Bose-Fermi Cancellation of Cosmological Coleman-Weinberg Potentials
  Cosmological Coleman-Weinberg potentials are induced when normal matter is
coupled to the inflaton. It has long been known that the corrections from
bosonic fields are positive whereas those from fermionic fields are negative.
In flat space both take the form $\pm \varphi^4 \ln(\varphi)$, and they can be
made to cancel by appropriately choosing the coupling constants. In an
expanding universe the bosonic and fermionic results no longer take the same
form, although their large field limits do. We choose the coupling constants so
that the large field limits cancel, and then follow the deviations which result
as inflation progresses. Although the result is not satisfactory we discuss how
adding scalars with various conformal couplings likely solves the problem.
