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We determine the value of the omega -rho- pi mesons coupling (g_{omegarhopi}), in the context of the vector meson dominance model, from radiative decays, the omega rightarrow 3pi decay width and the e^+e^- rightarrow 3pi cross section. For the last two observables we consider the effect of either a heavier resonance (rho(1450)) or a contact term. A weighted average of the results from the set of observables yields g_{omegarhopi} =14.7 pm 0.1 GeV^{-1} in absence of those contributions, and g_{omegarhopi} =11.9 pm 0.2 GeV^{-1} or g_{omegarhopi} =11.7 pm 0.1 GeV^{-1} when including the rho or contact term respectively. The inclusion of these additional terms makes the estimates from the different observables to lay in a more reduced range. Improved measurements of these observables and the rho(1450) meson parameters are needed to give a definite answer on the pertinence of the inclusion of this last one in the considered processes.
We analyze the most recent data for the pion vector form factor in the timelike region, employing a model-independent approach based on dispersion theory. We confirm earlier observations about the inconsistency of different modern high-precision data
We study possible contributions to the Ds^+ -> omega pi^+ and Ds^+ -> rho^0 pi^+ decay amplitudes. The Ds^+ -> omega pi^+ decay amplitude vanishes when the naive factorization is used, while the Ds^+ -> rho^0 pi^+ decay amplitude arises due to the an
Theoretical errors in the extraction of alpha from B -> pi^+ pi^-, rho^+ rho^-, rho pi decays are usually given in terms of upper bounds on alpha_eff-alpha obtained from isospin or from SU(3) relations, where alpha_eff is measured through CP asymmetr
The investigation in the work of the reaction electron-positron to omega and pi0 mesons in the 3P0 nonrelativistic quark model reveals that the reaction electron-positron to omega and pi0 mesons process at the energy region from the omega and pi meso
Simulation methods for the decays $ B to {pi}^+ {pi}^- V$, where $V$ is a $1^{--}$ vector-meson, are presented in detail. Emphasis is put on the use of the helicity formalism and the use of effective Lagrangians. We show the importance of ${{rho}^{0}