Predictions for B→KγγB \to K γγ decays

preprint2011arXivOpen access

Abstract

We present a phenomenological study of the rare double radiative decay B→KγγB\to K γγ in the Standard Model (SM) and beyond. Using the operator product expansion (OPE) technique, we estimate the short-distance (SD) contribution to the decay amplitude in a region of the phase space which is around the point where all decay products have energy ∼mb/3\sim m_b/3 in the rest frame of the BB-meson. At lowest order in 1/Q, where QQ is of order mbm_b, the B→KγγB\to K γγ matrix element is then expressed in terms of the usual B→KB\to K form factors known from semileptonic rare decays. The integrated SD branching ratio in the SM in the OPE region turns out to be ΔB(B→Kγγ)SMOPE≃1×10−9Δ{\cal{B}}(B \to K γγ)_{SM}^{OPE} \simeq 1 \times 10^{-9}. We work out the di-photon invariant mass distribution with and without the resonant background through B→K{ηc,χc0}→KγγB\to K \{η_c,χ_{c0}\}\to Kγγ. In the SM, the resonance contribution is dominant in the region of phase space where the OPE is valid. The present experimental upper limit on Bs→τ+τ−B_s \to τ^+ τ^- decays, which constrains the scalar/pseudoscalar Four-Fermi operators with τ+τ−τ^+ τ^-, leaves considerable room for new physics in the one-particle-irreducible contribution to B→KγγB\to K γγ decays. In this case, we find that the SD B→KγγB\to K γγ branching ratio can be enhanced by one order of magnitude with respect to its SM value and the SD contribution can lie outside of the resonance peaks.

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