B_{d,s}->rho, omega, K*, phi Decay Form Factors from Light-Cone Sum Rules Revisited

dc.creatorBall, Patricia
dc.creatorZwicky, Roman
dc.date2004-12-06
dc.date.accessioned2026-07-07T10:29:20Z
dc.date.available2026-07-07T10:29:20Z
dc.descriptionWe present an improved calculation of $B\to$ light vector form factors from light-cone sum rules, including one-loop radiative corrections to twist-2 and twist-3 contributions, and leading order twist-4 corrections. The total theoretical uncertainty of our results at zero momentum transfer is typically 10% and can be improved, at least in part, by reducing the uncertainty of hadronic input parameters. We present our results in a way which details the dependence of the form factors on these parameters and facilitates the incorporation of future updates of their values from e.g. lattice calculations. We also give simple and easy-to-inplement parametrizations of the $q^2$-dependence of the form factors which are valid in the full kinematical regime of $q^2$.
dc.description44 pages
dc.identifierhttps://arxiv.org/abs/hep-ph/0412079
dc.identifierhttp://arxiv.org/abs/hep-ph/0412079
dc.identifierPhys.Rev.D71:014029,2005
dc.identifierdoi:10.1103/PhysRevD.71.014029
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177765
dc.subjectHigh Energy Physics - Phenomenology
dc.titleB_{d,s}->rho, omega, K*, phi Decay Form Factors from Light-Cone Sum Rules Revisited
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