  In the standard model, energy release in dense stars is severely restricted
by the Pauli exclusion principle. However, if, in regions of space of high
fermion degeneracy, there is a phase transition to a state of exact
supersymmetry (SUSY), fermion to sfermion pair conversion followed by radiative
transitions to the Bose ground state could lead to a highly collimated gamma
ray burst. We calculate the cross section for electron to selectron pair
conversion in a SUSY bubble and construct a monte carlo for the resulting
sfermion amplification by stimulated emission.
