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It has been shown in ref. (8), that within the vector meson dominance approximation, the current mixing model is the only theory of ω-ϕ mixing which is compatible with the generalized first sum rule of Weinberg.
Our notation for the ω-ϕ mixing angles follows the one in ref. (7).
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We have written down only the superconvergence relations we are interested in. In particular our relations are independent of whether or not an X-meson plays an important role (SeeA. Baracca andA. Bramon:Nuovo Cimento,51 A, 873 (1967).)
The following masses were used in the calculations:m ρ=780 MeV,m ω=783 MeV,m ϕ=1018 MeV,m η=549 MeV.
The relationf πρϕ=0 was used.
The numerical factor 11.5·10−2 MeV in eq. (13) comes from the integration over the phase-space in the three-body final state.
The lower-sign solution in eq. (14) may also be rejected because of the fact that it is in violent disagreement with present experimental information. It gives for the experimental valueR=0.147±0.022 that Γ(η→2γ)≃1/50 keV.
The stated errors in eqs. (17) and (17′) correspond to the assumption that relations (1), (2), (2′) and (4) are exact.
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This work has been supported in part by U.S. Atomic Energy Commission, Contract No. AT (11-1)-264.
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Gounaris, G.J. Meson decays in brokenSU 3 . Nuovo Cimento A (1965-1970) 53, 565–570 (1968). https://doi.org/10.1007/BF02800136
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DOI: https://doi.org/10.1007/BF02800136