Abstract
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 BB¯ 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 Bsμ+μ branching ratio and BsBs mixing. For A10 masses above the tau threshold the A10 can be searched for in bsτ+τ processes with branching ratios 103.