| dc.contributor.author | Ammar, Raymond G. | |
| 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 | Darling, C. | |
| dc.contributor.author | Davis, Robin E. P. | |
| dc.contributor.author | Kotov, S. | |
| dc.contributor.author | Kravchenko, I. | |
| dc.contributor.author | Kwak, Nowhan | |
| dc.contributor.author | Zhou, L. | |
| dc.date.accessioned | 2007-04-11T21:13:42Z | |
| dc.date.available | 2007-04-11T21:13:42Z | |
| dc.date.issued | 1998-05 | |
| dc.identifier.citation | Bartelt, J, Csorna, SE, et al. Observation of the radiative decay D*+-> D+gamma. AMERICAN PHYSICAL SOC. May 1998. 80(18) 3919-1923 | |
| dc.identifier.other | http://publish.aps.org/ | |
| dc.identifier.uri | http://hdl.handle.net/1808/1362 | |
| dc.description.abstract | We have observed a signal for the decay D*(+) --> D(+)gamma at a significance of 4 standard deviations. From the measured branching ratio B(D*(+) --> D(+)gamma)/B(D*(+) --> D(+)pi(0)) = 0.055 +/- 0.014 +/- 0.010 we find B(D*(+) --> D(+)gamma) = 0.017 +/- 0.004 +/- 0.003, where the first uncertainty is statistical and the second is systematic. We also report the highest precision determination of the remaining D*(+) branching fractions. | |
| dc.language.iso | en_US | |
| dc.publisher | AMERICAN PHYSICAL SOC | |
| dc.title | Observation of the radiative decay D*+-> D+gamma | |
| dc.type | Article | |
| dc.rights.accessrights | openAccess | |
