Radiative $B\to K_1$ decays in the light-cone sum rules
| dc.creator | Lee, Jong-Phil | |
| dc.date | 2006-08-08 | |
| dc.date.accessioned | 2026-07-07T10:25:16Z | |
| dc.date.available | 2026-07-07T10:25:16Z | |
| dc.description | The weak form factor for $B\to K_{1B}$ where $K_{1B}$ is the $^1P_1$ state is calculated in the light-cone sum rules (LCSR). Combining the quark model result for the form factor of $B\to K_{1A}$ with $K_{1A}$ being the $^3P_1$ state, we have larger values for $B\to K_1$ form factors than the previous LCSR results. The increased form factors reduce the discrepancy between theory and the experimental data for $B\to K_1 γ$. Some phenomenological meanings are also discussed. | |
| dc.description | 15 pages, 4 figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0608087 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0608087 | |
| dc.identifier | Phys.Rev.D74:074001,2006 | |
| dc.identifier | doi:10.1103/PhysRevD.74.074001 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/176480 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Radiative $B\to K_1$ decays in the light-cone sum rules | |
| dc.type | text |