An alternative fit to Belle mass spectra for DD, D*D* and Lambda_C Lambda_c
| dc.creator | Bugg, D. V. | |
| dc.date | 2008-11-16 | |
| dc.date | 2009-01-11 | |
| dc.date.accessioned | 2026-07-07T13:16:17Z | |
| dc.date.available | 2026-07-07T13:16:17Z | |
| dc.description | Peaks observed by Belle in DD at 3.878 GeV and in D*D* at 4.156 GeV may be fitted by phase space multiplied by a form factor with an RMS radius of interaction 0.63 fm. The peak observed in Lambda_C Lambda_C at 4.63 GeV may be explained by Y(4660), multiplied by a corresponding form factor with RMS radius 0.94 fm. | |
| dc.description | 3 pages, 1 figures Shorted version, conclusions unchanged | |
| dc.identifier | https://arxiv.org/abs/0811.2559 | |
| dc.identifier | http://arxiv.org/abs/0811.2559 | |
| dc.identifier | J.Phys.G36:075002,2009 | |
| dc.identifier | doi:10.1088/0954-3899/36/7/075002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/230741 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | An alternative fit to Belle mass spectra for DD, D*D* and Lambda_C Lambda_c | |
| dc.type | text |