Estimate of BR(B -> X_s gamma) at O(alpha_s^2)
| dc.creator | Misiak, M. | |
| dc.creator | Asatrian, H. M. | |
| dc.creator | Bieri, K. | |
| dc.creator | Czakon, M. | |
| dc.creator | Czarnecki, A. | |
| dc.creator | Ewerth, T. | |
| dc.creator | Ferroglia, A. | |
| dc.creator | Gambino, P. | |
| dc.creator | Gorbahn, M. | |
| dc.creator | Greub, C. | |
| dc.creator | Haisch, U. | |
| dc.creator | Hovhannisyan, A. | |
| dc.creator | Hurth, T. | |
| dc.creator | Mitov, A. | |
| dc.creator | Poghosyan, V. | |
| dc.creator | Slusarczyk, M. | |
| dc.creator | Steinhauser, M. | |
| dc.date | 2006-09-22 | |
| dc.date | 2006-12-31 | |
| dc.date.accessioned | 2026-07-07T11:05:46Z | |
| dc.date.available | 2026-07-07T11:05:46Z | |
| dc.description | Combining our results for various O(alpha_s^2) corrections to the weak radiative B-meson decay, we are able to present the first estimate of the branching ratio at the next-to-next-to-leading order in QCD. We find BR(B -> X_s gamma) = (3.15 +_ 0.23) x 10^-4 for E_gamma > 1.6 GeV in the B-meson rest frame. The four types of uncertainties: non-perturbative (5%), parametric (3%), higher-order (3%) and m_c-interpolation ambiguity (3%) have been added in quadrature to obtain the total error. | |
| dc.description | 4 pages, 4 figures. Version accepted by the PRL. Words disallowed by the journal removed from the title. References updated and a note added | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0609232 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0609232 | |
| dc.identifier | Phys.Rev.Lett.98:022002,2007 | |
| dc.identifier | doi:10.1103/PhysRevLett.98.022002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/189308 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Estimate of BR(B -> X_s gamma) at O(alpha_s^2) | |
| dc.type | text |