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 (Q
PT)
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.