Radiative decays and the nature of heavy quarkonium
We argue that the photon spectra in radiative decays of various heavy quarkonium states provide important information on their nature. If two of these states are in the strong coupling regime, we are able to produce a parameter-free model-independent formula, which holds at next-to-leading order and...
| Autores: | , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2006 |
| País: | España |
| Institución: | Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya) |
| Repositorio: | Recercat. Dipósit de la Recerca de Catalunya |
| OAI Identifier: | oai:recercat.cat:2445/12842 |
| Acceso en línea: | https://hdl.handle.net/2445/12842 |
| Access Level: | acceso abierto |
| Palabra clave: | Partícules (Física nuclear) Fenomenologia (Física) Quarks Particles (Nuclear physics) Phenomenological theory (Physics) |
| Sumario: | We argue that the photon spectra in radiative decays of various heavy quarkonium states provide important information on their nature. If two of these states are in the strong coupling regime, we are able to produce a parameter-free model-independent formula, which holds at next-to-leading order and includes both direct and fragmentation contributions. When the formula is checked against recent CLEO data it favors Υ ( 2 S ) and Υ ( 3 S ) in the strong coupling regime and disfavors Υ ( 1 S ) in it. |
|---|