Knowledge of the form factors at the zero-recoil point is crucial to extract the element of the Cabbibo-Kobayashi-Maskawa matrix that parameterizes the amount of mixing between the b and c quarks, , from experiment. In the limit that the heavy quarks are infinitely heavy, heavy quark effective theory (HQET) predicts that the form factors , , and are equal. The formally dominant correction due to breaking of heavy quark symmetry comes from the inclusion of a dimension-three operator in the Lagrangian that leads to hyperfine-splitting between the heavy pseudoscalar and vector mesons. These leading order corrections are as required by Luke's theorem. Recent lattice simulations using the quenched approximation of QCD have made a big step forward in determining these zero-recoil form factors. Presently, however, the simulations use light quark masses that are much heavier than the physical ones and therefore rely on a chiral extrapolation down to the physical quark masses.
In this work we calculate the dominant corrections to the form factors , , and in quenched chiral perturbation theory (QPT) and determine the non-analytic dependence on the light quark masses. Using these results to extrapolate the quenched QCD lattice measurements of these form factors down to the physical pion mass should give a more reliable estimate of the errors associated with the chiral extrapolation.