We investigate the low energy phenomenology of the lighter pseudoscalar A₁⁰ in the NMSSM. The A₁⁰ mass can naturally be small due to a global U(1)R symmetry of the Higgs potential, which is only broken by trilinear soft terms. The A₁⁰ mass is further protected from renormalization group effects in the large tanβ limit. We calculate the →bsA₁⁰ amplitude at leading order in tanβ and work out the contributions to rare K, B and radiative Υ decays and B-B̄ mixing. We obtain constraints on the A₁⁰ mass and couplings and show that masses down to O(10) MeV are allowed. The b-physics phenomenology of the NMSSM differs from the MSSM in the appearance of sizable renormalization effects from neutral Higgs bosons to the photon and gluon dipole operators and the breakdown of the MSSM correlation between the Bₛ→μ⁺μ^- branching ratio and Bₛ-Bₛ mixing. For A₁⁰ masses above the tau threshold the A₁⁰ can be searched for in →bsτ⁺τ^- processes with branching ratios 10^-3.
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Gudrun Hiller (2004) studied this question.
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