Determining the sign of the b -> s gamma amplitude

dc.creatorGambino, Paolo
dc.creatorHaisch, Ulrich
dc.creatorMisiak, Mikolaj
dc.date2004-10-11
dc.date2005-02-14
dc.date.accessioned2026-07-07T11:43:30Z
dc.date.available2026-07-07T11:43:30Z
dc.descriptionThe latest Belle and BaBar measurements of the inclusive B -> X_s l^+ l^- branching ratio have smaller errors and lower central values than the previous ones. We point out that these results indicate that the sign of the b -> s gamma amplitude is the same as in the SM. This underscores the importance of B -> X_s l^+ l^- in searches for new physics, and may be relevant for neutralino dark matter analyses within the MSSM.
dc.descriptionJournal version, references added, minor modifications. 4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0410155
dc.identifierhttp://arxiv.org/abs/hep-ph/0410155
dc.identifierPhys.Rev.Lett.94:061803,2005
dc.identifierdoi:10.1103/PhysRevLett.94.061803
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201261
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Experiment
dc.titleDetermining the sign of the b -> s gamma amplitude
dc.typetext

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