  High energy solar neutrinos can come from the hep reaction ^3He(p,\nue^+)^4He
with a large end point energy of 18.8 MeV. Understanding the hep reaction may
be important for interpreting solar neutrino spectra. We calculate the
contribution of the axial charge transition $^3P_0\to ^1S_0$ to the hep
thermonuclear S factor using a one-body reaction model involving a nucleon
moving in optical potentials. Our result is comparable to or larger than
previous calculations of the s-wave Gamow Teller contribution. This indicates
that the hep reaction may have p-wave strength leading to an enhancement of the
S factor.
