will appear below.

To find the classical moduli space of the theory one should first impose the D-flatness equations and mod out by gauge transformations. This is equivalent to moding out the space of chiral fields by $SU(N_c)_{\IC}$. Using this symmetry we can diagonalize $X$ and then impose the equation of motion from . The eigenvalues of $X$ must satisfy $W^\prime(x)=0$. For generic couplings $\{s_i\}$ there are $k$ distinct solutions $c_1,\cdots, c_k$. Vacua of the gauge theory are labeled by sequences of integers $(r_1, r_2, \cdots, r_k)$; $r_l$ is the number of eigenvalues of the matrix $\langle X\rangle$ residing in the $l$’th minimum of the potential. The gauge group is broken by the $X$ expectation value: At low energies the theory describes $k$ decoupled supersymmetric QCD (SQCD) systems with gauge groups $SU(r_l)$ and gauged baryon number. For a given choice of $\{r_l\}$ there is a moduli space of vacua associated with giving expectation values to the quarks. Therefore, the classical moduli space consists of many disconnected components parametrized by the $\{r_i\}$. One can fine tune the couplings such that some of the eigenvalues $\{c_i\}$ coincide. The resulting multicritical behavior will be analyzed in section [*2*]{}.

Quantum mechanically, not all vacua 