  The ability to now make measurements of Be and B as well as put constraints
on \lisix\ abundances in metal-poor stars has led to a detailed reexamination
of Big Bang Nucleosynthesis in the $A\groughly6$ regime. The nuclear reaction
network has been significantly expanded with many new rates added. It is
demonstrated that although a number of $A>7$ reaction rates are poorly
determined, even with extreme values chosen, the standard homogeneous model is
unable to produce significant yields (Be/H and B/H $<10^{-17}$ when $A\le7$
abundances fit) above $A=7$ and the \liseven/\lisix\ ratio always exceeds 500.
We also preliminarily explore inhomogeneous models, such as those inspired by a
first order quark-hadron phase transition, where regions with high
neutron/proton ratios can allow some leakage up to $A>7$. However models that
fit the $A\le7$ abundances still seem to have difficulty in obtaining
significant $A>7$ yields.
