Radiative B decays to the axial mesons at next-to-leading order
arXiv:hep-ph/0403034 · doi:10.1103/PhysRevD.69.114007
Abstract
We calculate the branching ratios of at next-to-leading order (NLO) of where is the orbitally excited axial vector meson. The NLO decay amplitude is divided into the vertex correction and the hard spectator interaction part. The one is proportional to the weak form factor of transition while the other is a convolution between light-cone distribution amplitudes and hard scattering kernel. Using the light-cone sum rule results for the form factor, we have $\calB(B^0\to K_1^0(1270)γ)=(0.828\pm0.335)\times 10^{-5}$ and $\calB(B^0\to K_1^0(1400)γ)=(0.393\pm0.151)\times 10^{-5}$.
17pages, 4 figures. Minor changes, typos corrected. PRD accepted version
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- Implications of the first observation of
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- Branching ratio for B -> K_1 gamma decay in next-to-leading order in LEET
- Annihilation Contributions in B -> K_1 gamma decay in next-to-leading order in LEET and CP-asymmetry
- Radiative to axial-vector meson decays at NLO in Soft-Collinear Effective Theory
- Branching Ratio and CP-asymmetry for B-> 1^{1}P_{1}gamma decays
- Mass relations among family members of quarks and leptons