevD.37.1719 | |
dc.description.abstract | We report results on the differential and total cross sections for inclusive production of the charmed particles D*+, D*(0), D(0), D(+), D(s), 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 D(0) 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 D(0)π+. | |
dc.publisher | American Physical Society | |
dc.title | Charm production in nonresonant e(+)e(-) annihilations at √s =10.55 GeV | |
dc.type | Article | |
kusw.kuauthor | Baringer, Philip S. | |
kusw.kudepartment | Physics and Astronomy | |
kusw.oanotes | Per SHERPA/RoMEO 10/08/2014: Link to publisher version required. Publisher copyright and source must be acknowledged with citation. Author's Post-print on author's personal website, employers website, institutional repository or e-print server. Publisher's version/PDF can be used on author's personal website, employers website or institutional repository. Publisher's version/PDF cannot be used on "e-print servers" or shared repositories | |
dc.identifier.doi | 10.1103/PhysRevD.37.1719 | |
kusw.oaversion | Scholarly/refereed, publisher version | |
kusw.oapolicy | This item does not meet KU Open Access policy criteria. | |
dc.rights.accessrights | openAccess | |