dc.contributor.author | Ammar, Raymond G. | |
dc.contributor.author | Ball, S. | |
dc.contributor.author | Baringer, Philip S. | |
dc.contributor.author | Bean, Alice | |
dc.contributor.author | Besson, David Zeke | |
dc.contributor.author | Coppage, Don | |
dc.contributor.author | Copty, N. | |
dc.contributor.author | Davis, Robin E. P. | |
dc.contributor.author | Hancock, N. | |
dc.contributor.author | Kelly, M. | |
dc.contributor.author | Kwak, Nowhan | |
dc.contributor.author | Lam, H. | |
dc.date.accessioned | 2007-04-13T21:12:44Z | |
dc.date.available | 2007-04-13T21:12:44Z | |
dc.date.issued | 1994-03 | |
dc.identifier.citation | CINABRO, D, HENDERSON, S, et al. Observation of D(0) → K+pi-. PHYSICAL REVIEW LETTERS. March 1994. 72(10) : 1406-1410 | |
dc.identifier.uri | http://hdl.handle.net/1808/1438 | |
dc.description.abstract | Using the CLEO II data sample, with an integrated luminosity of 1.8 fb-1 at and near the UPSILON(4S) resonance, we have observed a signal for D0 --> K+pi-, which could be due to either D0D0BAR mixing or doubly Cabibbo suppressed decay, or a combination of the two. We find B(D0 --> K+pi-)/B(D0 --> K- pi+)= 0.0077 +/- 0.0025 (stat) +/- 0.0025 (syst). | |
dc.language.iso | en_US | |
dc.publisher | AMERICAN PHYSICAL SOC | |
dc.relation.isversionof | http://publish.aps.org/ | |
dc.title | Observation of D(0) → K+pi- | |
dc.type | Article | |
dc.rights.accessrights | openAccess | |