In recent papers it has been observed that non-Hermitian Hamiltonians, such
as those describing ig phi (3) and -g phi (4) field theories, still posses
s real positive spectra so long as the weaker condition of PT symmetry hold
s. This allows for the possibility of new kinds of quantum field theories t
hat have strange and quite unexpected properties. In this paper a technique
based on truncating the Schwinger-Dyson equations is presented for renorma
lizing and solving such field theories. Using this technique if is argued t
hat a -g phi (4) scalar quantum field theory in four-dimensional space-time
is renormalizable, is asymptotically free, has a nonzero value of [0\phi \
0], and has a positive definite spectrum. Such a theory might be useful in
describing the Higgs boson.